Eclipse-induced changes to topside ion composition and field-aligned ion flows in the August 2017 solar eclipse: e-POP observations
We present in situ ion composition and velocity measurements during the August 2017 solar eclipse from the Enhanced Polar Outflow Probe (e-POP), which crossed the path of totality at similar to 640-km altitude within 10 min of totality passing. These measurements reveal two distinct H+ ion populations, an similar to 40% decrease in topside plasma density, a similar drop in upward but not downward H+ ion flux, and a downward O+ ion velocity of similar to 100 m/s. These features are directly linked to changes in the H+/O+ composition and in interhemispheric or field-aligned light ion flow and to a reduction in the negative spacecraft potential. These observed features were absent on the preceding, noneclipse days and corroborate the reduction in F region plasma density and topside total electron content observed by the Global Positioning System receivers on board. They are attributed to the temporary reduction of photoionization in the eclipsed F region.
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2016-01-01T00:00:00Z
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2018-10-28T00:00:00Z
Copyright 2018 American Geophysical Union.
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