TY - T1 - Electron Energy Partition across Interplanetary Shocks. III. Analysis SN - / UR - http://hdl.handle.net/10138/314673 T3 - A1 - Wilson, Lynn B.; Chen, Li-Jen; Wang, Shan; Schwartz, Steven J.; Turner, Drew L.; Stevens, Michael L.; Kasper, Justin C.; Osmane, Adnane; Caprioli, Damiano; Bale, Stuart D.; Pulupa, Marc P.; Salem, Chadi S.; Goodrich, Katherine A. A2 - PB - Y1 - 2020 LA - eng AB - An analysis of model fit results of 15,210 electron velocity distribution functions (VDFs), observed within 2 hr of 52 interplanetary (IP) shocks by the Wind spacecraft near 1 au, is presented as the third and final part on electron VDFs near IP shocks. The core electrons and protons dominate in the magnitude and change in the partial-to-total thermal pressure ratio, with the core electrons often gaining as much or more than the protons. Only a moderate positive correlation is observed between t... VO - IS - SP - OP - KW - Solar wind; Interplanetary shocks; Solar coronal mass ejections; Solar coronal mass ejection shocks; Space plasmas; Plasma astrophysics; Plasma physics; Interplanetary particle acceleration; QUASI-PERPENDICULAR SHOCKS; ION-ACOUSTIC INSTABILITY; HEAT-FLUX INSTABILITY; EARTHS BOW SHOCK; LOW-MACH-NUMBER; SOLAR-WIND; TEMPERATURE EQUILIBRATION; VELOCITY DISTRIBUTIONS; ANOMALOUS RESISTIVITY; COLLISIONLESS SHOCKS; 115 Astronomy, Space science N1 - PP - ER -