Investigation of O+ and H+ 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.

Gkioulidou, Matina

Investigation of O⁺ and H⁺ 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.

Matina Gkioulidou¹, Shinichi Ohtani², Donald G Mitchell¹, Brian Larsen³ and Sarah K. Vines⁴, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)JHU/APL, Laurel, MD, United States, (3)Los Alamos National Laboratory, Los Alamos, NM, United States, (4)University of Texas at San Antonio, San Antonio, TX, United States