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... 
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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 
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ER  -