Quantization of natural energy pathways in space

IF 2.2 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Andrei Moldavanov
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Abstract

A phenomenon of energy transfer in space through a natural energy infrastructure shaped by confinement of the parameters of energy exchange is considered. The infrastructure consists of two interconnected energy spectra intrinsically stemming from the suggested model of an open thermodynamic system. The spectra are based on innate limitation imposed on the efficiency of energy exchange (primary spectrum) and the net passing energy (secondary spectrum). In this context, the primary spectrum creates the quantitative basis for realization of solution in the points of equilibrium, whereas the secondary spectrum forms the guiding energy tubes (GET) for bidirectional transfer between the distant energy points. According to the discussing theory, the family of GETs may be taken as the pathways for energy transfer with the observable signatures of spontaneous shaping, folding, and invariancy. Fundamentally, the conducted simulation for the event of energy transfer in the magnetosphere reveals the existence of connections between GET and the well-known magnetic flux tube, with the major advantage of GET in the more universal character of the underlying theory.
空间自然能量路径的量子化
考虑了能量交换参数限制形成的自然能量基础设施在空间中的能量转移现象。基础结构由两个相互连接的能谱组成,这些能谱本质上源于一个开放热力学系统的建议模型。光谱是基于对能量交换效率(一次光谱)和净通过能量(二次光谱)的固有限制。在这种情况下,一次光谱为平衡点解的实现提供了定量基础,而二次光谱则形成了引导能量管(GET),用于远距离能量点之间的双向传递。根据讨论理论,get族可以作为能量传递的途径,具有可观察到的自发成形、折叠和不变性特征。从根本上说,对磁层中能量传递事件的模拟揭示了GET与众所周知的磁通管之间存在联系,而GET的主要优势在于其基础理论具有更普遍的特征。
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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