Investigation of O<SUP>+</SUP> and H<SUP>+</SUP> Properties During the Evolution of Two Intense Geomagnetic Storms: Implications for Solar Wind Conditions' Effect on the Abundance of Ionospheric vs. Solar Wind Plasma Source in the Inner Magnetosphere.

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ADS bibcode
2019AGUFMSM31A..02G
year
2019
Listed Authors
Gkioulidou, M.
Ohtani, S.
Mitchell, D. G.
Larsen, B.
Vines, S. K.
Listed Institutions
Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
JHU/APL, Laurel, MD, United States
Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Los Alamos National Laboratory, Los Alamos, NM, United States
University of Texas at San Antonio, San Antonio, TX, United States

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