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Didactic conditions for the formation of technical competences of university students 大学生技术能力形成的教学条件
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.09
G.K. Nauryzbayeva
This paper discusses the issue of organizing professional-oriented training (POT) in physics for students of the educational program "Power Engineering" in order to form students' technical competencies, which are extremely necessary and important in the process of performing professional tasks in the future. The article presents the didactic conditions for the formation and development of technical competencies of university students, an example of a professionally oriented lecture on the topic of physics with an emphasis on the electric power industry, tasks for independent work of a student with technical content. Selected laboratory works on the considered topic of the section of mechanics are shown, which are necessary for fixing the lecture material. Particular attention is paid to the organization of the student's research work - attracting students to an effective, informative, and most importantly - professionally oriented research work of the student. The effectiveness of the organization of POT in physics is shown.
本文探讨了如何对“动力工程”专业的学生进行物理专业培训,以培养学生在未来执行专业任务过程中极为必要和重要的技术能力。本文介绍了大学生技术能力形成和发展的教学条件,并以以电力工业为重点的物理专业讲座为例,介绍了具有技术内容的学生独立工作的任务。所选的关于力学部分所考虑的主题的实验作品被展示,这是固定讲座材料所必需的。特别注意学生的研究工作的组织-吸引学生进行有效的,信息丰富的,最重要的是-以专业为导向的学生研究工作。证明了物理中组织POT的有效性。
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引用次数: 0
Simulation of atomization and ignition of high-pressure jet stream 高压喷射气流雾化与点火模拟
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.08
S. Bolegenova
This work is a significant study in terms of modern combustion physics of the problem of computer modeling of atomization, ignition, and combustion of high-pressure reactive liquid fuels under high turbulence. The need for a detailed study of the physical and chemical processes occurring during the combustion of reactive fuels is determined by the increased requirements for the efficiency of various technical devices, the accuracy of ignition prediction, and the combustion rate conditioned by the current environmental requirements for environmental protection. The processes of atomization, ignition, and combustion of atomized jet fuel (heptane) at high pressures were investigated using a numerical model. Numerical simulation methods were used to get profiles of the temperature plume, distribution of concentrations of the oxidizer, and reaction products (carbon dioxide and soot) in the combustion space. The optimum value of the initial pressure for heptane has been determined. The practical significance of the computational experiments presented in this paper is that the results obtained can be used in designing various reactive technical devices using combustion, which would simultaneously solve the problem of optimizing the process, increasing fuel combustion efficiency, and minimizing emissions of harmful substances.
这项工作是现代燃烧物理学中对高压反应性液体燃料在高湍流条件下雾化、点火和燃烧的计算机模拟问题的重要研究。对反应性燃料燃烧过程中发生的物理和化学过程进行详细研究的需要,是由对各种技术装置的效率、点火预测的准确性和当前环境保护要求所制约的燃烧速度的要求不断提高所决定的。采用数值模型研究了喷气燃料(庚烷)在高压下的雾化、点火和燃烧过程。采用数值模拟方法得到了燃烧空间内温度羽流、氧化剂浓度分布和反应产物(二氧化碳和烟尘)的分布。确定了庚烷的最佳初始压力值。本文计算实验的实际意义在于,所得结果可用于设计各种燃烧反应工艺装置,同时解决优化工艺、提高燃料燃烧效率和减少有害物质排放的问题。
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引用次数: 0
Electrochemical sensor for ascorbic acid based on zinc oxide nanostructures 基于氧化锌纳米结构的抗坏血酸电化学传感器
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.06
Zh.U. Paltusheva
Nanostructured semiconductor ZnO and ZnO-GO samples were synthesized at room temperature by chemical bath deposition technique. In this work, the electrochemical non-enzymatic determination of ascorbic acid was studied using the grown nanostructures deposited on a glassy carbon electrode. The morphology and structural properties of the synthesized nanostructured materials were analyzed using a scanning electron microscope and an X-ray diffractometer. The electrochemical properties were studied by the methods of cyclic voltammetry using a single-channel potentiostat-galvanostat. The sensitivity of the obtained electrodes was calculated based on concentrations of ascorbic acid in phosphate buffer solution from 0.3 mM to 3 mM at various scanning speeds. Thus, it was found that the sensitivity of the ZnO-GO sample is lower than that of the ZnO sample, which may be due to the dielectric properties of graphene oxide. However, after annealing in the atmosphere, the sensitivity of the ZnO-GO sample increased, which is associated with a decrease in defects in the sample and an increase in the specific surface area of the samples. As a result of the research, a modified ZnO-GO/GCE electrode with a high sensitivity of 386 μAM-1cm-2 was created, which is promising for use as the basis of a biosensor for determining the level of vitamin C in blood, food, and drugs.
采用化学浴沉积法在室温下合成了纳米结构的半导体ZnO和ZnO- go样品。本文研究了沉积在玻碳电极上的纳米结构对抗坏血酸的电化学非酶测定。利用扫描电子显微镜和x射线衍射仪对合成的纳米结构材料的形貌和结构特性进行了分析。采用单通道恒电位恒流器循环伏安法研究了其电化学性能。在不同的扫描速度下,根据磷酸盐缓冲溶液中抗坏血酸的浓度从0.3 mM到3 mM,计算所得电极的灵敏度。因此,我们发现ZnO- go样品的灵敏度低于ZnO样品,这可能是由于氧化石墨烯的介电性质。然而,在大气中退火后,ZnO-GO样品的灵敏度增加,这与样品中缺陷的减少和样品的比表面积的增加有关。通过此次研究,制备出了灵敏度高达386 μAM-1cm-2的ZnO-GO/GCE修饰电极,有望作为测定血液、食品、药品中维生素C含量的生物传感器的基础。
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引用次数: 0
Installation and technique of experimental investigations of composite materials based on beryllium 铍基复合材料实验研究的装置与技术
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.04
Ye.А. Kenzhin
Interest in beryllium-based composite materials has emerged recently, when intermetallic compounds such as titanium beryllide Be12Ti began to be considered as a promising material for neutron multiplication in thermonuclear fusion facilities, such as ITER and DEMO. Titanium beryllide stands out from other beryllides because it has the highest neutron multiplication rates and also has the added benefit of being more thermally stable than beryllium metal. Titanium beryllide interacts much weaker with water vapor, excluding the possibility of the formation of explosive hydrogen in the blanket body, is less prone to gas swelling, and, unlike metallic beryllium, retains a smaller amount of accumulated tritium. It has also been confirmed that the compatibility of titanium beryllide with structural materials is much higher than that of beryllium. To use titanium beryllide, it is important to study the parameters of its interaction with hydrogen isotopes. One of the most well-known methods for is the method of thermal desorption spectroscopy (TDS). The objective of this paper is the development of a specialized experimental setup for TDS research and the development of a methodology for performing experiments. The results of methodical experiments are presented, in which the procedures for saturation of samples in a deuterium medium and procedures for conducting TDS experiments were worked out. Methodical experiments on studying the parameters of the interaction of deuterium with samples of monolithic titanium beryllide were carried out on the material produced by Ulba Metallurgical Plant JSC, saturated in deuterium at atmospheric pressure and a sample temperature of 973 K. linear heating rates of 10 and 20 K/min. Based on the results of the development of the technique for conducting experimental studies of titanium beryllide, a differential mode of the TDS method was recommended. In this case, it is necessary to use a hydrogen isotope, deuterium, as a control probe.
当金属间化合物如铍化钛Be12Ti开始被认为是热核融合设施(如ITER和DEMO)中中子增殖的有前途的材料时,人们对铍基复合材料的兴趣最近出现了。铍化钛从其他铍化物中脱颖而出,因为它具有最高的中子增殖率,并且比铍金属更热稳定。铍化钛与水蒸气的相互作用要弱得多,排除了在毯体中形成爆炸性氢的可能性,不太容易发生气体膨胀,而且与金属铍不同,铍化钛保留了较少的累积氚。还证实了铍化钛与结构材料的相容性远高于铍。为了使用铍化钛,研究其与氢同位素相互作用的参数是很重要的。热解吸光谱法(TDS)是其中最著名的方法之一。本文的目的是为TDS研究开发一个专门的实验装置,并开发一种进行实验的方法。给出了系统的实验结果,给出了样品在氘介质中饱和的步骤和进行TDS实验的步骤。以Ulba冶金厂JSC生产的材料为材料,在常压下饱和氘,样品温度为973 K,线性加热速率为10和20 K/min,进行了研究氘与整体铍化钛样品相互作用参数的系统实验。根据铍化钛实验研究技术的发展结果,推荐了一种差别化的TDS方法。在这种情况下,有必要使用氢同位素氘作为控制探针。
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引用次数: 0
Calculation of thermomechanical stresses and deformations in a reactor ampoule device with lithium ceramics under neutron irradiation 中子辐照下锂陶瓷反应器安瓿装置的热力学应力和变形计算
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.05
Ye.V. Chikhray
Reactor experiments remain one of the few available methods for evaluating the performance of promising functional materials for fusion reactors under conditions of simultaneous exposure to neutron and gamma radiation, a gaseous environment, and thermal loads. Testing under neutron irradiation together with the application of numerical simulations (Finite Element Method) can lead to a complete understanding of the complex mechanical behavior of packed layers of pebbles by relating the macroscopic response of the infill to the microscopic interactions in a single pebble. The objective of this paper is describing the procedure and results of modeling of thermomechanical stresses and deformations that occur in the pebble bed of ceramic balls and in the irradiation device housing, in which the studied ceramic samples are placed during irradiation at the WWR-K reactor (Almaty, Kazakhstan). Calculation results show that ceramic pebbles, densely filled into the capsule of the WWR-K irradiation device so that they cannot move inside the filling, when heated to 1073K, will undergo thermomechanical loads from 10 to 80MPa, which exceeds the ultimate strength of 60MPa of ceramics Li4SiO4. The share of pebbles, the load on which exceeds the tensile strength, will be from 5 to 10% of their total number. In this case, the capsule will move down by 1-2mm, and expand by 200 microns radially under the influence of thermal elongation of the steel vacuum tubes connecting the capsule to the mounting flange. The strength of the tubes will not be affected. At a certain value of external pressure, the pebbles will abruptly move ("jump") into the empty area above the pebble bed, reducing the pressure on the remaining pebbles. It is not possible to describe such behavior within the framework of this model. The above calculations are relevant for the case of compacted pebble bed of lithium ceramics under neutron irradiation. A possible way to avoid the potential destruction of ceramic pebbles is to reduce the thickness of the capsule wall by 2-3 times, which will lead to an increase in the plasticity of the capsule walls, a decrease in the wall pressure on the pebble bed, and a decrease in the heating temperature of the capsule and ceramics.
在同时暴露于中子和伽马辐射、气体环境和热负荷的条件下,反应堆实验仍然是评估聚变反应堆中有前途的功能材料性能的少数可用方法之一。中子辐照试验结合数值模拟(有限元法)的应用,可以通过将填充物的宏观响应与单个卵石的微观相互作用联系起来,从而全面了解卵石充填层的复杂力学行为。本文的目的是描述在WWR-K反应堆(阿拉木图,哈萨克斯坦)辐照期间放置陶瓷样品的陶瓷球的球床和辐照装置外壳中发生的热机械应力和变形的建模过程和结果。计算结果表明,在wwrk - k辐照装置的胶囊内密集填充陶瓷卵石,使其无法在填料内移动,当加热到1073K时,将承受10 ~ 80MPa的热机械载荷,超过陶瓷Li4SiO4的极限强度60MPa。超过抗拉强度的卵石所占的份额将从其总数的5%到10%不等。在这种情况下,在连接胶囊与安装法兰的钢制真空管的热伸长的影响下,胶囊将向下移动1-2mm,并径向膨胀200微米。管子的强度不会受到影响。在一定的外部压力下,鹅卵石会突然移动(“跳”)到卵石床上方的空白区域,减少了对剩余鹅卵石的压力。在这个模型的框架内描述这样的行为是不可能的。上述计算与中子辐照下锂陶瓷球床压实的情况有关。避免陶瓷卵石潜在破坏的一种可能方法是将胶囊壁的厚度降低2-3倍,这样会导致胶囊壁的塑性增加,使球床上的壁压降低,使胶囊和陶瓷的加热温度降低。
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引用次数: 0
Development and synchronization of semiconductors excitation sources for active elements on self-terminatint transitions in metal vapors 金属蒸气中自终止跃迁的半导体元件激发源的研制与同步
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.07
N.A. Vasnev
The paper is devoted to development of atypical excitation approaches of bistatic laser monitor active elements for the imaging of high-speed processes at a powerful background radiation. The practical significance is increasing the temporal resolution of the bistatic laser monitor, as well as improving the imaging parameters by minimizing the jitter of radiation pulses. To achieve this goal, semiconductor excitation sources of active media based on copper bromide vapor were developed, and their synchronization was performed in a pulse-repetition mode. The developed pump sources are set of identical commutation cells. Each cell contains storage capacitor, commutator and transformer. Powerful HGTG27N120BN insulated-gate bipolar transistors (IGBT) were chosen as commutators. Their switching storage capacitors are discharged through the primary winding of the transformer and as result the voltage pulse is induced in the secondary winding. The transformer load was the gas discharge tube (GDT) of the small-size brightness amplifier with the specified geometric parameters (l=40 cm, d=2.5 cm, V=196 cm3). The simultaneous switching of 10 identical cells provided GDT breakdown. The radiation power of the active element in oscillator mode was 665 mW. The developed brightness amplifier with semiconductor pump source was used in the bistatic scheme of the laser monitor for the imaging of the test object. The pumping of the second active element, the illumination source (l=90 cm, d=5 cm, V=1767 cm3), was performed by means of thyratron TGI1-1000-25. The pulse repetition frequency of the illumination source and the brightness amplifier was 10,5 and 21 kHz respectively. As result each second image was formed with increased brightness and contrast. The maximal jitter of radiation pulses in this case was 16 ns. The average jitter was 6 ns. Two identical semiconductor pump sources were tested simultaneously. The resulting array of waveforms (GDT current and GDT voltage) show that in most cases the jitter was completely absent, and when it appeared, it did not exceed 4 ns. The imaging at this configuration of the pump sources was not performed due to semiconductor source power (465 W) turned out to be insufficient for the excitation of the illumination source, and therefore options for increasing it were proposed.
本文研究了双基地激光监测有源元件在强背景辐射下高速成像的非典型激发方法。其实际意义在于提高双基地激光监测仪的时间分辨率,并通过减小辐射脉冲的抖动来改善成像参数。为了实现这一目标,开发了基于溴化铜蒸汽的活性介质半导体激励源,并以脉冲重复模式进行了同步。开发的泵源是一组相同的换向电池。每个电池包含存储电容器、换向器和变压器。换向器选用高性能的HGTG27N120BN绝缘栅双极晶体管(IGBT)。它们的开关存储电容器通过变压器的初级绕组放电,因此在次级绕组中感应电压脉冲。变压器负载为指定几何参数(l=40 cm, d=2.5 cm, V=196 cm3)的小型亮度放大器气体放电管(GDT)。同时切换10个相同的电池提供GDT击穿。振荡模式下有源元件的辐射功率为665 mW。研制的半导体泵浦源亮度放大器应用于激光监视器的双基地方案中,对被测对象进行成像。第二个有源元件,即照明源(l=90 cm, d=5 cm, V=1767 cm3),通过闸流管tg1 -1000-25进行泵送。照明光源和亮度放大器的脉冲重复频率分别为10、5和21 kHz。结果,每一幅图像的亮度和对比度都有所增加。在这种情况下,辐射脉冲的最大抖动为16ns。平均抖动为6 ns。同时测试了两个相同的半导体泵源。得到的波形阵列(GDT电流和GDT电压)表明,在大多数情况下,抖动完全不存在,当它出现时,它不超过4 ns。由于半导体源功率(465 W)不足以激发照明源,因此没有在这种泵源配置下进行成像,因此提出了增加它的选项。
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引用次数: 0
Formation of students' research abilities while studying the discipline "Optics" 在“光学”学科学习过程中学生科研能力的形成
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.010
R.А. Zhunussova
The article describes the methods for developing the research skills of future physics teachers in the process of studying optics at a university. The purpose of this study is to improve the research abilities of students in lectures, practical and laboratory classes in optics. In the course of pedagogical research, we developed a model for the formation of readiness for research activities in the school of future physics teachers and formed the criterion and tools for determining readiness, which were applied during the teaching of optics. And also, a number of pedagogical conditions are defined, which, in our opinion, form the research competencies of students. Methods of problem-based learning, practice-oriented learning, methods of analysis and synthesis, methods of observation were applied. The relevance of the research topic lies in the problem of preparing future teachers of physics for organizing research activities with schoolchildren. Therefore, we have developed and tested the educational and methodological complex "Optics", proposed methods, forms, criteria for evaluating the research skills of future physics teachers. The presented methodology for the formation of research competence can be used for teaching other basic disciplines. The results of the research will be relevant for teachers of pedagogical universities who are looking for effective ways to train future specialists who are able to qualitatively prepare students for research activities.
本文阐述了在大学光学专业学习过程中培养未来物理教师科研能力的方法。本研究的目的在于提高学生在光学课堂、实务及实验中的研究能力。在教学研究过程中,我们开发了未来物理教师学校研究活动准备形成的模型,并形成了确定准备的标准和工具,并在光学教学中应用。此外,我们还定义了一些教学条件,在我们看来,这些条件形成了学生的研究能力。采用问题导向学习方法、实践导向学习方法、分析综合方法、观察法等。本研究课题的相关性在于培养未来的物理教师与学童一起组织研究活动的问题。因此,我们开发和测试了教育和方法论复杂的“光学”,提出了评估未来物理教师研究技能的方法、形式和标准。本文提出的研究能力形成方法可用于其他基础学科的教学。这项研究的结果将与师范大学的教师有关,他们正在寻找有效的方法来培养未来的专家,这些专家能够为学生的研究活动做好素质准备。
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引用次数: 0
Search and identification of young stellar objects in infrared dust bubbles N19 红外尘埃泡N19中年轻恒星物体的搜索和识别
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.02
A.M. Alisher
Соңғы жылдары ғарыш кеңістігіндегі денелер мен сәулеленудің өзара әрекеттесуін зерттейтін астрофизика ғылымының қарқынды дамуы, сондай-ақ аспан денелерін бақылаудың жаңа әдістерінің пайда болуы жұлдыз аралық ортада физикалық процестерді мұқият зерттеуге мүмкіндік беріп келеді. Жұлдыздардың пайда болу мұмкіндігі жұлдызаралық газ бен тозаңның тығыздығы мен мөлшеріне байланысты, ал жұлдыздар қоршаған жұлдызаралық ортаның қасиеттерін өзгертеді, оны қыздырады, газдың үздіксіз қозғалысын қолдайды және қоршаған ортаны өз заттарымен толықтырып, оның химиялық құрамын өзгертеді. Ұсынылған жұмыста бірінші рет N19 инфрақызыл тозаңды көпіршік аймағында жас жұлдыз объектілеріне іздеу жүргізілді. Таңдалған қажеттеі критерийлер бойынша жас жұлдыз объектілерін іздеуге арналған компьютерлік ортады MatLab математикалық модельдеу бағдарламасы жасақталды. Табылған инфраақызыл сәулелену көздерінен І класс жас жұлдыздарына жататын 11 объект, ал ІІ классқа 26-сы және  20-сы өтпелі диск сатысындағы жас жұлдыз объектісі болатыны анықталды. Нәтижесінде инфрақызыл N19 тозаңды көпіршік маңында жас жұлдыз нысандарына үміткерлер үшін  “түс-түс” диаграммасы тұрғызылған. Сонымен қатар, түс көрсеткіштерінің өзгеру диапазондары талданған және осы диаграмма жас жұлдыз объектілерін олардың эволюциялық сатысына сәйкес анықтаудың жаңа критерийлерді айқындауға мүмкіндік беретіндігін көрсетілген.
这样做会导致设备发生故障或损坏设备内部和天体物理学。 这样做会导致设备发生故障或损坏设备内部、这样做将导致设备无意中变得危险,并可能导致火灾或触电。这样做可能会导致发生火灾或电击,可能会导致发生火灾或电击,可能会导致对环境造成火灾或电击、这样做可能会导致设备损坏、供气系统损坏或设备内部损坏,以及设备化学性质损坏。打开 N19 红外线灯时,这样做将导致火灾或触电。请勿将计算机化的 MatLab 数学模型与计算机化的对象控制器一起使用。一年级使用 11 个对象,二年级使用 26-sy 和 20-sy 圆盘。这样做可能会导致火灾或电击,如火灾或电击,可能会导致火灾或电击。如果您不想使用该图,请不要让该物体演变,也不要将其作为标准。
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引用次数: 0
Determination of physical parameters of the W40 HII region using observations of Н110a radio recombination line 利用Н110a射电重组线观测确定W40 HII区域的物理参数
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.01
A.B. Manapbayeva
HII regions are ionized regions of interstellar gas, which ionized by intensive ultraviolet radiation from nearby hot stars. Radio recombination line is one of the main tools for investigating the HII region, in particular, the distribution of HII is obtained and the main physical conditions of the interstellar matter are determined from hydrogen lines. This study was carried out based on the analysis of the H110a recombination emission line toward the W40 HII region, which is one of the most active star-forming regions in the Aquila Molecular Cloud. We used archival observational data of the H110a radio recombination line in the Aquila Molecular Cloud, obtained during February in 2015 using the 26m NanShan radiotelescope in the Xinjiang Astronomical Observatory of the Chinese Academy of Sciences. During the period of the study, an integrated intensity map of H110a toward the W40 HII region and the corresponding spectra were constructed. The electron density and temperature of the HII region, the emission measure, the optical thickness, the Lyman continuum flux, the excitation parameter, the radius of the Strömgren sphere, and the mass of ionized hydrogen inside the sphere were calculated. The values of the emission measure and optical thickness indicate that the H110a recombination radio line is optically thin and traces a very dense region (<6462 AU) with a high electron temperature. The numbers of photons of the Lyman continuum indicates the presence of a massive O9.5 star, that equivalent to a zero-age main-sequence star located within the HII region. The obtained values of the physical parameters indicate that the region of ionized hydrogen under study is an ultracompact region. The results of this article lay the foundation for further research aimed at studying the evolution of HII regions, as well as their role in the processes of starformation.
HII区域是星际气体的电离区域,它被附近热恒星强烈的紫外线辐射电离。射电复合谱线是研究HII区域的主要工具之一,特别是通过氢谱线获得HII的分布,确定星际物质的主要物理条件。本研究是基于对Aquila分子云中最活跃的恒星形成区之一W40 HII区域的H110a重组发射线的分析进行的。我们使用了2015年2月中国科学院新疆天文台26m南山射电望远镜在Aquila分子云中获得的H110a射电重组线的档案观测数据。在研究期间,构建了H110a向W40 HII区域的综合强度图和相应的光谱。计算了HII区的电子密度和温度、发射量、光学厚度、莱曼连续通量、激发参数、Strömgren球半径和球内电离氢的质量。发射测量值和光学厚度表明,h10a复合射电谱线在光学上很薄,并在高电子温度下追踪到一个非常致密的区域(<6462 AU)。莱曼连续体的光子数量表明存在一颗巨大的O9.5恒星,相当于一颗位于HII区域的零年龄主序星。得到的物理参数值表明,所研究的电离氢区域是一个超紧区。本文的研究结果为进一步研究HII区域的演化及其在恒星形成过程中的作用奠定了基础。
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引用次数: 0
Physical fields as factors of natural processes in the works of the center for astrophysical research of North Kazakhstan University 北哈萨克斯坦大学天体物理研究中心工作中作为自然过程因素的物理场
Pub Date : 2023-09-01 DOI: 10.26577/rcph.2023.v86.i3.03
A.A. Solodovnik
Some features of the approach to solving both purely practical and general theoretical problems based on the application of the field approach as a causal factor in the development of a number of phenomena are considered. In particular, when studying the genesis and evolution of mesospheric silvery clouds, the determining influence of a number of large-scale tropospheric processes on their development is consistently revealed. An original method of synthetic maps is proposed in this direction. Extensive statistical analysis of the cartographic material revealed that cyclonic activity, frontogenesis, development of occlusions and thunderstorm foci have a pronounced physical effect on the formation of silvery clouds over the northern hemisphere. The extraordinary results of the work stimulated further study of the influence of the temperature field of high latitudes in the southern hemisphere of the Earth – Antarctica – on the features of the seasonal evolution of the area of the global field of silvery clouds of the southern hemisphere. For the first time in research practice, statistically convincing evidence has been obtained that the surface temperature field is the leading factor in the formation of silvery clouds. This makes it possible, in turn, to consider silvery clouds as a significant marker of climate change. Along with this, longitude variations of the area of silvery clouds of the northern hemisphere of the Earth are considered. The results suggest the influence of geophysical fields on the genesis of such clouds. The question of the nature of gravitational and inert coupling is considered separately. A hypothesis has been put forward that allows not only to clarify the view of the nature of the inert mass, but also to estimate several general characteristics of the Universe relatively simply. The work is completed by a proposal to take a fresh look at the physical nature of information, based on the field method.
该方法的一些特点,以解决纯实践和一般的理论问题为基础的应用领域的方法作为一个因果因素的发展,在一些现象被考虑。特别是在研究中间层银云的形成和演化时,不断揭示了一些大尺度对流层过程对银云发展的决定性影响。在此方向上提出了一种新颖的合成地图方法。对地图资料的广泛统计分析显示,气旋活动、锋生、闭塞的发展和雷暴焦点对北半球银色云的形成有显著的物理影响。这项工作的非凡成果促使人们进一步研究地球南半球(南极洲)高纬度地区的温度场对南半球全球银色云场区域季节性演变特征的影响。在研究实践中,首次获得了统计上令人信服的证据,表明地表温度场是银云形成的主导因素。反过来,这使得将银色云视为气候变化的重要标志成为可能。与此同时,还考虑了地球北半球银色云区域的经度变化。结果表明地球物理场对这种云的形成有影响。重力耦合和惰性耦合的性质问题是分开考虑的。有人提出了一个假说,它不仅可以澄清惰性物质的性质,而且可以相对简单地估计宇宙的几个一般特征。这项工作是通过一项建议来完成的,该建议以现场方法为基础,重新审视信息的物理性质。
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Recent Contributions to Physics
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