抽象的

Magnetosphere Formation of A Tidally Locked Planet or Satellite

Deepanshu Chouhan

Magnetosphere is the part of a planet that contains the magnetic field lines that prevent harmful solar winds that can wipe out any kind of life by destroying the atmosphere of the planet. Some tidally locked planets were thought to lack this magnetosphere as they don’t have convection currents in their core, but recent studies of exo-planets have revealed that due to tidal heating, core of planets can melt. If the temperature inside the core excides a certain threshold then due to ionization the core can get partially charged producing a changing electric field which in turn can produce magnetic field.

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化学文摘社 (CAS)
谷歌学术
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学术钥匙
研究圣经
引用因子
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开放学术期刊索引 (OAJI)
参考搜索
哈姆达大学
印度科学网
学者指导
国际创新期刊影响因子(IIJIF)
国际组织研究所 (I2OR)
宇宙
日内瓦医学教育与研究基金会
秘密搜索引擎实验室

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