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The electric wind of Venus: A global and persistent 'polar wind'-like ambipolar electric field sufficient for the direct escape of heavy ionospheric ions

机译:金星的电风:一种足以持久地重逸电离层离子直接逸出的整体持久性“极风”状双极性电场

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摘要

Understanding what processes govern atmospheric escape and the loss of planetary water is of paramount importance for understanding how life in the universe can exist. One mechanism thought to be important at all planets is an "ambipolar" electric field that helps ions overcome gravity. We report the discovery and first quantitative extraterrestrial measurements of such a field at the planet Venus. Unexpectedly, despite comparable gravity, we show the field to be five times stronger than in Earth's similar ionosphere. Contrary to our understanding, Venus would still lose heavy ions (including oxygen and all water-group species) to space, even if there were no stripping by the solar wind. We therefore find that it is possible for planets to lose heavy ions to space entirely through electric forces in their ionospheres and such an "electric wind" must be considered when studying the evolution and potential habitability of any planet in any star system.
机译:了解什么过程控制着大气逃逸和行星水的流失,对于理解宇宙中的生命如何生存至关重要。被认为对所有行星都重要的一种机制是“双极”电场,它可以帮助离子克服重力。我们报告了在金星行星上这种磁场的发现和首次定量外星测量。出乎意料的是,尽管重力相当,但我们显示出该场比地球类似的电离层强五倍。与我们的理解相反,即使太阳风没有剥夺金星,金星仍然会向太空失去重离子(包括氧气和所有水族物种)。因此,我们发现,行星有可能完全通过其电离层中的电力将重离子损失到太空,并且在研究任何恒星系统中任何行星的演化和潜在可居住性时必须考虑这种“电风”。

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