The Martian photoelectron boundary as seen by MAVEN
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DOI: 10.1002/2017ja024497
Abstract: Photoelectron peaks in the 20-30 eV energy range are commonly observed in the planetary atmospheres, produced by the intense photoionization from solar 30.4 nm photons. At Mars, these photoelectrons are known to escape the planet… read more here.
Keywords: escape; photoelectron boundary; photoelectron; field ... See more keywords