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Titlebook: Handbook of the Solar-Terrestrial Environment; Y. Kamide,A. Chian Book 2007 Springer-Verlag Berlin Heidelberg 2007 Climatology.Storm.Weath

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书目名称Handbook of the Solar-Terrestrial Environment
编辑Y. Kamide,A. Chian
视频video
概述A unique compendium on the Solar-Terrestrial Environment by the leading experts worldwide.Contains parts on the Sun and the Solar Wind, the Earth, Space Plasmas, and on Processes and Phenomena in the
图书封面Titlebook: Handbook of the Solar-Terrestrial Environment;  Y. Kamide,A. Chian Book 2007 Springer-Verlag Berlin Heidelberg 2007 Climatology.Storm.Weath
描述As a star in the universe, the Sun is constantly releas- cover a wide range of time and spatial scales, making ?? ing energy into space, as much as ?. ? ?? erg/s. Tis observations in the solar-terrestrial environment c- energy emission basically consists of three modes. Te plicated and the understanding of processes di?cult. ?rst mode of solar energy is the so-called blackbody ra- In the early days, the phenomena in each plasma diation, commonly known as sunlight, and the second region were studied separately, but with the progress mode of solar electromagnetic emission, such as X rays of research, we realized the importance of treating and UV radiation, is mostly absorbed above the Earth’s the whole chain of processes as an entity because of stratosphere. Te third mode of solar energy emission is strong interactions between various regions within in the form of particles having a wide range of energies the solar-terrestrial system. On the basis of extensive from less than ? keV to more than ? GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-e
出版日期Book 2007
关键词Climatology; Storm; Weather; Wind; comets; earth magnetosphere; geomagnetic storms; magnetic reconnection; s
版次1
doihttps://doi.org/10.1007/978-3-540-46315-3
isbn_softcover978-3-642-07968-9
isbn_ebook978-3-540-46315-3
copyrightSpringer-Verlag Berlin Heidelberg 2007
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978-3-642-07968-9Springer-Verlag Berlin Heidelberg 2007
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Magnetospherenamical influence of electric and magnetic fields, as well as under the influence of waves and instabilities, which the plasmas themselves control in turn. This chapter constitutes a largely theoretical overview of Earth’s magnetosphere and the physical processes that govern it.
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ABZ’2014 Conference. In the course of our development, we discovered some problems in our initial modeling approach. This has led us to propose a second approach and then a third one. Each approach is more efficient than the previous one in terms of proof obligations (roughly speaking: 2000, 1000,
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