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Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind

机译:太阳风中的卡古耶观察到血浆波和电子密度剖面的研究

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The moon has basically no intrinsic magnetic field and atmosphere, and plasma cavity called “Lunar Wake”' is created just behind the moon in the solar wind. Electrons which collided with moon surface are supposed to be carried toward downstream region of solar wind forming unique electron density distribution around the moon. In the present paper, we study electron density profile around the moon at nominal altitude of KAGUYA (~100km) in the solar wind controlled by the parameters such as IMF direction and solar wind velocity.
机译:月亮基本上没有内在的磁场和大气,并且在太阳风中的月亮后面形成了“月尾”的等离子体腔。 与月亮表面相撞的电子应该被带到太阳风的下游区域,形成在月球周围的独特电子密度分布。 在本文中,我们在诸如IMF方向和太阳风速等参数控制的太阳脉风中,在卡古耶(〜100km)的标称高度周围的电子密度剖面。

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