Titlebook: Radiation in Astrophysical Plasmas; V. V. Zheleznyakov Book 1996 Kluwer Academic Publishers 1996 Astronomical Observation.Plasma.astronomy

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書目名稱Radiation in Astrophysical Plasmas影響因子(影響力)




書目名稱Radiation in Astrophysical Plasmas影響因子(影響力)學(xué)科排名




書目名稱Radiation in Astrophysical Plasmas網(wǎng)絡(luò)公開度




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書目名稱Radiation in Astrophysical Plasmas被引頻次學(xué)科排名




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書目名稱Radiation in Astrophysical Plasmas讀者反饋學(xué)科排名

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先驅(qū)

0067-0057 he discovery of radio emission from the Sun and Galaxywhich alerted theoretical radio astronomers to the problem of theorigin of extra-terrestrial radio emission. It has been found that theobserved radio emission from cosmic sources is generated by virtue ofthe mechanisms which work mainly in plasma

填滿

Introduction,mospheres, interstellar and interplanetary medium, planet ionospheres and magnetospheres) is mostly in a plasma state. The rare exceptions among radiation sources, such as planet surfaces and lower atmospheres, are not considered in this book. In this respect, the diversity in profiles and scales of

蔓藤圖飾

Electromagnetic waves in homogeneous plasma,rial are favoured. Complexity and the wide variety of wave processes in plasma, especially the magnetized one, forced us to restrict ourselves to only the theory of high-frequency waves. Their features are completely determined by the electrons, whereas the influence of ions is negligible. Such a re

anachronistic

arcane

Transfer of radiation in astrophysical plasmas,et of waves with wave vectors . from a phase space element . or wave packet, propagates along the rays, the curves tangential to the group velocity vector υ.. This vector in isotropic plasma is collinear with energy flux, or Poynting, vector. In magnetoactive plasma the time-average of the Poynting

KIN

Emission by astrophysical plasmas,e emission depends on its energy, the type of the motion in electric and/or magnetic fields, and on the properties of the surrounding medium. The major contributions to the emissivity of astrophysical plasma come from bremsstrahlung, ?erenkov, and magnetic bremsstrahlung emissions which are the main

Adjourn

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