Energetic Particles and Auroras in Magnetosphere/Ionosphere(Physics Research and Technology)

磁层/电离层中的高能粒子和极光

地球科学史

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作      者
出  版 社
出版时间
2019年10月15日
装      帧
精装
ISBN
9781536159042
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页      码
540
语      种
英文
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图书简介
The importance and actuality of the geomagnetosphere’s research are based on following three factors:1. The geomagnetosphere is the nearest giant natural laboratory, where is possible by a lot of satellites and ground measurements investigate in details many different plasmas and energetic processes in space, caused finally by interaction of high kinetic energy solar wind plasmas and its perturbations (interplanetary coronal mass ejections – icmes, interplanetary shock waves – isws, interplanetary interaction regions – iir) with frozen in interplanetary magnetic fields – imf with the rotated main geomagnetic field. This interaction leads to dynamic transformation magnetic fields in geomagnetosphere, generation and trapping high energy particles (which can be called as magnetospheric cosmic rays – mcr), generation of many types instabilities and electromagnetic radiations. These processes are in principle similar to processes in magnetospheres of other planets and their moons, in the atmosphere of the sun and other stars, in interplanetary and in interstellar space, in many different astrophysical objects, i.E.
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