During magnetic storm recovery at lunar distance, electron temperatures increase fourfold while ions increase less than twofold, accompanied by higher electrostatic fluctuation power, indicating electron energization in the magnetotail.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
physics.space-ph 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Properties of the Stormtime Plasma Sheet at the Lunar Distance
During magnetic storm recovery at lunar distance, electron temperatures increase fourfold while ions increase less than twofold, accompanied by higher electrostatic fluctuation power, indicating electron energization in the magnetotail.