Wednesday, August 15, 2018

Nonlinear dynamic of clock mechanisms

Miőa D. Stojićević
Doctoral Dissertation
UNIVERSITY OF BELGRADE
FACULTY OF MECHANICAL ENGINEERING
Belgrade, 2018.

NOTE: Thesis was translated from Serbian to English using Google Translate and has not yet been corrected for any translation errors.

ABSTRACT: Clock mechanisms belongs in the field of precision mechanics, and they measures the flow of time with a precision uniformity of its work. A key subassembly of the clock mechanism is a escapement mechanism that, by its functions, creates disruptions in the oscillatory process so that the oscillations are no longer their own, but are forced with a frequency that is subjective to change. Therefore, the correct mathematical and physical description of the functioning of clock mechanisms cannot be correctly achieved by neglecting small disorders of higher order, linearization of differential equations and approximations common to the classical approach in the study of mechanisms.

The subject of the study of this dissertation are precisely these small disorders of higher order that occur in the escapement mechanism and undermine the uniformity of the work of the clock mechanism. Using the theory of perturbation, mathematical expressions for the calculation of errors are derived for two types of impulse mechanisms. The correctness of both these mathematical expressions and those general integral formulas was verified by computer simulation and the analysis of the motion of the 3D model of the corresponding escapement mechanisms. A qualitative and quantitative analysis of errors of the escapement mechanisms, i.e. frequency disturbances of the clock oscillator caused by their escapement mechanisms are presented. In addition to investigating the disturbance of the work of the escapement mechanism, the dissertation provides an overview of all the non-linear dynamic properties of the clock mechanism oscillator as well as a description of the parts of the clock that were used to simulate the clock. The numerical results of these simulations showed a high degree of agreement with the results of the theoretical numerical calculations, which confirmed the correctness of mathematical expressions performed using the perturbation calculus.

1. Introduction

1.1 The subject of research

Mechanisms of timers represent a real treasury of both theoretical and practical knowledge and skills from almost all fields of mechanical engineering, in particular theoretical mechanics and theories of mechanisms. Despite the fact that, in spite of this, the principles of their work, their constructive and functional characteristics, geometry, kinematics, analysis and synthesis are little studied in these disciplines, they can be the subject of numerous interesting and fruitful research. The results of such research can be significant, not only as recommendations for the correct synthesis of clock mechanisms, but also for theoretical disciplines such as kinematics, nonlinear dynamics, in particular the theory of nonlinear oscillations, mechanism theory, the science of machine elements and machine materials, etc. What's more, the results of these research can be extended and generalized to other fields of science, such as the theory of automatic control, the theory of deterministic chaos, celestial mechanics, the mathematical basics of the theory of perturbation account, and so on.

The fact is that clock mechanisms belong to areas of precision mechanics, which with a high degree of uniformity of their movement measures the flow of time [1], [2], and [3]. The slightest disturbances in the uniformity of their movement are the source of unacceptable inaccuracy of these mechanical instruments. For this reason, the correct mathematical and physical description of the functioning of clock mechanisms can not be achieved correctly by neglecting small disturbances by higher order linearizations of differential equations and approximations common to the classical approach in the study of mechanisms [4]. Such approximations would eliminate the essence of the dynamics of their work. In accordance with the prominent facts [5] and [6], the subject of the study of this work are precisely small disorders of higher order that impair the uniformity of the clock mechanism and thus generate errors in the measurement of the flow of time. In order to understand the effects of these small clock disturbances, it is necessary to carry out an analysis of its mechanism, which includes the classification of sub-assemblies and the functional analysis of each sub-assembly of the clock mechanism.

Essentially each clock mechanism consists of five sub-assemblies: a drive mechanism, a transmission mechanism, an oscillator, a movement regulator or a pulse mechanism and a cursor.

The focus of research on this dissertation will be the non-linear dynamic properties of the oscillators [7] and [8] and the impulse mechanisms [1], [9] and [10] as functionally the most important sub-assemblies of the clock mechanism. The characteristics of these sub-assemblies have a decisive influence on the behavior of the clock mechanism as a whole on the process of measuring the flow of time. A hypothetical view is that forced silenced oscillations of a clock mechanism such as a pendulum [11] or a spiral spring balancer [12] and [13] do not have a constant frequency, but that it suffers small disturbances [5] due to interaction with a mean-impulse mechanism. It is also assumed that the key factor of this disorder is the phase difference between the angular oscillation speed and the force of force that periodically affects the oscillator. A hypothetical view is that it is possible to carry out an analytical-algebraic expression for changing the frequency of forced oscillations of the clock oscillator using a perturbation account [14] and [2]. It is known that the piano watch is a physical pendulum whose oscillation period is not constant, but depends on the amplitude [8] and [15]. In addition, neither the spiral spring at the balance point of the timer has a constant stiffness coefficient [12], but it is a function of the angle of rotation of the oscillator. In accordance with the above, it is hypothesized that the intensity of the forced moment, the attenuation factor, that is, the quality factor of the oscillator and the oscillation amplitudes, have a significant effect on the uniformity of the clock travel. As the own frequency of oscillation of the clock oscillator (pendulum [7] or balancing point) depends on the geometric characteristics, the distribution of its masses and the moment of the inertia of the oscillator, it is reasonable to assume that the thermal dilatations [16] have a significant influence on the process of time measurement itself. It is also assumed that these thermal dilatations can be compensated by reducing their harmful effect or possibly eliminating them altogether [17].

One of the research goals in this doctoral dissertation is, first of all, to determine one or more of the suitable methods of perturbation [14] and [18] which would lead to general analytical formulas for changing the frequency of the oscillator due to its interaction with the impulse mechanism. The assumption is that these analytic expressions will be able to derive the use of commutative meanings by Krylov and Bogoliubov [14] and [18], as well as the method of multiple scales and the time scale [18].

Among the more important aims of this study is that the obtained general-formula formulates to a few typical types of impulse-based mechanisms and, if necessary, to classify them, depending on whether they increase or decrease their own frequency of the clock oscillator. Furthermore, it is important to verify the validity of these formulas by computer simulation and motion analysis, and thus verify not only the obtained analytical expressions, but also the methods of the perturbation account [14] and [18] used. In addition to the formal-mathematical and quantitative description, one of the goals of this paper is the physical and qualitative clarification of the phenomenon described above. One of the major research goals in this dissertation is the study of the effect of thermal dilatations on the frequency stability of the clock oscillator oscillations [16] and [17]. Accordingly, it is necessary to find suitable analytical and numerical methods, as well as computer modeling and simulation procedures to compensate for these harmful effects. One of the final goals of this doctoral dissertation is the synthesis and construction of a fully functional 3D computer clock model, including computer simulation and analysis of its work [19] and [20].


1.2 Scientific methods of research and expected results

In the process of realization of scientific results, in this doctoral dissertation the following general scientific methods were applied:

  • methods of differential and integral calculus,
  • numerical methods,
  • methods of computer modeling of forms,
  • methods of computer simulation and motion analysis.

In the process of realization of scientific results, in this doctoral dissertation the following special scientific methods were applied:

  • the method of perturbation account
  • the method of averaging according to the metric of the perturbation account
  • the method of multiple scales or the time scale,
  • Computer simulation method "Event based motion study" in the SolidWorks application.

1.3 Hypotheses

The linear oscillation theory shows that the frequency of compulsory damped oscillations is constant if the attenuation coefficient is constant. Empirical facts oppose the results of the linear theory of oscillations and find that the frequency of forced oscillations can be changed due to the interaction of the oscillator with the impulse mechanism. In this dissertation, it is assumed that the frequency of the clock oscillator (pendulum or balance point) depends on the phase difference between the angular oscillation speed and the forced force of the force that periodically affects the oscillator. Moreover, starting from the fact that the clock frequency oscillator's own frequency depends on its moment of inertia, it is assumed that the temperature dilatations have a significant effect on the said frequency. The assumption is that these influences can be reduced or completely eliminated by a suitable oscillator design. According to the prominent, the key starting hypotheses in this dissertation read as follows:

  • Using the perturbation method it is possible to perform analytical expressions for changing the frequency of forced oscillations of the clock oscillator due to its interaction with the impulse mechanism.
  • Analytical expressions for the change of the oscillator's own frequency due to its interaction with the impulse mechanism can be verified by computer simulation of forced silenced oscillations. It is also assumed that this verification will confirm the accuracy of the expressions obtained by the theory of the perturbation account.
  • It is possible to perform analytical procedures for compensating for the thermal dilation of the clock oscillator.
  • Iterative procedure for approximate compensation of the heat dilatations of the clock oscillator (pendulum) can be formulated and successfully using the appropriate computer application for 3D modeling. The methods of Krylov and Bogoliubov,
  • It is possible to achieve synthesis and generate a fully functional computer model of the clock mechanism and perform a successful computer simulation of his work.

1.4 Displays the chapters

Doctoral dissertation "Non-linear dynamics of clock mechanisms" is divided into 9 parts: introduction, 6 chapters and conclusion.

Chapter 2 "Theory of Time Measurement" shows a brief history of time measurement, in line with the modern definitions of the time measurement unit. It is shown that man recognized the need to have information about time in prehistory, observing the cycles of the Sun and the Moon. Then the first civilizations of ancient Egypt and Mesopotamia developed calendars. These calendars were used to predict the date of seasonal astronomical events essential for successful organization of the state and society. These civilizations gave the first division to sixty parts that remained to this day (clock is 60 minutes, minutes 60 seconds). Later, the civilizations of ancient Greece and Rome, are improving methods and devices for measuring the flow of time, so that the first solar and water clocks appear. The Middle Ages records the emergence of the first primitive mechanical monitors made by monks, of which the first records of the description of mechanical watches come to us. In the XVII century, the development of precise measurement of the flow of time begins and the transformation era begins - from timers that were so large that they could only be placed in towers to mechanisms that reduce the clock so that it can be worn on the hand. At the end of the chapter we give an overview of the development of a unit of time - from the first civilizations (who took the day as a natural and basic unit) to the modern age - where we can define a second over the radiation period in the atom of a cesium.

Chapter 3, "Theoretical Basics of the Perturbation Account," depicts the purpose and meaning of the technique of double-time conditions, which become apparent when the crucial deficiency of the method of regular perturbations is discovered. Since the main topic of this dissertation is precisely the analysis of errors of the average impulse mechanisms, these disorders will be described later in the specific formulas for calculating the change of the clock travel. The intention is to carry out the analysis using the theory of perturbations, and this, inter alia, by the method of double time scale.

First, in this chapter, the essence of the method mentioned will be summarized. Therefore, we will demonstrate an attempt to approximately solve the linear differential equation of the second order with constant coefficients by the method of regular perturbations. After explaining the perturbation technique of double the time, the essence of the Krilov and Bogoljub methods is explained briefly. In this way, control can be made of the results obtained and possibly compare both methods and give a critical overview of the benefits and difficulties of their applications.

Chapter 4, "Oscillator", describes the first of the two most important satellites subassembly. The oscillator can be constructed as a physical pendulum or as a balancing wheel. The physical pendulum represents a body swinging around a point located outside the center of equilibrium, while the balancing wheel is a massive body, a circle around the fixed axis, which passes through its center of mass and performs oscillations under the action of the elastic restitution moment of force. In addition to describing the functionality of these two oscillator performances, the calculation of the circular error by the double-time method is given. A circular error is a change in the pendulum period caused by a change in the amplitude. This chapter also gives an overview of the oscillator's disturbances that occur as a result of external influences, such as temperature, aerostatic thrust, resistance and air density. The influence of temperature is considered to be the most significant, and it manifests itself through the propagation and collecting of the pendulum materials, and this affects the periodic oscillations. The aerostatic thrust, in accordance with the Archimedes Law, reduces the weight of the pendulum for the weight of the pendulous air. The physical pendulum of the timer, with the exception of the restitution gravitational force, acts also with the force of the air resistance, due to which the pendulum loses energy. The change in air density caused by a change in pressure, humidity, and / or a change in air temperature has a direct impact on the overall energy of the pendulum that oscillates, the other energy parameters, and the timing of the timer.It is, in essence, caused by a change in the dynamic resistance acting on the pendulum. These changes can be classified as the effects of the environment in which the pendulum moves and are often considered to be of lowerer influences than the temperature. This chapter presents their mathematical model of the impact of aerostatic thrust, as well as the mathematical model of resistance and density of air. With the development of mechanical timers, solutions for compensating oscillator errors were developed as well. Most attention is devoted to temperature compensation and given the calculation and example of the pendulum, which is temperature compensated. The impact of air (resistance, density and aerostatics) is negligible, although with precision clocks (astronomical clocks, chronometers, high-quality public and tower timers), this error is noticeable and can become impermissibly large,in the case of long periods of extremely high or low atmospheric pressure. Therefore, the basic budget of this error is given and its order of magnitude is shown.

Chapter 5, "Spit-impulse mechanisms", is a key sub-assembly of every mechanical clock, because it maintains and counts the oscillator oscillations and thus measures the flow of time. With its functions this mechanism introduces disruptions into the oscillatory process so oscillations are no longer their own, but are forced with a frequency that is susceptible to change. Therefore, the process of measuring time itself distorts the accuracy of this measurement. The occurrence of an average impulse mechanism changes the oscillation oscillator oscillation time, and thus the timing of the timer, is called a fault of the average impulse mechanism or a short error of the breaker. Within the classification, three types of a mean-impulse mechanism are shown: a boiler-backed, impulse, pulse mechanism, a calm, pulse-free mechanism and a free-flow-impulse mechanism. Using the appropriate momentum interaction diagrams,the constructive and dynamic characteristics of the obstacles are shown qualitatively, with particular reference to the errors of the oscillation period they generate. After classifying the impulse-based mechanisms, a general formula for the error of the average-impulse mechanism was derived using the double-time scale (scale) of the perturbation method. A general formula for the error of the average-impulse mechanism was also developed, using the technique of averaging by the Krylov and Bogoliubov methods. In both cases, only those clock mechanisms that incorporate spiral springs with the balance point as an oscillator were considered, but it should be emphasized that the results of these analyzes are universally applicable to all other types of impulse mechanisms, including those that are installed in stationary clamps with pendulum .It starts from the fact that the balancing wheel of the clock mechanisms performs compulsory muffled oscillations, and it is assumed that the attenuation is due to the viscous moment of force proportional to the angular oscillation velocity. The identity of all approximate solutions and full compliance with the estimation of the order of the size of the approximation error and the order of the size of the time interval are shown, on which these approximations apply to both methods.

Chapter 6, "Other parts of the clock", completes the whole story related to sub-clocks of the clock. The chapter provides descriptions of the three remaining parts of the watch: remontoire, transmission group and winding mechanism. Remontoire is the mechanism most commonly seen with towers in towers. The most important purpose of this mechanism is to provide a secondary, uniform and constant winding source for the pulse mechanism, thus ensuring the accuracy of the clock.The principle of operation of the remontoire as well as its basic parts is shown. The parameters of the remontoire are given, which will be used in Chapter 7, "Model of the whole hour". The transmission group represents a group of gears that are paired to transfer the drive in one direction, from this loop to the drill to the average impulse mechanism, and in the second direction the uniform intervals of the impulse mechanism are converted into seconds, minutes and hours. The winding mechanism is shown as a separate sub-assembly interlaced with a transmission group. By showing its components, as well as the principle of winding and maintaining the moment of the clock, a story about all sub-assemblies of the clock will be made, which will be made as a 3D model, and on which mathematical models are tested in the previous chapters.The parameters of the remontoire are given, which will be used in Chapter 7, "Model of the whole hour". The transmission group represents a group of gears that are paired to transfer the drive in one direction, from this loop to the drill to the average impulse mechanism, and in the second direction the uniform intervals of the impulse mechanism are converted into seconds, minutes and hours. The winding mechanism is shown as a separate sub-assembly interlaced with a transmission group. By showing its components, as well as the principle of winding and maintaining the moment of the clock, a story about all sub-assemblies of the clock will be made, which will be made as a 3D model, and on which mathematical models are tested in the previous chapters.The parameters of the remontoire are given, which will be used in Chapter 7, "Model of the whole hour". The transmission group represents a group of gears that are paired to transfer the drive in one direction, from this loop to the drill to the average impulse mechanism, and in the second direction the uniform intervals of the impulse mechanism are converted into seconds, minutes and hours. The winding mechanism is shown as a separate sub-assembly interlaced with a transmission group. By showing its components, as well as the principle of winding and maintaining the moment of the clock, a story about all sub-assemblies of the clock will be made, which will be made as a 3D model, and on which mathematical models are tested in the previous chapters.and in the second direction, the uniform intervals of the mean-impulse mechanism turn into seconds, minutes and hours. The winding mechanism is shown as a separate sub-assembly interlaced with a transmission group. By showing its components, as well as the principle of winding and maintaining the moment of the clock, a story about all sub-assemblies of the clock will be made, which will be made as a 3D model, and on which mathematical models are tested in the previous chapters.and in the second direction, the uniform intervals of the mean-impulse mechanism turn into seconds, minutes and hours. The winding mechanism is shown as a separate sub-assembly interlaced with a transmission group. By showing its components, as well as the principle of winding and maintaining the moment of the clock, a story about all sub-assemblies of the clock will be made, which will be made as a 3D model, and on which mathematical models are tested in the previous chapters.as well as the principle of winding and maintaining the moment of the clock, the story about all sub-assemblies of the clock that will be made as a 3D model and on which the mathematical models are tested in the previous chapters are rounded up.as well as the principle of winding and maintaining the moment of the clock, the story about all sub-assemblies of the clock that will be made as a 3D model and on which the mathematical models are tested in the previous chapters are rounded up.

Chapter 7, "3D model of the clock mechanism and simulation of work", gives an overview of the results that are checking the accuracy of the formula for faults of the impulse mechanisms in the quasi-oscillation mode of oscillation of the balance point, carried out using the theory of the perturbation account. At the beginning, a 3D model of the whole clock was created in the SolidWorks application and the execution process was simulated. The watchmaker clock was made as a watch with a pendulum. In addition to the simulation of his work, a simulation was performed with a watchmaker, which uses a balanced spring instead of the pendulum. On this type of timer, at the very beginning of the simulation process, the oscillation period, or the frequency of the free-damped oscillations of the balance point, which is built into both oscillator assemblies and wires (balancing point and free overvoltage circuit and balancing point and reverse rotation), were measured.All results are tabulated. If only the dynamic characteristics are taken into account, all the impulse mechanisms can be divided into three large groups: bradycrons, tachycrons and isohrons. A detailed analysis of the oscillator oscillation oscillator oscillator also shows the physical cause - the errors of the mean-impulse mechanisms are not the result of a linear theory of oscillation, but precisely the nonlinear dynamics of the clock mechanism, which in this dissertation was mathematically treated by the methods of the perturbation account.A detailed analysis of the oscillator oscillation oscillator oscillator oscillator also shows the physical cause - the errors of the mean-impulse mechanisms are not the result of the linear oscillation theory, but precisely the nonlinear dynamics of the clock mechanisms, which is mathematically processed by the methods of the perturbation account in this dissertation.A detailed analysis of the oscillator oscillation oscillator oscillator oscillator also shows the physical cause - the errors of the mean-impulse mechanisms are not the result of the linear oscillation theory, but precisely the nonlinear dynamics of the clock mechanisms, which is mathematically processed by the methods of the perturbation account in this dissertation.

2. Theory of time measurement

2.1 The history of time measurement

It can not be established reliably when awareness of the flow of time occurs, or with certainty who can determine when and when it began to measure and record time intervals. It is assumed that the megalithic civilizations of the prehistoric age used simple calendars based on the apparent movement of the Sun and the Moon, that is, the spring equinox and moonlight [21] and [22]. It is certain that during the Neolithic and Bronze Age stone objects and sculptures of a circular shape were built (Stonehenge [23]) and presumed to be used as calendars for primitive measurements of longer time intervals and prediction of emerging seasonal events - equinox and solstice. Awareness of time, once awakened, has always been based on a strong intuition of the equilibrium of the time flow. On this intuitive performance, all measurements of time, from the prehistoric age,to this day.

Written history [24], [25], proves that ancient civilizations performed caring and extensive observations and recordings of cyclical movements of celestial bodies and thus created rather precise calendars. These calendars were used to predict the date of seasonal astronomical events significant for the planning of agricultural works, war hikes, construction projects and other activities essential for the successful organization of the state and society. Except for calendars, which were measured by long, secular, time intervals, Ancient Egypt used sunny timepieces for measuring shorter, daily intervals of time. To measure time during the night, special devices were used to observe the apparent movement of stars or the transition of a series of stars through a meridian site. Apart from the above mentioned devices, the ancient Egyptians also used water clocks [26],by which the flow of time was measured by approximately uniform flow of water. The recording of time intervals in a sixty-sized number system is exactly the maturity of ancient Egypt and Mesopotamia.

Ancient Greece and Rome (300 BC - 500 AD) promote the achievements of the ancient Egyptians. At that time, mathematically precisely constructed solar clocks were used [27], [28]. The Roman architect, Marko Vitruvie Polio, in the section "On Architecture" [29], analyzes in detail the movement of the shadow of the gnomon and describes the variation of the methods and methods of constructing the solar clock. Water climes (klepsiders) become a complex hydro-mechanical device with different methods of improving the accuracy of time interval measurements. In 50 BC, astronomer Andronikos of Cyrus (Andronicus of Cyrrhus) builds in Athens the Wind Tower and supplies it with a sunny clock, a klepsidor, and a windshield [30]. The klepsidra is known (Figure 1), which is 3 years p.n.e. constructed an inventor, mathematician and father of pneumatics, Ctesibius of Alexandria (Ctesibius of Alexandria).


Figure 1 Klepsidra Ktesibi of Alexandria [31]

For the recording of secular time intervals, Stara Greece uses solar and lunisolar calendars, while the old Rome is solely solar [28]. When it comes to timing instruments, Stara Persia will remain remembered for high precision clups, which can be compared with the accuracy of modern mechanical timers. In addition to water clocks, weather in ancient Persia was also measured by astrolabs (Figure 2) - instruments for determining the positions of stars of the Sun on the sky, or alternatively, the geographic length of the city and navigation [32].


Figure 2 Astrolab[33]

Similar to other ancient civilizations, and in ancient China, the flow of time was measured by solar clocks and climes of various constructions, complexity and level of accuracy [34]. The traditional lunar calendar, which is still used today in China, is an ancient Chinese civilization.

Civilizations of the Middle Ages inherit, use and perfect antique achievements and methods of measuring time. Sunglasses and clippers are still widely used, and with them ever more frequent use are timepieces - candles (clock candles), clocks - lamps (flame watches) and sand clocks. The idea is everywhere the same: roughly evenly combustion of wax and oil, that is, the emptying of sand from the glass container is read out on suitably constructed rocks, thus recording the flow of time. Clock candles are mentioned for the first time in China, around 520, for the measurement of time during the night [35]. In Europe, during the era of Anglo-Saxon King Alfred the Great (849-899), we use satin candles, carefully weighed masses and diameters. The most famous Muslim mechanic,Budiuzaman Al-Jazari (1136-1206) constructed sophisticated mechanical timepieces with dials and poles whose work was based on measuring the mass of the burning candle [36]. The skill of building sunny watchmakers, inherited from the ancient times, is especially perfected by Muslim inventors, mathematicians and astronomers in the Middle Ages. Thus, Arab astronomer Ibn Al Satyr (Ibn Al-Shatir, 1304-1375), the first explains the characteristics of the equatorial sundial and construct, in gnomonic projection, the famous horizontal sundial (replica in figure 3), in the northern minaret of the Umayyad Mosque [37].the first explains the characteristics of the equatorial solar clock and constructs, in the gnomonic projection, the famous horizontal sunny clock (replica in Fig. 3), on the northern minaret of the large mosque in Damascus [37].the first explains the characteristics of the equatorial solar clock and constructs, in the gnomonic projection, the famous horizontal sunny clock (replica in Fig. 3), on the northern minaret of the large mosque in Damascus [37].


Figure 3 Replica of Al-Shatira's sunny clock in Damascus [37]

From the mid-15th century, the concept of equatorial sunshine begins to apply in Europe. Italian astronomer Giovani Padovani (Giovanni Padovani, born 1512) publishes a 1570s discussion of sunny clocks in which he gives instructions for their construction on horizontal and vertical levels. Similar to this work, Italian astronomer and mathematician Giuseppe Biancani (Giuseppe Biancani, 1565-1624) published the year 1620 a book on the construction of various types of sunshine timers. Sandy clocks begin to be used in the 11th century, first of all for measuring time and navigation on ships, then in everyday life, cooking, in churches, monasteries, manufaktures, etc. They are the first instruments for reliable and precise measurement of short time intervals , simple design and easy maintenance.It is also noted that the Portuguese sailor Ferdinand Magelan (Ferdinand Magellan, 1480-1521) used 18 sands of clocks (Figure 4) on each ship during the famous maritime expeditions [38].


Figure 4 Sand clock

The middle ages also show the appearance of the first mechanical watch with gears and primitive speed regulators. In constructing such timers, Chinese engineers - early medieval constructors have been particularly emphasized as described in papers [39] and [40]. Ji Xing (683-727), a Chinese engineer, astronomer and mathematician, is building an astronomical clock with a primitive water-powered mechanism. In 976, the astronomer and military engineer Zang Siksung (X century) constructed a watch with a living, which activated the bell in the clock tower every 15 minutes. Su Song (1020-1101), a mathematician, astronomer, cartographer and horologist, builds an astronomical watch with a breakthrough, a reinforcing sphere and a mechanism for outbursts, and sound advertising of the past hours. Izvan Kine, the construction of complex mechanical timers with speed regulators,bells and outbursts emerged during the 11th and 12th centuries in Damascus and Baghdad. The first clock with an epicicular planetary transmission mechanism, whose complexity was surpassed only in the 14th century, was built by the Andalusian mathematician and astronomer Al Muradi in the 11th century [41].

In medieval Europe, the first watchmakers were monks in order to more effectively organize life and work within the monastery, by accurately measuring the time, as evidenced by 11th-century notes [42]. Giovanni de Dondi, 1318-1899, Italian physicist, engineer and professor of astronomy in Padua, first publishes a detailed description of the mechanical clock in the Il Tractus Astarii in 1364 [43]. Except for Padua, significant examples of medieval mechanical watchmakers were built in Milan (1335), Straussburg (1354), Lund (1380), Ruane (1389), Moscow (1402), Prague (1462) and Venice (1499), Figure 5.


Figure 5 The clock in Venice, 1499.

The rest is recorded in the second volume of the Russian illustrated ten-volume yearly (Lys's Letopisnyj vvod) from the second half of the 16th century that the Serbian monk Lazar Hilandarac (Lazar Crnorizac) constructed the first mechanical public watchmaker in Russia in 1404 (Figure 6) [44] [45]. For the history of Serbian time measurement, it is important to note that the oldest preserved Serbian watch is located in the Studenica Monastery, which is carved along the southern portal of the Church of the Holy Virgin.


Figure 6 Serbian monk Lazar shows the Great Prince his watch [45]

The key feature of the mechanisms of all these and other medieval timers is the presence of the primitive controller of the "verge & foliot" (Figure 7) which is supplied with a crown point (pos. 5) with teeth (item 3) and a spindle (item 6) with pallets (item 4), regulates the travel of the clock mechanism by periodically changing the direction of rotation of the balance lever. On the spindle there is a lever (item 1) with two of them (item 2).


Figure 7 Crown wheel, spindle and balancer [46]

The balance lever is not an oscillator and does not have a fixed oscillation period, but regulates the travel of the timer mechanism solely by its own inertia. This invention relates to the year 1273 and attributes it to the French constructor Vilars Dehonekort (Villard de Honnecourt, XIII century) [47]. Most medieval timepieces do not have minute handles, but astronomical watches show the geocentric daily and annual sunsets in the orthographic or stereographic projection of the heavenly arch. The first mention of a minute point was recorded in one manuscript from 1475, and the second hand appeared for the first time in Germany, during the 15th century [47]. Timepieces with weights, outbursts and walkers of the type "verge & foliot" were also known in the Ottoman Empire. One such clock mechanism is described by engineer Taki Al Din (Taqi ad-Din Muhammad ibn Ma'ruf,1526-1585) in the technical tract on mechanical timers from 1556.

The turning point in the development and improvement of time measurement took place in 1656, when Dutch scientist Christiaan Huygens (Christiaan Huygens, 1629-1695) constructed the first watch with a pendulum and a spiral spring watch.


Figure 8 Christian Heagens (1629-1695) [48]
In 1673, Huygens published a scientific study entitled "Horologium Oscillatorium: a gray motto pendulorum ad horologia aptato demonstrationes geometricae" [49], his life-work, which counts in three of the most important scientific studies in theoretical mechanics of the seventeenth century. In this book, Huygens analyzes the mechanical oscillations, the derivative of the mathematical and physical pendulum period, and examines other numerous problems of theoretical mechanics and horology. With this part, as well as the clock mechanisms he constructed, Christiaan Huygens established a new method of time measurement based on oscillatory processes. Namely, as mechanical oscillations are characterized by sufficiently stable own frequency, that is, by a stable oscillation period, counting of these oscillations can accurately measure the duration of the time intervals. From Huygens' time, to this day,this method has remained in force and is an essential principle for the functioning of all timers, including electronic - quartz and atomic.

During the entire Middle Ages, watchmakers were built mainly as public, tower and were supplied with massive mechanisms of great dimensions. However, the late Middle Ages also recorded the appearance of hand and pocket watchmakers. The first portable timer, the so-called. The Nuremberg egg (fig. 9), which could be worn in a pocket or purse (taschenuhr), was constructed in Nuremberg by watchmaker Peter Hennein (Peter Henlein, 1485-1542) [50].


Figure 9 Nirnbeck egg, around 1550s

This one and timekeepers similar to him from the same period (mid 16th century) had spring propulsion and were not supplied with an oscillator, but rather by a walker of the type "verge & foliot". Due to the extremely small accuracy (the walk was a few hours a day), they were used more as fashion details and status symbols, and less as instruments for measuring time. Only after Hajgens's invention of the balancing point with spiral spring 1656-1657. Pocket and manual clocks become reliable precision timers, and in the following centuries, they are more perfect, more popular and more important in everyday life.

Since the 17th century, the history of time measuring instruments has been the most important part of the history of the development of the average - impulse mechanisms. The "verge & foliot" speed controller conditions huge pendulum oscillation amplitudes (even over ± 50 °), which significantly increases the impact of a circular error on the total drop of isohronism [46]. It was precisely the need to reduce the amplitude of the pendulum vibrations that was the main reason for the introduction of a new type of regulator in the construction of the timer. It is a reciprocating wheel or anchor controller, whose design was explained by English watchmaker William Clement (1633-1704) and British scientist Robert Hook (1635-1703), in 1670. That same year, the watchman Joseph Knib (Joseph Knibb, 1640-1711) built the first watch with the Clement-Huke boiler in Oxford.The main characteristic of the reverse twist is the absence of a pulse separation from the average function. Both are realized on the same impulse-average surfaces of the anchor palette, only at different stages of the oscillation period of the pendulum. Further improvement of the wheel regulators, perhaps most important in the entire history of science and the skill of building timers, was accomplished by Tomas Tompion (Thomas Tompion, 1639-1713), Fig. 10, the father of British horology, according to the idea of ​​mathematicians and astronomers Richard Towneley, 1629-1707, in 1675.perhaps the most significant in the history of science and the skill of clock construction, was accomplished by Tomas Tompion (Thomas Tompion, 1639-1713), Fig. 10, the father of British horology, according to the idea of ​​mathematicians and astronomers Richard Towneley, 1629-1707, in 1675.perhaps the most significant in the history of science and the skill of clock construction, was accomplished by Tomas Tompion (Thomas Tompion, 1639-1713), Fig. 10, the father of British horology, according to the idea of ​​mathematicians and astronomers Richard Towneley, 1629-1707, in 1675.


Figure 10 Tomas Tompion (Thomas Tompion, 1639.-1713.) [51]

This is the so-called invention. peaceful, impulsive mechanisms, which constructively and functionally separate the impulse from the average function. George Gray (Honorable George Graham, 1673-1751), in Figure 11, Tompion's pupil and the once-great Great Master of the Honored Timbers of London, perfected the invention in 1715 and enabled his massive application.


Figure 11 George Graham (George Graham, 1673.-1751.) [48]

In addition to the Graham's quiet steering wheel regulator, the same class includes many other impulse mechanisms. Let us mention the names of some who are built into stationary (tower and wall) timepieces: Amman-Lepo's (Amant-Lepaute 1741, 1750), BrokΓ³ (Achille Brocot 1849), a needle-pallet mechanism; as well as the names of still regulator for mobile (hand-held and pocket-) clocks: Tompionov cylinder (Tompion 1695) shown in Figure 12, "duplex" (Pierre Le Roy, 1748) and "virgule" (Antoine LΓ©pine Jean 1780.).


Figure 12 Tompion's cylinder barrier

Further development of the walk regulator was achieved by designing the so-called. free, average-impulse mechanisms. The present invention proceeds precisely from the idea that the impulse and the average function are completely released from the direct impact of the drive, or that the oscillator itself be as free as possible from any influence of the regulator. The realization of the first principle led to the construction of the so-called. gravity-based pulse mechanisms, and from the other, the technical solutions of chronometric regulators and the so-called. English and Swiss free ancestors with an anchor. The first gravity walker was constructed by English watchmakers Tomas Madge (Thomas Mudge, 1715 - 1794) and Alexander Kaming (Alexander Cumming 1732 - 1814) in 1766 [46]. The invention is perfected by Henry Kather (Henry Kather, 1777-1835) around 1830, and DΕΎ. M.Bloxam (James Mackenzie Bloxam) around 1850. However, the realization of these conceptual solutions was hampered by the unstable behavior of their average function, known as "roughening" or "bouncing" (approximate tripping, nem galoppieren). This significant problem was finally solved by the great British horologist and lawyer Edmund Beckett Denison, 1st Baron Grimthorpe, QC, 1816-1905, (Figure 13), the invention of the famous "double three-stroke gravity prevention", (Fig. 14), which was incorporated into the mechanism of the clock "Big Ben" in 1856. It still regulates the journey of the Great Westminster Clock with exceptional accuracy and reliability [52].


Figure 13 Edmund Beckett Denison (Edmund Beckett Denison, 1816.-1905.) [52]

Figure 14 Double triangle gravitational barrier [52]

An English free ancestor with an anchor, characteristic of pointed points at the center point, was constructed by Englez Tomas Madge in 1757, by French watchmakers Abraham BrΓ©guet (Abraham-Louis BrΓ©guet, 1747-1823, Figure 15) and Robin (Robert Robin, 1742-1999) [53].


Figure 15 Abraham BrΓ©guet (Abraham-Louis BrΓ©guet, 1747-1823)

Swiss freeway regulator with anchor, which differs from the English variant only in the shape of a tooth of the average point, was created around 1910, and because of its simplicity, today it has the widest use in the mechanisms of hand and pocket watches. The first naval chronometer, Fig. 16, was constructed in 1730 by John Harrison (John Harrison 1693-1776), in which he incorporated one version of a counter-rotational impulse mechanism - the so-called. "Grasshopper" and solved the famous problem of determining latitude at sea [20].


Figure 16 The first naval chronometer by John Harrison in 1730. [20]

The first freewheel chronometer was made by the French watchmaker Pierre Leo (Pierre Le Roy 1717-1855) in 1748. The invention was enhanced by the English watchmakers John Arnold (1736-1999, Fig. 17) in 1779, and Thomas Earnshaw (1749-1829, Fig. 18) in 1783, enabling the mass production of naval chronometers [48].


Figure 17 John Arnold (John Arnold 1736-1999)

Figure 18 Tomas Ernso (Thomas Earnshaw 1749.-1829.) [48]

Besides distinguishing all the features of free-impulse-free mechanisms, chronometric walk regulators have another, valuable property: the skillful design solution eliminates the need for lubrication! If not, the stability of the chronometer's course would be partly endangered by changes in the characteristics of the oil that changes its viscosity over time due to the oxidation and accumulation of impurities. For their choral discoveries, John Arnold and Tomas Ernso received great and well-deserved state awards, as it turned out that the technical solutions that were just embedded in chronometric, impulse-based mechanisms literally saved tens of thousands of seafarers 'and seafarers' lives!

At the end of this historical overview of the development of mechanical timers over centuries, it is necessary to point out two more mechanisms, from the class of free travel regulators. The first is Rifler's pulse mechanism Zigmund Rifler (Sigmund Riefler, 1847-1912, Figure 19, Deutsches Reichs Patent 1889), which was installed in astronomical watches of the highest accuracy between 1890 and 1965. The error of these piano timepieces was less than 10 milliseconds a day.


Figure 19 Zigmund Rifler (Sigmund Riefler 1847-1912) and his astronomical watch

The second free travel regulator is contemporary, patented in 2000 by Beat Haldimann (Beat Haldimann, 1964.- , Figure 20), one of the 20 most important horologists and watchmakers of today [54]. Haldimann's work and discoveries are the best proof that "the art, science and skill" of building mechanical watchmakers is not only alive,but to go through a new Renaissance [48].


Figure 20 Beat Haldimann (Beat Haldimann, 1964.-)

In the period from the 17th to the 19th centuries, other improvements were made to the clock mechanisms. Evard Berlow (Edward Barlow, 1639-1719), an English priest and mechanic, improves the existing version of the sound-tagging mechanism of the past hours (the so-called Outburst Mechanisms), and standardizes the modes of advertising for the past quarter-and-a-half hours (Westminster's grande sonnerie, German and Roman emergencies, passing strikes, etc.). From the time of the great watchmakers Tomas Tompson and George Gray, when made individually and by order, pocket watchmakers are becoming more perfect and accurate, so that from the middle of the 19th century they would move into mass and high standardized production in the famous Swiss manufactories and factories of precision mechanics. It is believed that the first wristwatch was made by Abraham-Louis Brega (Abraham-Louis Breguet,1747-1823) for Carolina Bonaparte, 1810. However, the popularity of watchmakers and their mass production began only after the First World War, during which they became standard equipment of officers and pilots.

During the 17th to 20th century, numerous achievements were made in terms of perfecting clock mechanisms oscillators. The most important innovation was certainly the compensation of the thermal dilatations of the pendulum and the system of the balance wheel - the spiral spring, the most damaging effect on the accuracy of the clock work. The first successful temperature compensation of the pendulum was accomplished by John Harrison around 1720, his invention of the so-called. lattice pendulum [17]. This compensation was realized by a series of rods - carriers of this pendant made of two different metals (for example, steel and brass) that suffer from thermal dilatations in opposite directions.The calculation of this compensation is done so that the resulting dilation of the last carrier is equal to zero. A similar solution Harrison built into the first naval chronometer, which he built in 1730. The bimetallic compensation of the thermal dilatations of the balancing point and the spiral springs was accomplished by the French watchmaker Pierre Le Roy (1717-1785) in 1765. Enriched by English watchmaker Tomas Ernsoa, it was used until the beginning of the 20th century.It was used until the beginning of the 20th century.It was used until the beginning of the 20th century.

In 1896, French - Swiss physicist Charles Edouard Guillaume, 1861-1938, discovered nickel and iron alloys - invar, anibal and elinvar, thereby eliminating the need for existing bimetallic compensation [55]. Namely, both the invar and the anibal have a slight thermal expansion, they are suitable for making the balance point, and the elinvar for making spiral springs because it suffers only a slight change in elasticity with temperature change. In 1933, engineer Dr. Reinhardt STRAUMAN (Reinhard Straumann, 1892-1967) creates an alloy of nickel, chromium, manganese, titanium, beryllium and iron - nivaroks (Nivarox) which by their qualities outweighed elinvar, and therefore from the middle of the 20th century, just one is used exclusively for the production of coil springs [56].

Since 2007, watch balances are predominantly made of glucidur (Glucydur), beryllium alloys, copper and iron having a slight thermal expansion, is non-magnetic and very hard. A widespread belief is that the future development of the watch industry will be supported in innovative solutions in the field of metallurgy and new materials. [57].


2.2 Time measurement units

Measurement of time flow, as well as the measurement of all other physical quantities, is based on defining, adopting and practical realization of certain units of measure. In this chapter, the history of units of time measurement, from ancient, ancient civilizations to the modern age, will be briefly exposed and discussed.

Historical sources testify that anti-peoples used the day as the natural and basic unit of time-consuming measures. In ancient Egypt, from 2000 BC, the day and night periods of the day were shared at 12 o'clock each, from where the first definition of the measure is likely to come as 1/24 of the day [35]. It differs from the contemporary because the duration of the ancient Egyptian clock was different for the day and night periods of the day and changed every day of the year [24]. The described way of daylight and daylight was kept in Europe until the late Middle Ages, during which the measurement of time in the sunshine was gradually replaced by mechanical. In the Old Babylon, from 300 BC, the day was divided into shorter time intervals, in accordance with the adopted sixty-six number system, to 60 parts, each of which was then re-divided into 60 parts, etc.It was also used to divide the day into 12 equal parts, which corresponds to the contemporary time interval of 2 hours (120 minutes) [25]. For astronomical observations, in the Old Babylon, a special unit was defined - the so-called. one time span that lasts 4 modern minutes, as well as a measure of 4/3 of a second, identical to Hebrew helek. However, no sixty division of the day was not used in Old Babylon as an independent unit of time. Nevertheless, the undeniable fact is that the modern standard division of hours in minutes and seconds is a direct consequence of the sixty-sized system defined in the civilization of Old Babylon. The peoples of Helen's civilization used the division of the day into six parts and represent the already mentioned heritage of Old Babylon. Astronomers Hipparchus (Hipparchus of Nicaea, 190-120 BC) and Ptolemy (Claudius Ptolemy, 100-170 n.e.) apart from the mentioned division, define and use the middle clock as the 24th part of the mean solar (sun) day and the integer quarter of the quarter and a third of the mean hour [58]. The middle day and the middle class did not endure seasonal changes, but as constants, they represented the right standards of time measurement as the Old Babylonian and Hellenic civilizations did. These civilizations use an astronomical unit for a unit of one degree as 1/360 part of the mean solar day, or 4 minutes. (for 4 minutes, viewed from Earth, the Sun moves on the ecclemy of the heavenly arch for exactly 1 arc). All three mentioned civilizations used solar, lunar, and lunisolar calendars to measure and record longer time intervals.part of the mean solar (sun) day and the integer quarter of the quarter and a third of the mean hour [58]. The middle day and the middle class did not endure seasonal changes, but as constants, they represented the right standards of time measurement as the Old Babylonian and Hellenic civilizations did. These civilizations use an astronomical unit for a unit of one degree as 1/360 part of the mean solar day, or 4 minutes. (for 4 minutes, viewed from Earth, the Sun moves on the ecclemy of the heavenly arch for exactly 1 arc). All three mentioned civilizations used solar, lunar, and lunisolar calendars to measure and record longer time intervals.part of the mean solar (sun) day and the integer quarter of the quarter and a third of the mean hour [58]. The middle day and the middle class did not endure seasonal changes, but as constants, they represented the right standards of time measurement as the Old Babylonian and Hellenic civilizations did. These civilizations use an astronomical unit for a unit of one degree as 1/360 part of the mean solar day, or 4 minutes. (for 4 minutes, viewed from Earth, the Sun moves on the ecclemy of the heavenly arch for exactly 1 arc). All three mentioned civilizations used solar, lunar, and lunisolar calendars to measure and record longer time intervals.represented the right standards of time measurement as the Old Babylonian and Hellenistic civilizations did. These civilizations use an astronomical unit for a unit of one degree as 1/360 part of the mean solar day, or 4 minutes. (for 4 minutes, viewed from Earth, the Sun moves on the ecclemy of the heavenly arch for exactly 1 arc). All three mentioned civilizations used solar, lunar, and lunisolar calendars to measure and record longer time intervals.represented the right standards of time measurement as the Old Babylonian and Hellenistic civilizations did. These civilizations use an astronomical unit for a unit of one degree as 1/360 part of the mean solar day, or 4 minutes. (for 4 minutes, viewed from Earth, the Sun moves on the ecclemy of the heavenly arch for exactly 1 arc). All three mentioned civilizations used solar, lunar, and lunisolar calendars to measure and record longer time intervals.as well as lunisolar calendars for measuring and recording longer time intervals.as well as lunisolar calendars for measuring and recording longer time intervals.

Second, as a measure of time, is mentioned for the first time in Persia, approximately 1000 years of our era [32]. Their astronomers share a time period between two young months - for days, hours, minutes, seconds, thirds and quarters of seconds. In Central Europe, a similar division is also used by Roger Bacon (Rogerius Beconus, 1219-1292), an English philosopher and scientist [59]. In accordance with these historical facts, it can be concluded that the second was derived from lunisolar cycles, by trying to accurately measure the lunar and defining solar measures of time. When it comes to measuring and recording the duration of lunatics, it is necessary to briefly mention a week as a unit of time. Undoubtedly, this time interval has entered the European civilization through the Hebrew and Judaic traditions, and they again lead from the Old Babylonian lunisolar calendar which,using the intercalation day, synchronized the last day of the last week of the month with the appearance of the young month. The Hebrew nation began to use it for a week in the time of Israelite, in the 9th century BC. as a time interval independent of the cycle of moonlight. The Old Babylonian era was accepted by the Old Greeks in the 4th century BC, and the Roman Empire from the 1st to the 4th century BC. Through the process of Christianization, during the early Middle Ages, the week was also accepted by the European peoples as part of the Judeo-Christian tradition. In the next two thousand years, it became the unchanged standard time interval in most of the civilized world.as a time interval independent of the cycle of moonlight. The Old Babylonian era was accepted by the Old Greeks in the 4th century BC, and the Roman Empire from the 1st to the 4th century BC. Through the process of Christianization, during the early Middle Ages, the week was also accepted by the European peoples as part of the Judeo-Christian tradition. In the next two thousand years, it became the unchanged standard time interval in most of the civilized world.as a time interval independent of the cycle of moonlight. The Old Babylonian era was accepted by the Old Greeks in the 4th century BC, and the Roman Empire from the 1st to the 4th century BC. Through the process of Christianization, during the early Middle Ages, the week was also accepted by the European peoples as part of the Judeo-Christian tradition. In the next two thousand years, it became the unchanged standard time interval in most of the civilized world.

Second, as a basic measure of time, it was only established with the advancement of mechanical timers, in the second half of the 16th century. Namely, the second that represents the 86400th part of the day has become more precisely measurable only by defining the mean solar time represented by mechanical clocks, but by abandoning the real solar time by sunny clocks. Historical sources claim that the Swiss watchmaker Jost BΓΌrgi (Jost BΓΌrgi, 1552-1632) constructed the first mechanical watchmaker with a secondary one in 1579. In 1581, in his astronomical Observatory Uranienborg, Danish astronomer of Tycho Brahe (Tycho Brahe, 1546-1601) modified the timers to display seconds.

However, the presence of a second hand does not yet mean that the clock accurately measures the second time intervals. Namely, the insufficient technical perfection of the clock built at the end of the 16th century did not allow precise definition and reliable measurement of second intervals. On the timekeepers of that time, the secondary actors had a more decorative role. Only in 1644, French scientist Maran Mersen (1588-1648) calculated by calculating that the mathematical pendulum length of 994 mm, in the field of the earth is more difficult with a standard velocity g = 9,80665 m / s2, oscillates with a period of exactly 2 seconds . This knowledge opened the way for the production of mechanical pendulum timers with a pendulum that will not only be able to show the flow of seconds, but also accurately and reliably measure second time intervals. In 1670, English watchmaker William Clement,1638-1704) perfected the Haggens watch by supplying it to the pendulum with a period of 2 seconds. So, the second became a practical unit for measuring time only when real oscillators began to be built into mechanical circuits, with stable own frequencies of oscillation. In 1832, the German mathematician Gaus (Carl Friedrich Gaus, 1777-1855) first suggested a second as the basic measure of time in his system of measures "millimeter - milligram - second". In 1862, the British Scientific Association BSA formally proposed a CGS system of measures that was gradually replaced by the MKS system over the next 70 years. In both systems the measure of the second is adopted as the basic unit of time. During the 1940s, the ICC was accepted as an international system of measures, in which the second was defined as 1/86400 part of the middle solar day.Second, it became a practical unit for measuring time only when mechanical oscillators began to be installed in real time with stable oscillation frequencies. In 1832, the German mathematician Gaus (Carl Friedrich Gaus, 1777-1855) first suggested a second as the basic measure of time in his system of measures "millimeter - milligram - second". In 1862, the British Scientific Association BSA formally proposed a CGS system of measures that was gradually replaced by the MKS system over the next 70 years. In both systems the measure of the second is adopted as the basic unit of time. During the 1940s, the ICC was accepted as an international system of measures, in which the second was defined as 1/86400 part of the middle solar day.

Second, it became a practical unit for measuring time only when mechanical oscillators began to be installed in real time with stable oscillation frequencies. In 1832, the German mathematician Gaus (Carl Friedrich Gaus, 1777-1855) first suggested a second as the basic measure of time in his system of measures "millimeter - milligram - second". In 1862, the British Scientific Association BSA formally proposed a CGS system of measures that was gradually replaced by the MKS system over the next 70 years. In both systems the measure of the second is adopted as the basic unit of time. During the 1940s, the ICC was accepted as an international system of measures, in which the second was defined as 1/86400 part of the middle solar day.The German mathematician Gaus (Carl Friedrich Gaus, 1777-1855), first proposes a second as the basic measure of time in his system of measures "millimeter - milligram - second". In 1862, the British Scientific Association BSA formally proposed a CGS system of measures that was gradually replaced by the MKS system over the next 70 years. In both systems the measure of the second is adopted as the basic unit of time. During the 1940s, the ICC was accepted as an international system of measures, in which the second was defined as 1/86400 part of the middle solar day.The German mathematician Gaus (Carl Friedrich Gaus, 1777-1855), first proposes a second as the basic measure of time in his system of measures "millimeter - milligram - second". In 1862, the British Scientific Association BSA formally proposed a CGS system of measures that was gradually replaced by the MKS system over the next 70 years. In both systems the measure of the second is adopted as the basic unit of time. During the 1940s, the ICC was accepted as an international system of measures, in which the second was defined as 1/86400 part of the middle solar day.In both systems the measure of the second is adopted as the basic unit of time. During the 1940s, the ICC was accepted as an international system of measures, in which the second was defined as 1/86400 part of the middle solar day.In both systems the measure of the second is adopted as the basic unit of time. During the 1940s, the ICC was accepted as an international system of measures, in which the second was defined as 1/86400 part of the middle solar day. In 1956, the second was redefined as part of a medium solar (synodic or tropical) year for an appropriate epoch because it was noticed that the rotation of the Earth around its own axis was not uniform enough to be used as a standard for defining a unit of time. Since 1960, the duration of a mid-tropical year is no longer obtained from astronomical measurements, but from a budget from special formulas, which terminates an explicit link between the duration of one second and the duration of the day. Namely, the development of science, technology and technology reached such a high level in the mid-20th century, that the establishment of the definition of a unit of time at the speed of the Earth's rotation and revolution was no longer precise enough. The development of atomic timers during the 1950s brought in 1967 to the Thirteenth General Conference on Weights and Measures until the adoption of a new definition of a second. According to this definition,it represents a duration of 9,192,631,770 radiation times that corresponds to a quantum transition between two hyperfine levels of the baseline state of the cesium-133 atom. The definition of "atomic seconds" has established the International Atomic Time (TAI) as a coordinate standard of high precision time obtained by the arithmetic mean of time measures and maintains over 400 atomic clocks that have been installed in more than fifty national laboratories around the world over the past five decades. International Atomic Time is the basis of the Coordinate Universal Time (UTC) which is used to measure the flow of civilian time on Earth. During the seventies of the twentieth century, the relativistic gravitational influence of time dilation with a change in altitude to the flight of atomic timers was measured. In 1980.and the correction of this effect is formally introduced by calculating the time each atomic clock shows, with the corresponding local at zero altitude (universal, mean sea level level). Today, the relative error of measuring the frequencies of individual atomic clocks does not exceed a value of $10^{-15}$, and the national standards agencies maintain a network of atomic timers and synchronize them with an accuracy of $10^{-9}$ per day. Despite this high accuracy, atomic clocks continue to improve, so the latest, the so- optical watches, measures and maintain the operating frequency of coherent radiation in the optical region with a relative error of $10^{-18}$ [60].the relative error of measuring the frequencies of individual atomic timers does not exceed the value of $10^{-15}$, and the national standards agencies maintain a network of atomic timers and synchronize them with an accuracy of $10^{-9}$ per day. Despite this high accuracy, atomic clocks continue to improve, so the latest, the so- optical watches, measures and maintain the operating frequency of coherent radiation in the optical region with a relative error of $10^{-18}$ [60].the relative error of measuring the frequencies of individual atomic timers does not exceed the value of $10^{-15}$, and the national standards agencies maintain a network of atomic timers and synchronize them with an accuracy of $10^{-9}$ per day. Despite this high accuracy, atomic clocks continue to improve, so the latest, the so- optical watches, measures and maintain the operating frequency of coherent radiation in the optical region with a relative error of $10^{-18}$ [60].measures and maintain the operating frequency of coherent radiation in the optical region with a relative error of $10^{-18}$ [60].measures and maintain the operating frequency of coherent radiation in the optical region with a relative error of $10^{-18}$ [60].

3. Theoretical basics of the perturbation account

3.1. The double time method (2T)

One of the important goals of this dissertation is the qualitative and quantitative analysis of the errors of the average impulse mechanisms, that is, the frequency disturbances of the clock oscillator caused by their impulse mechanisms. The key results of such an analysis will be described by the specific formulas for calculating the change in the timing of the timer. How is the intention to carry out the analysis using the theory of perturbation, and this, inter alia, by the method of double-scale (scale) of time, will first in this chapter summarize the essence of the method mentioned above. In the third chapter of this dissertation, after explaining the perturbation technique of the double time of time, the essence of the Krylov and Bogoliubov methods is briefly explained. In this way, control can be made of the obtained results and possibly compare both methods and give a critical overview of the benefits and difficulties of their applications.

The double-time technique belongs to one general method of perturbation known under the names: analysis of multiple proportions or scale variables, multiple expansion or multiple-scale methods. It is used for the analysis of phenomena whose states can be described by generalized coordinates of distinctly different dimensions. Poorly suppressed oscillations (linear or nonlinear, free or forced) represented by differential equation

$$π‘₯̈ + Ο‰^2π‘₯ + Ρ𝑓(π‘₯, π‘₯̇) = 0;\, Ξ΅∈(0,1), Ξ΅≪1,\tag{3.1}$$

a typical example of such phenomena. In equation (3.1), the free oscillations are poorly disturbed (perturbated) by the member $Ρ𝑓(π‘₯, π‘₯̇)$ which, in general, is non-linear. The constant $Ξ΅$ can be chosen in different ways, and in this case, it is convenient that it represents exactly the attenuation factor $ΞΎ$. Namely, in the case of free oscillations with low attenuation, the rate of decrease in the amplitude is significantly lower in relation to the angular oscillation frequency, and in the case of forced oscillations, a very slow change in oscillation phase may occur. The impression is that there are two different scales of time within the oscillatory process. The introduction of multiple proportions of variables into the perturbation account is attributed to mathematician and physicist PoincarΓ©, although he himself claimed that the idea originated from the astronomer Lindstedt. By dealing with the general theory of perturbation, mathematicians Krylov and Bogoliubov, apart from the method of averaging, also developed in detail the technique of double the time.

In order for the double-time process to be perfectly clear, it is necessary first to emphasize the motivation for its application. The purpose and meaning of the double-time technique will become apparent when the crucial deficiency of the method of regular perturbations is discovered. Therefore, an attempt will be made to use the method of regular perturbations to approximately solve the following linear differential equation of the second order with constant coefficients:

$$πœ‘̈ + 2ΞΎΟ‰_0Ο†̇ + Ο‰_0^2Ο† = 0;\,ΞΎ∈(0,1), ΞΎ≪1.\tag{3.2}$$

It describes free oscillations, with its own angular frequency $Ο‰_0$ and small attenuation, if the attenuation factor is $ΞΎ∈(0,1), ΞΎ_1$. The initial conditions are known ($Ο†(0) = Ξ¦_0, Ο†̇ = 0$), but they do not matter for this demonstration. This attempt will not lead to a correct solution. It will be precisely this failure to illustrate the disadvantage of regular perturbations that will justify the reason for the introduction of the double-timing method. It should be noted that in equation (3.2), the term $2ΞΎΟ‰_0Ο†̇ $ represents a small disturbance, i.e, a small perturbation of the free unstressed oscillations described by the equation

$$πœ‘̈ + Ο‰_0^2Ο†̇ = 0;\tag{3.3}$$

because the attenuation factor $ΞΎ$ is a very small positive number. The method of regular perturbations requires an approximate solution of the differential equation (3.2) in the form of a perturbation order

$$Ο†(𝑑) = Ο†_0(𝑑) + ΞΎ^1Ο†_1(𝑑) + ΞΎ^2Ο†_2(𝑑) + ⋯ + ΞΎ^𝑛φ_𝑛(𝑑) + 𝑂(ΞΎ^{𝑛 + 1}),\tag{3.4}$$

which represents the sum of the exact solution $Ο†_0(𝑑)$ of the simplified differential equation (3.3), in which the disorder $2ΞΎΟ‰_0Ο†̇ $ is ignored, and a number of perturbation members. The symbol $𝑂(ΞΎ^{𝑛 + 1})$ represents the order of the size of the residue of the approximation and is $ΞΎ^{𝑛 + 1}$. These members of the higher order remotely (perturbate) idealized solution $Ο†_0(𝑑)$, and thus correct it and approach the desired solution $Ο†(𝑑)$ of the equation (3.2), in which the disorder $2ΞΎΟ‰_0Ο†̇ $ is not neglected. If $ΞΎ∈(0,1)$, the higher order members should decrease successively, which means that the perturbation approximation should of the exact solution (3.4) is an asymptotic functional order. In such a development of an approximate solution to an asymptotic order, each individual function, as a member of the order, grows slower in relation to the previous one at an appropriate time interval. That this does not always have to be and the necessity will just illustrate this example.

The approximation solution of the equation (3.2) is required in the following form of the collection of the initial solution and correction of the first order:

$$Ο†(𝑑) ≈ Ο†_0(𝑑) + ΞΎΟ†_1(𝑑),\tag{3.5}$$

in which all members $ΞΎ^𝑛φ_𝑛(𝑑), 𝑛 > 1$ are ignored. In this case, it is certain that, for the given $ΞΎ$, there is always a finite time interval $𝑑∈[0, 𝑑_𝑀]$, within which the rest of the approximation has an order of magnitude $𝑂(ΞΎ^2)$. The above fact follows directly from the theorem that Murdock (James Murdock) argues in the book "Perturbation - Theory and Methods" [61]. If equation (3.5) to replace the differential equation (3.2) gives the equation:

$$πœ‘̈_0 + 2ΞΎΟ‰_0Ο†̇ _0 + Ο‰_0^2Ο†_0 + ΞΎΟ†̈_1 + 2ΞΎ^2Ο‰_0Ο†̇ _1 + ΞΎΟ‰_0^2 Ο†_1 = 0.\tag{3.6}$$

In equation (3.6), the article $2ΞΎ^2Ο‰_0Ο†̇_1$ is ignored as a small value of higher order. Differential equation (3.6) can be decomposed into the following system of two differential equations:

$$πœ‘̈_0 + Ο‰_0^2Ο†_0 = 0\tag{3.7}$$ $$ΞΎ(πœ‘̈_1 + Ο‰_0^2Ο†_1) = -2ΞΎΟ‰_0Ο†̇ _0.\tag{3.8}$$

The solution of the equation (3.7) describes the free unbroken oscillations and for the initial conditions $Ο†_0(0) = Ξ¦_0, Ο†̇_0 = 0$ reads:

$$Ο†_0(𝑑) = Ξ¦_0 \cos Ο‰_0𝑑.\tag{3.9}$$

If the solution (3.9) is replaced by the equation (3.8), the differential equation is obtained:

$$πœ‘̈_1 + Ο‰_0^2Ο†_1 = 2Ο‰_0^2 Ξ¦_0 \sin Ο‰_0𝑑.\tag{3.10}$$

Equation (3.10) is a non-homogeneous non-homogeneous differential equation of the second order and can be solved by the Lagrange method of variation of the constants. For the initial conditions $Ο†_1(0) = 0, Ο†̇_1 = 0$, the equation solution (3.10) is given by:

$$Ο†_1(𝑑) = Ξ¦_0(\sin Ο‰_0 - Ο‰_0𝑑\cos Ο‰_0𝑑).\tag{3.11}$$

Thus, the approximate solution of the differential equation (3.2) is:

$$πœ‘(𝑑)=𝛷_0\cos πœ”_0𝑑+πœ‰(𝛷_0(\sin πœ”_0𝑑−πœ”_0 𝑑\cos πœ”_0𝑑))+𝑂(πœ‰^2).\tag{3.12}$$

It is immediately noticed that the solution (3.12), as the sum of the expressions (3.9) and (3.11), does not correspond to the solution given by the linear theory of oscillations. It is not correct from the point of view of the perturbation method, as it disrupts the asymptotic approximation to the exact solution, the process on which the theory of perturbation is essentially based. The main cause of this disturbance is the fact that with time $𝑑$, the member $ξ𝑑ω_0Ξ¦_0\cos Ο‰_0𝑑$ grows unlimited and thus loses the character of small corrections of the initial solution $Ο†_0(𝑑)$. Namely, in expression (3.12), for each $𝑑 = 𝑂(1/ΞΎ)$ the second member grows to such an extent that its order of magnitude becomes equal to the order of the size of the first member, due to which the perturbation approximation of the exact solution ceases to have the character of asymptotic development. The expression of the form 𝑑cosΟ‰0𝑑 in the solution (3.12) is called a secular member (secular - from the Latin word saeculum, the one that has a time long, for centuries) and is a formal consequence of the expression:

$$2Ο‰_0^2 Ξ¦_0 \sin Ο‰_0𝑑,\tag{3.13}$$

on the right-hand side of the equation, in the differential equation (3.10). Although there is no active external coercion, the term (3.13) is a fictitious cyclic influence - a coercion, which is described in the resonances with its own oscillations described by the homogeneous part of the differential equation (3.10). Therefore, this term is called a factor of resonant coercion or resonant forcing. And in general, any form of expression $A\cos Ο‰_0𝑑 + 𝐡\sin Ο‰_0𝑑$ in homogeneous differential equation form:

$$πœ‘̈_1 + Ο‰_0^2Ο†_1 = A\cos Ο‰_0𝑑 + 𝐡\sin Ο‰_0𝑑\tag{3.14}$$

represents a factor of resonant coercion and, in its particular solution, causes the appearance of secular members of the form $𝑑\cos Ο‰_0 𝑑$ and $𝑑\sin Ο‰_0𝑑$. The properties of the secular members are examined in detail by Murdock [61] and more precisely explains in what sense their appearance is "harmful". The secularity of such members can be apparent [61], for example in the approximations of periodic functions to infinite degrees. In such a case, secular members may be acceptable if the limited accuracy of an approximate solution is acceptable in a sufficiently short time interval. The same author points out that there are cases where the secular members are inevitable, for example in approximate solutions in the form of asymptotic functional orders, when neither the exact solution is limited, that is, when it also contains secular members [61]. In the case of solving the differential equation (3.2) by the method of regular perturbations, an approximate solution (3.10) containing secular members can be acceptable accuracy, but only in a sufficiently short time interval, which can be estimated by a numerical calculation. In particular, for $𝑑 = 𝑑_𝑆 = 1/(ΞΎΟ‰_0)$ the secular member is equated with the first term, and for $𝑑≥𝑑_𝑆$ the asymptotic development ceases to be valid. Time interval $𝑑∈[0, 𝑑_𝑀]$ In which the approximate solution (3.10) has an acceptable accuracy is usually extremely short $𝑑_𝑀≪𝑑_𝑆$ . As already pointed out, at this time interval, for some particular value of the damping factor $ΞΎ∈(0,1)$, the remainder of the approximation has an order of magnitude $𝑂(ΞΎ^2)$. If the members of the higher order $ΞΎ^𝑛φ_𝑛(𝑑), 𝑛>1$ were used in the perturbation calculation , the order of the size of the residual approximation would decrease $𝑂(ΞΎ^{𝑛+1}), 𝑛>1$, but would always be valid at the same time interval $𝑑∈[0, 𝑑_𝑀]$ on which lower-order approximations were also valid. Mardock [61], points out in the commentary of Theorem 3.2.1. that the time interval of the first-order approximation can be extended to a time interval $𝑑∈ [0, 𝑑_𝑀/ ΞΎ ]$ with increasing the order of the size of the approximation residue with $𝑂(ΞΎ^2)$ to $𝑂(ΞΎ^1)$, provided that the functions $Ο†_0(𝑑)$ and $Ο†_1 (𝑑)$ perturbation approximations do not contain secular members. Thus, in general, the method of regular perturbations will not be suitable for application whenever differential equations contain resonant coercive factors, or whenever the solutions of these differential equations consequently contain secular members. This fact is a key deficiency of the method of regular perturbations and a motive for applying another technique to a perturbation account.

The double time method is one of the alternative techniques that goes beyond the problem of the secular members present in the method of regular perturbations. In addition, the double-time method extends the time interval of approximation validity, and this is the order of the magnitude of the constant $ΞΎ$, which in the case of regular perturbations is generally impossible to achieve. Namely, precisely by the elimination of secular members, the double time method ensures that the remainder of the approximate approximation of the approximate solution $Ο†(𝑑)≈Ο†_0(𝑑)$ has the order of the size $𝑂(ΞΎ)$ at a time interval $𝑑∈[0, 𝑑_𝑀 / ΞΎ]$. This time interval is for the order of magnitude of the damping factor $ΞΎ$ is longer than the time interval $𝑑∈ [0, 𝑑_𝑀 ]$ on which the residue the approximation of the order $𝑛 = 1$, obtained by regular perturbation, has the order of magnitude $𝑂(ΞΎ^2)$. This is a heuristic procedure, the validity of which is proven by post festum. This method will be briefly explained in the example of an approximate solution of the differential equation of free-damped oscillations (3.2). The essence of the dual time scale method is based on replacing independently variable $𝑑$ two variable $𝑑_1$ and $𝑑_2$ :

$$𝑑_1 = 1 ∙ 𝑑; 𝑑_2 = ΞΎ ∙ 𝑑, ΞΎ∈(0,1),\tag{3.15}$$

assuming that they are independent of each other during the performance of the perturbation account. The constant $ΞΎ$ is the attenuation factor. It has already been emphasized that this procedure has a physical meaning, since the rate of falling of the amplitude of the free, poorly suppressed oscillations is considerably lower than the angular frequency of the oscillations. In terms of (3.15), the variable $𝑑_1$ is the flow of "ordinary" time in which harmonic oscillations take place, and the variable $𝑑_2$ represents the "slow" scale of the time during which the dissipation of the oscillator energy takes place and the amplitude of the damped oscillations decreases. The approximate solution $Ο†(𝑑_1 , 𝑑_2 , ΞΎ)$ is sought in the form of the collection of the initial solution $Ο†_0(𝑑_1 , 𝑑_2)$ and the first row correction $ΞΎΟ†_1(𝑑_1 , 𝑑_2)$, as shown by the expression

$$Ο†(𝑑_1 , 𝑑_2 , ΞΎ) ≈ Ο†_0(𝑑_1 , 𝑑_2) + ΞΎΟ†_1(𝑑_1 , 𝑑_2).\tag{3.16}$$

Once again, the most important objective of this method is emphasized, which Murdock in particular emphasizes in [61]. It is a matter of an approximate solution (3.16) in the form of an asymptotic functional order, at some time interval, to be defined. In order to achieve this, it is necessary to ensure that at that time interval the functions of the perturbation order (3.16) are limited, or that they do not contain secular members. The initial conditions $Ο†(0) = Ξ¦_0, Ο†(0) = 0$ are formulated for both functions $Ο†_0(𝑑_1 , 𝑑_2)$ and $Ο†_1(𝑑_1, 𝑑_2)$, expressions

$$Ο†_0(0,0) = Ξ¦_0, Ο†̇ _0(0,0) = 0, Ο†_1(0,0) = 0, Ο†̇_1(0,0) = 0.\tag{3.17}$$

In accordance with the formulas (3.15), the first and the second derivative of the angular coordinate $Ο†$ by time $𝑑$ is given by the following terms, respectively:

$$Ο†̇ = \frac{πœ•Ο†}{πœ•π‘‘_1} \frac{πœ•π‘‘_1}{πœ•π‘‘} + \frac{πœ•Ο†}{πœ•π‘‘_2} \frac{πœ•π‘‘_2}{πœ•π‘‘} = \frac{πœ•Ο†}{πœ•π‘‘_1} + ΞΎ\frac{πœ•Ο†}{πœ•π‘‘_2} ,\tag{3.18}$$ $$πœ‘̈ = \frac{πœ•Ο†̇ }{πœ•π‘‘_1} + ΞΎ\frac{πœ•Ο†̇ }{πœ•π‘‘_2} = \frac{πœ•^2Ο†}{πœ•π‘‘_1^2} + 2ΞΎ\frac{πœ•^2Ο†}{πœ•π‘‘_1πœ•π‘‘_2} + ΞΎ^2\frac{πœ•^2Ο†}{πœ•π‘‘_1^2}≅\frac{πœ•^2Ο†}{πœ•π‘‘_1^2} + 2ΞΎ\frac{πœ•^2Ο†}{πœ•π‘‘_1πœ•π‘‘_2}.\tag{3.19}$$

In the expression (3.19) the term containing $ΞΎ^2$ is neglected as a small value of higher order. Using the expressions (3.16), and by neglecting the members comprising $ΞΎ^2$, the relation (3.18) and (3.19) are, respectively:

$$Ο†̇ = \frac{πœ•Ο†_0}{πœ•π‘‘_1} + ΞΎ \Big(\frac{πœ•Ο†_0}{πœ•π‘‘_2} + \frac{πœ•Ο†_1}{πœ•π‘‘_1}\Big),\tag{3.20}$$ $$πœ‘̈ = \frac{πœ•^2Ο†_0}{πœ•π‘‘_1^2} + 2ΞΎ\frac{πœ•^2Ο†_0}{πœ•π‘‘_1πœ•π‘‘_2} + ΞΎ\frac{πœ•^2Ο†_1}{πœ•π‘‘_1^2}.\tag{3.21}$$

When the expressions (3.16), (3.20) and (3.21) are included in the differential equation (3.2), after ignoring the members containing $ΞΎ^2$, the following differential equation is obtained:

$$\frac{πœ•^2Ο†_0}{πœ•π‘‘_1^2} + Ο‰_0^2Ο†_0 + ΞΎ\Big(\frac{πœ•^2Ο†_1}{πœ•π‘‘_1^2} + Ο‰_0^2Ο†_1 + 2\frac{πœ•^2Ο†_0}{πœ•π‘‘_1πœ•π‘‘_2} + 2Ο‰_0\frac{πœ•Ο†_0}{πœ•π‘‘_1}\Big) = 0.\tag{3.22}$$

Since the attenuation factor $ΞΎ$ is small but different from zero, the left side of the equation (3.22) is equal to zero if the equations are:

$$\frac{πœ•^2Ο†_0}{πœ•π‘‘_1^2} + Ο‰_0^2Ο†_0 = 0; Ο†_0 = Ξ¦_0, \frac{πœ•Ο†_0}{πœ•π‘‘_1} = 0, \,\, \text{for}\,\, 𝑑1 = 𝑑2 = 0\tag{3.23}$$ $$\frac{πœ•^2Ο†_1}{πœ•π‘‘_1^2} + Ο‰_0^2Ο†_1 = -2\frac{πœ•^2Ο†_0}{πœ•π‘‘_1πœ•π‘‘_2}-2Ο‰_0\frac{πœ•Ο†_0}{πœ•π‘‘_1}; Ο†_1 = 0, \frac{πœ•Ο†_1}{πœ•π‘‘_1} = -\frac{πœ•Ο†_0}{πœ•π‘‘_2},\,\, \text{for}\,\, 𝑑1 = 𝑑2 = 0\tag{3.24}$$

simultaneously satisfied. With each of the mentioned equations, specific initial conditions are given, according to their general formulation (3.17), and in accordance with the expressions (3.16) and (3.20).

The system of differential equations (3.23) - (3.24) is solved successively, with the fact that the differential equation (3.23) is only formally partial, and in essence it represents a simple differential equation with constant coefficients with respect to the variable $𝑑_1$. Thus, the equation (3.23) leads to the initial solution $Ο†_0(𝑑_1, 𝑑_2)$, which is corrected by the correction of the first order $ΞΎΟ†_1(𝑑_1, 𝑑_2)$. In this corrective term, the function $Ο†_1(𝑑_1, 𝑑_2)$ represents the solution of the equation (3.24), which depends on the previously obtained function $Ο†_0(𝑑_1, 𝑑_2)$. One equation solution (3.23) is given by the expression:

$$Ο†_0(𝑑_1) = Ξ¦\sin(Ο‰_0𝑑_1 + Ξ³), Ξ¦ = π‘π‘œπ‘›π‘ π‘‘, Ξ³ = π‘π‘œπ‘›π‘ π‘‘,\tag{3.25}$$

describing the free harmonic oscillations by an independent variable $𝑑_1$ and in which the constant $Ξ³$ represents the angle of the phase difference. Therefore, as the solution $Ο†_0(𝑑_1)$ of the homogeneous differential equation (3.23), the harmonic function (3.25) is variable $𝑑_1$, it is bounded $Ο†_0(𝑑_1) = 𝑂(1)$ at an arbitrary long time interval $𝑑_1∈[0, ∞)$. It is necessary to provide this property also for the function $Ο†_1(𝑑_1, 𝑑_2)$ according to the variable $𝑑_1$, so that the approximate solution $Ο†(𝑑_1, 𝑑_2, ΞΎ)$ would not lose the character of the asymptotic function order, by the variable $𝑑_1$.

In order to solve the differential equation (3.24), the assumption ("Ansatz") is introduced that neither the amplitudes nor the phase difference are of constant size, but that they represent functions of the variable $𝑑_2$:

$$Ο†_0(𝑑_1, 𝑑_2) = Ξ¦(𝑑_2) \sin(Ο‰_0𝑑_1 + Ξ³(𝑑_2)).\tag{3.26}$$

The partial derivative of the function (3.26) by the variable $𝑑_1$ is given by the function:

$$\frac{πœ•Ο†_0}{πœ•π‘‘_1} = Ξ¦(𝑑_2)Ο‰_0\cos(Ο‰_0𝑑_1 + Ξ³(𝑑_2)) = Φω_0\cos ψ,\tag{3.27}$$

and the partial derivative of the function (3.27) by the variable $𝑑_2$ is given by the formula:

$$\begin{align}\frac{πœ•^2Ο†_0}{πœ•π‘‘_1πœ•π‘‘_2} &= \frac{πœ•Ξ¦(𝑑_2)}{πœ•π‘‘_2}Ο‰_0\cos(Ο‰_0𝑑_1 + Ξ³ (𝑑_2)) - Ξ¦(𝑑_2)Ο‰_0\sin(Ο‰_0𝑑_1 + Ξ³(𝑑_2))\frac{πœ•Ξ³(𝑑_2)}{πœ•π‘‘_2}\\ &= \frac{πœ•Ξ¦}{πœ•π‘‘^2}Ο‰_0\cos ψ - Ξ¦ \frac{πœ•Ξ³}{πœ•π‘‘^2}Ο‰_0\sinψ.\tag{3.28}\end{align}$$

For the sake of conciseness, the phase angle (phase) of oscillation was introduced $ψ = Ο‰_0𝑑_1 + Ξ³(𝑑_2)$. When the expressions (3.27) and (3.28) are included in the differential equation (3.24), the following equation is obtained:

$$\frac{πœ•^2Ο†_1}{πœ•π‘‘_1^2} + Ο‰_0^2Ο†_1 = 2Ξ¦\frac{πœ•Ξ³}{πœ•π‘‘_2}Ο‰_0\sin ψ - 2(\frac{πœ•Ξ¦}{πœ•π‘‘_2} + Φω_0) Ο‰_0\cos ψ.\tag{3.29}$$

The members on the right-hand side of equation (3.29), which contain the functions $\cos ψ$ and $\sin ψ$, represent members of the resonant coercion, as functions of time $𝑑_1$, and cause the solution of this differential equation to contain secular members. By eliminating the mentioned resonant coercive members in the differential equation (3.29), which are harmonic functions of variable $𝑑_1$, the secular members are eliminated from the solution $Ο†_1(𝑑_1, 𝑑_2)$ as functions of the same variable $𝑑_1$, thus ensuring that $Ο†_1(𝑑_1, 𝑑_2)$ is limited by the variable $𝑑_1$. By this procedure, the differential equation (3.29) becomes homogeneous, its solution $Ο†_1(𝑑_1, 𝑑_2)$ must be a harmonic function of the variable $𝑑_1$, which means that both it and the function $Ο†_0(𝑑_1, 𝑑_2)$ are limited by the variable $𝑑_1$ at a time interval $𝑑_1 ∈ [0, ∞)$. Annihilation of secular members is done by the following equations:

$$Ξ¦(𝑑_2) \frac{πœ•Ξ³(𝑑_2)}{πœ•π‘‘_2} = 0,\tag{3.30}$$ $$\frac{πœ•Ξ¦(𝑑2)}{πœ•π‘‘_2} + Ξ¦(𝑑_2)Ο‰_0 = 0.\tag{3.31}$$

As $Ξ¦(𝑑_2) ≠ 0$, from the equation (3.30) it follows immediately that the phase difference does not change with time, ie that it is constant: $Ξ³(𝑑_2) = Ξ³_0 = π‘π‘œπ‘›π‘ π‘‘$. The general solution of the differential equation (3.31) is:

$$Ξ¦(𝑑_2) = 𝐢𝑒^{-Ο‰_0𝑑^2}\tag{3.32}$$

in which the constant $𝐢 = π‘π‘œπ‘›π‘ π‘‘$ is determined from the initial conditions. As the equation (3.30) describes the exponential decrease in the amplitude of the free-damped oscillations with time $𝑑_2$, and it is limited by $𝑑_2∈[0, ∞)$. Replacement of the solution (3.32) in (3.26) gives the zero approximation of the differential equation (3.2), that is, the formula of the first member of the perturbation order:

$$Ο†_0(𝑑_1, 𝑑_2) = 𝐢𝑒^{-Ο‰_0𝑑^2} ∙ \sin (Ο‰_0𝑑_1 + Ξ³_0).\tag{3.33}$$

From the initial conditions given in (3.23), the constants $𝐢 = Ξ¦_0$ and $Ξ³_0 = Ο€/2$ are determined and the final expression for the zero approximation of the solution of the differential equation (3.2) in the function of time coordinates $𝑑_1$ and $𝑑_2$ is:

$$Ο†_0(𝑑_1, 𝑑_2) = Ξ¦_0𝑒^{-Ο‰0𝑑2} ∙ \cos Ο‰_0𝑑_1.\tag{3.34}$$

These are the exhausted possibilities for further solving the differential equation (3.24), so that the function $Ο†_1(𝑑_1, 𝑑_2)$ remains indeterminate. The approximate solution of the equation (3.2) is defined only as the zero "improved" approximation (3.34) of the perturbation order. By passing to the "regular" time coordinate $𝑑$, and in accordance with the equations $𝑑_1 = 𝑑$ and $𝑑_2 = ΞΎ ∙ 𝑑$, formula (3.34) becomes:

$$Ο†_0(𝑑) = Ξ¦_0𝑒^{-ΞΎΟ‰0𝑑} ∙ \cos Ο‰_0𝑑.\tag{3.35}$$

However, in spite of the fact that no analytical expression for the function $Ο†_1 (𝑑_1, 𝑑_2)$ has been defined, some of its essential characteristics are defined, on the axes where it is possible to estimate the order of the size of the remainder of the zero approximation $Ο†_0(𝑑)$, as well as the order of the time interval in which this approximation is valid. This assessment will also be proof of the validity of the implemented procedure for solving the differential equation (3.2) by the perturbation method of the double time scale. To evaluate the magnitude of the residue of the approximation and the time interval at which the scale can be used, it is necessary to discuss the properties of the asymptotic functional order,

$$Ο†(𝑑_1, 𝑑_2, ΞΎ) = Ο†_0(𝑑_1, 𝑑_2) + ΞΎΟ†_1 (𝑑_1, 𝑑_2) + O(ΞΎ^2) = Ο†_0(𝑑_1, 𝑑_2) + O(ΞΎ), ΞΎ∈(0,1),\tag{3.36}$$

which approximates the exact solution of the differential equation (3.2). First of all, the characteristic of asymptotic development (3.36) is that the order of the size of the approximation residue is equal to the order of the size of the first excluded member $ΞΎΟ†_1(𝑑_1, 𝑑_2) = O (ΞΎ)$, at some interval of variables $𝑑_1$ and $𝑑_2$. In the case of solving the differential equation (3.2) by the double time method, it is ensured that the function $Ο†_0(𝑑_1, 𝑑_2)$ is bounded $Ο†_0(𝑑_1, 𝑑_2) = O(1)$ by both variables $𝑑_1$ and $𝑑_2$, at intervals $𝑑_1∈ [0, ∞)$ and $𝑑_2∈ [0, ∞)$. By passing to the regular time coordinate $𝑑$, it follows immediately that the function $Ο†_0(𝑑)$ is bounded $Ο†_0(𝑑) = 𝑂(1)$, for $𝑑∈[0, ∞)$. By eliminating secular members from the function $Ο†_1(𝑑_1, 𝑑_2)$ according to the variable $𝑑_1$, its limit on the interval $𝑑_1∈[0, ∞)$ is also ensured. However, since the process of solving the differential equation (3.29), the elimination of secular members from the function $Ο†_1(𝑑_1, 𝑑_2)$ according to the variable $𝑑_2$ is not ensured, for the function $Ο†_1(𝑑_1, 𝑑_2)$ it can only be claimed [61] that $Ο†_1(𝑑_1, 𝑑_2) = O (1)$, at some final time interval $𝑑_2∈ [0, 𝑑_𝑀]$. By passing to the regular time coordinate, $𝑑_2 = ΞΎ ∙ 𝑑$, it follows that the function $Ο†_1(𝑑)$ is bounded $Ο†_1(𝑑) = 𝑂(1)$ at the final time interval $𝑑 ∈ [0, 𝑑_𝑀/ΞΎ]$ which is the order of the dimension factor $ΞΎ$ is longer than the interval $𝑑∈ [0, 𝑑_𝑀]$. From here it follows implicitly that $ΞΎΟ†_1 (𝑑_1, 𝑑_2) = O (ΞΎ)$, at $𝑑∈ [0, 𝑑_𝑀/ΞΎ], 𝑑 = 𝑂 (1/ΞΎ)$. For the fixed value of the damping factor $ΞΎ$, the conclusions are correct for each other value of the number $ΞΎ_1≤ΞΎ$, that is, the approximation is more accurate and valid for a longer time interval, if the attenuation factor is lower $𝑑_2$, for the function $Ο†_1(𝑑_1, 𝑑_2)$ can only be claimed [61] that $Ο†_1(𝑑_1, 𝑑_2) = O (1)$ is bounded according to the variable $𝑑_2$, at some final time interval $𝑑_2∈ [0, 𝑑_𝑀]$. By passing to the regular time coordinate, $𝑑_2 = ΞΎ ∙ 𝑑$, it follows that the function $Ο†_1 (𝑑)$ is bounded $Ο†_1 (𝑑) = 𝑂(1)$ at the final time interval $𝑑∈ [0, 𝑑_𝑀/ΞΎ]$ which is the order of the dimension factor ΞΎ is longer than the interval $𝑑∈ [0, 𝑑_𝑀]$. From here it follows implicitly that $ΞΎΟ†_1 (𝑑_1, 𝑑_2) = O (ΞΎ)$, at $𝑑∈ [0, 𝑑_𝑀/ΞΎ], 𝑑 = 𝑂(1/ΞΎ)$. For the fixed value of the damping factor $ΞΎ$, the conclusions are correct for each other value of the number $ΞΎ_1≤ΞΎ$, that is, the approximation is more accurate and valid for a longer time interval, if the attenuation factor is lower $𝑑_2$ for the function $Ο†_1(𝑑_1, 𝑑_2)$ can only be claimed [61] that $Ο†_1(𝑑_1, 𝑑_2) = O(1)$ is bounded according to the variable $𝑑_2$, at some final time interval $𝑑_2∈[0,𝑑_𝑀 ]$. By passing to the regular time coordinate, $𝑑_2 = ΞΎ ∙ 𝑑$, it follows that the function $Ο†_1(𝑑)$ is bounded $Ο†_1(𝑑) = 𝑂(1)$ at the final time interval $𝑑∈ [0, 𝑑_𝑀/ΞΎ]$ which is the order of the dimension factor $ΞΎ$ is longer than the interval $𝑑∈ [0, 𝑑_𝑀]$. From here it follows implicitly that $ΞΎΟ†_1(𝑑_1, 𝑑_2) = O(ΞΎ)$, at $𝑑∈[0, 𝑑_𝑀/ΞΎ], 𝑑 = 𝑂(1/ΞΎ)$. For the fixed value of the damping factor $ΞΎ$, the conclusions are correct for each other value of the number $ΞΎ_1≤ΞΎ$, that is, the approximation is more accurate and valid for a longer time interval, if the attenuation factor is lower.at some final time interval $𝑑_2∈ [0, 𝑑_𝑀]$. By passing to the regular time coordinate, $𝑑_2 = ΞΎ ∙ 𝑑$, it follows that the function $Ο†_1(𝑑)$ is bounded $Ο†_1(𝑑) = 𝑂(1)$ at the final time interval $𝑑∈ [0, 𝑑_𝑀/ΞΎ]$ which is the order of the dimension factor $ΞΎ$ is longer than the interval $𝑑∈ [0, 𝑑_𝑀]$. From here it follows implicitly that $ΞΎΟ†_1(𝑑_1, 𝑑_2) = O(ΞΎ)$, at $𝑑∈[0, 𝑑_𝑀/ΞΎ], 𝑑 = 𝑂(1/ΞΎ)$. For the fixed value of the damping factor $ΞΎ$, the conclusions are correct for each other value of the number $ΞΎ_1≤ΞΎ$, that is, the approximation is more accurate and valid for a longer time interval, if the attenuation factor is lower at some final time interval $𝑑_2∈ [0, 𝑑_𝑀]$. By passing to the regular time coordinate, $𝑑_2 = ΞΎ ∙ 𝑑$, it follows that the function $Ο†_1(𝑑)$ is bounded $Ο†_1(𝑑) = 𝑂(1)$ at the final time interval $𝑑∈[0, 𝑑_𝑀/ΞΎ]$ which is the order of the dimension factor $ΞΎ$ is longer than the interval $𝑑∈ [0, 𝑑_𝑀]$. From here it follows implicitly that $ΞΎΟ†_1 (𝑑_1, 𝑑_2) = O(ΞΎ)$, at $𝑑∈ [0, 𝑑_𝑀/ΞΎ], 𝑑 = 𝑂(1/ΞΎ)$. For the fixed value of the damping factor $ΞΎ$, the conclusions are correct for each other value of the number $ΞΎ_1≤ΞΎ$, that is, the approximation is more accurate and valid for a longer time interval, if the attenuation factor is lower $𝑑 = [0, 𝑑_𝑀/ΞΎ]$ which for the order of the dimension factor $ΞΎ$ is longer than the interval $𝑑∈ [0, 𝑑_𝑀]$. For the fixed value of the damping factor $ΞΎ$, the conclusions are correct for each other value of the number $ΞΎ_1≤ΞΎ$, that is, the approximation is more accurate and valid for a longer time interval, if the attenuation factor is lower.

On the basis of the above, it follows that

$$Ο†_0(𝑑) = 𝑂(1),\,\,\text{for}\,\, 𝑑∈ [0, 𝑑_𝑀/ΞΎ_1]\,\,\text{and for each}\,\,ΞΎ_1≤ΞΎ, ΞΎ∈ (0,1).\tag{3.37}$$

As for the error of approximation, which is calculated as the difference of the exact solution and its zero approximation, $|Ο†(𝑑, ΞΎ)-Ο†_0(𝑑, ξ𝑑)| = |ΞΎΟ†_1(𝑑, ξ𝑑)| = O(ΞΎ)$ then it follows immediately that there are constants $𝑐$, $ΞΎ_1$ and $𝑑_𝑀$ such that the exact solution $Ο†(𝑑, ΞΎ)$ satisfies the following condition:

$$|Ο†(𝑑, ΞΎ) - Ο†_0(𝑑, ξ𝑑) | ≤ 𝑐ξ,\,\,\text{for}\,\, 𝑑∈ [0 , 𝑑_𝑀/ΞΎ_1]\,\,\text{and for each}\,\, ΞΎ_1≤ΞΎ, ΞΎ∈(0,1).\tag{3.38}$$

This statement confirms that the approximate solution $Ο†_0(𝑑)$ asymptotically approaches the exact solution $Ο†(𝑑)$ at a time interval $𝑑∈ [0, 𝑑_𝑀/ΞΎ]$. By the proof of the theorem 5.2.1. In [61], Murdock confirms that the perturbation method of double time conditions can be successfully applied in solving both non-homogeneous differential equations that describe oscillatory processes. Theorem 5.2.1. has the same formal record as paragraph (3.38), as well as the same essence of the evidence presented here.



3.2. Perturbation method of averaging over Krylov and Bogoliubov

It has already been pointed out that the errors of the average impulse mechanisms are analyzed using the theory of perturbations, and not only by the method of the double time, but also by the technique of averaging by the Krilov method (Nikolai Mitrofanovich Krylov, 1879-1955) and Bogoliubov (Nikolay Nikolaevich Bogoliubov, 1909-1992). In this chapter, the essence of the mentioned method will be summarized, as well as its similarity to the double-timing method. The perturbation technique of Krylov and Bogoliubov is a mathematical procedure for the approximate analysis of nonlinear oscillatory processes, by replacing the exact differential equation with an approximate, simpler equation, formed by a special technique of averaging. Except in the analysis of nonlinear oscillations, it is used in heavenly mechanics, for example in the determination of slow planetary precession of periapsis.

Let the differential equation of the oscillations be given in the form:

$$\frac{𝑑^2𝑒}{𝑑𝑑^2} + Ο‰_0^2𝑒 = π‘Ž + Ξ΅ ∙ 𝑓(𝑒, \frac{𝑑𝑒}{𝑑𝑑});\, Ξ΅∈ (0,1),\, πœ€≪1.\tag{3.39}$$

If $Ξ΅=0$, the equation (3.39) describes a harmonic oscillator with constant force (force or momentum), and its solution is:

$$𝑒_0(𝑑) = aΟ‰_0^2 + A\sin (Ο‰_0𝑑 + 𝐡).\tag{3.40}$$

Constants $A$ and $B$ are determined from the initial conditions. If $Ξ΅≠0$, the solution (3.40) of the equation (3.39) has a small disorder, perturbation and, according to the Krylov and Bogoliubov method, is assumed in the same form, but so that $A$ and $B$ are no longer constants but represent the functions of time $t$ and the parameter $Ξ΅$. Therefore, the equation solution (3.39) when $Ξ΅≠0$ is sought in the form:

$$𝑒_0(𝑑) = aΟ‰_0^2 + A(𝑑) \sin (Ο‰_0𝑑 + 𝐡(𝑑)).\tag{3.41}$$

Since two unknown functions of time $t$ have been introduced, it is necessary to introduce some suitable restriction, that is, an additional condition. For this method, the following condition is introduced:

$$\frac{𝑑𝑒_0}{𝑑𝑑} = A(𝑑) Ο‰_0\cos (Ο‰_0𝑑 + 𝐡(𝑑)).\tag{3.42}$$

As $A$ and $B$ are functions of time $t$, the first derivative of the equation (3.41) is:

$$\frac{𝑑𝑒_0}{𝑑𝑑} = \frac{𝑑𝐴(𝑑)}{𝑑𝑑}\sin(Ο‰_0𝑑 + 𝐡(𝑑)) + 𝐴(𝑑)\cos(Ο‰_0𝑑 + 𝐡(𝑑)) ∙ (Ο‰_0 + \frac{𝑑𝐡(𝑑)}{𝑑𝑑}).\tag{3.43}$$

From the equations (3.42) and (3.43), the additional condition can be expressed concisely by the equation:

$$ \frac{𝑑𝐴(𝑑)}{𝑑𝑑}\sin(Ο‰_0𝑑 + 𝐡(𝑑)) + 𝐴(𝑑)\frac{𝑑𝐡(𝑑)}{𝑑𝑑}\cos (Ο‰_0𝑑 + 𝐡)) = 0.\tag{3.44}$$

In accordance with the expressions (3.41), (3.43) and (3.44), the differential equation (3.39) is equivalent to the following equation system:

$$ \frac{𝑑𝐴(𝑑)}{𝑑𝑑} = Ρω_0 𝑓(aΟ‰_0^2 + A(𝑑)\sin(ψ), \cos(ψ)) ∙ \cos (ψ),\tag{3.45}$$ $$\frac{𝑑𝐡(𝑑)}{𝑑𝑑} = πœ€πœ”_0𝑓(Π°πœ”_0^2 + А(𝑑)\sin(πœ“), \cos(πœ“))∙(−1𝐴(𝑑))\sin(πœ“),\tag{3.46}$$

where $ψ = Ο‰_0𝑑 + 𝐡(𝑑)$ phase angle (phase) oscillation.

The equations (3.45) and (3.46) are exact, because so far no approximation has been applied. Since the functions $𝐴(𝑑)$ and $𝐡(𝑑)$ change slowly with time (since $Ξ΅≪1$), the right sides of equations (3.45) and (3.46) can be approximated to their mean values ​​over a time interval $𝑑∈⌈0, 2Ο€/Ο‰_0⌉$ ie, $ψ∈⌈0,2Ο€⌉$. The approximation is performed by assuming that the functions $A$ and $B$ at the interval are constant and independent of time. In this way the equations

$$\frac{𝑑𝐴_{𝑆𝑅}(𝑑)}{𝑑𝑑} = \frac{Ξ΅}{2πω_0} \int_{0}^{2Ο€} 𝑓 \big(aΟ‰_0^2 + A\sin (ψ), cos (ψ)\big) ∙ cos (ψ) π‘‘Οˆ,\tag{3.47}$$ $$\frac{𝑑𝐡_{𝑆𝑅}(𝑑)}{𝑑𝑑} = \frac{Ξ΅}{2πω0} \int_{0}^{2Ο€} 𝑓 \big(aΟ‰_0^2 + A\sin (ψ), cos (ψ)\big) ∙ (-1𝐴) sin (ψ) π‘‘Οˆ,\tag{3.48}$$

which represent the very essence of the Krylov and Bogoliubov method. We point out once again that the functions $A$ and $B$, on the right-hand sides of equations (3.9) and (3.10), are inside the integral, the constants. After solving this system of differential equations (3.47-3.48), we can obtain approximately the solution of the differential equation (3.39), as the zero approximation, in the form:

$$𝑒_0(𝑑) = aΟ‰_0^2 + 𝐴_{𝑆𝑅}(𝑑) \sin (Ο‰_0𝑑 + 𝐡_{𝑆𝑅}(𝑑)).\tag{3.49}$$

The purpose of the described procedure is based on the assumption that the system of equations (3.47-3.48) is simpler to solve from the initial differential equation (3.39).

The error of the approximate solution is calculated as the difference of the exact solution of the differential equation (3.39) and its zero approximation $𝑒_0(𝑑)$ of the $𝑒(𝑑)$. An order of magnitude of this error, which assesses the accuracy of approximation

$$\big| 𝑒(𝑑, Ξ΅) - 𝑒_0(𝑑, Ξ΅) \big| = O(Ξ΅),\tag{3.50}$$

is equal to the order of magnitude $O(Ξ΅)$ omitted the first member of the perturbation asymptotic development of accurate solutions. Krylov and Bogoliubov proved the position that there are constants $𝑐$, $Ξ΅_1$ and $𝑑_𝑀$, such that the error of approximation (3.50) fulfills the following requirements:

$$\big| 𝑒(𝑑, Ξ΅) - 𝑒_0(𝑑, Ξ΅) | ≤ 𝑐 ∙ Ξ΅\,\, \text{for}\,\, 𝑑∈ [0, 𝑑_𝑀/Ξ΅] \,\, \text{and for each}\,\, Ξ΅_1 ≤ Ξ΅, Ξ΅∈ (0,1).\tag{3.51}$$

It should be noted that the interval of approximation validity, as in the double time scale method, is extended to the order of magnitude of the parameter of the disorder $Ξ΅$. For the fixed value of the parameter $Ξ΅$, the conclusions are also valid for each other value of the parameter $Ξ΅_1 ≤ Ξ΅$ ie, the approximation is more accurate and valid for a longer time interval, if the number $Ξ΅$ is smaller. The position (3.51) confirms that the approximate solution $𝑒_0(𝑑,Ξ΅)$ asymptotically approaches the exact solution $𝑒(𝑑,Ξ΅)$ at the time interval $𝑑∈[0, 𝑑_𝑀/Ξ΅]$. Enclosing the proof of this paragraph in [61], Murdock confirms the correctness of the perturbation method of Krylov and Bogoliubov as one possible heuristic procedure in the approximate solution of differential equations of the form (3.39). Since the differential equation (3.39) and the equations (3.47) and (3.48) represent only the mathematical models of a group of physical phenomena,the proof of the practical usability of this, as well as of other perturbation procedures, can be verified only by experiment or by computer simulation of these physical phenomena.

In this analysis, the equation (3.47) describes the expected slow change ($Ξ΅≪1$) of the amplitude of the oscillatory process and is coupled with the equation (3.48). For the purposes of our analysis, the equation (3.48) is particularly significant and interesting. It reveals that the phase difference $B$ of the oscillatory process is not constant, but that it changes slowly over time and describes the speed of that change, that is, the disturbance of the frequency of the oscillator $Ο‰_0$ caused by external coercion. If it is a clock oscillator, the equation (3.48) is just the formula for calculating the error of the average-impulse mechanism.

It is necessary to notice and discuss the similarity of the perturbation method of Krylov and Bogoliubov and the methods of two time conditions. First of all, a full consensus is found on the estimation of the order of the size of the error of approximation and the order of the size of the time interval to which this approximation is valid by both methods (3.51) and (3.52). The dual-time method introduces the coordinates of the "regular" time $𝑑$ and the coordinate of the "slow" time $Ρ𝑑$, thus, in general terms, explicitly separates the "fast" from the "slow" changes within the same dynamic process. The method of Krylov and Bogoliubov does not explicitly do so, but introduces the assumption that the functions $𝐴(𝑑)$ and $𝐡(𝑑)$ are changed so slowly in relation to the oscillation phase $ψ(𝑑)$ at the time interval $𝑑∈⌈0, 2Ο€/Ο‰_0⌉$, that it can be assumed that those at that time interval are approximately constant and independent of time.