Plasma Wave Scenario in Comets

V. Yadav
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引用次数: 1

Abstract

Plasma waves have a universal presence in our solar system – planets, some of their satellites and interplanetary medium. The solar plasma environment of also supports the generation of plasma waves such as electron and ion cyclotron waves, the magnetosonic and Alfven waves which travels a long distance in heliosphere. The plasma environment around a comet is also capable of sustaining plasma waves, some of which are observed in comets Giacobini-Zinner, Halley, Grigg-Skjellerup and Borrelly. Some other comets such as Hyakutake and 67/PChuryumov-Gerasimenko are also supposed to sustain plasma waves but are yet to be observed. This paper presents a brief review on the plasma wave observations in cometary plasma environment carried out so far and some of the unresolved plasma wave issues in comets.
彗星中的等离子体波
等离子体波在我们的太阳系——行星、它们的一些卫星和行星际介质中普遍存在。太阳等离子体环境也支持等离子体波的产生,如电子和离子回旋波、磁子波和阿尔芬波,它们在日球层中传播很远。彗星周围的等离子体环境也能够维持等离子体波,其中一些在Giacobini-Zinner, Halley, Grigg-Skjellerup和Borrelly彗星上观察到。其他一些彗星,如百武彗星和67/PChuryumov-Gerasimenko彗星,也被认为能维持等离子体波,但尚未被观测到。本文简要介绍了彗星等离子体环境中等离子体波观测到目前为止的一些进展,以及彗星等离子体波尚未解决的一些问题。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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