TY  -  
T1  - The Response of the Venusian Plasma Environment to the Passage of an ICME : Hybrid Simulation Results and Venus Express Observations 
SN  -  /  
UR  - http://hdl.handle.net/10138/308356 
T3  -  
A1  - Dimmock, A. P.; Alho, M.; Kallio, E.; Pope, S. A.; Zhang, T. L.; Kilpua, E.; Pulkkinen, T. I.; Futaana, Y.; Coates, A. J. 
A2  -  
PB  -  
Y1  - 2018 
LA  - eng 
AB  - Owing to the heritage of previous missions such as the Pioneer Venus Orbiter and Venus Express, the typical global plasma environment of Venus is relatively well understood. On the other hand, this is not true for more extreme driving conditions such as during passages of interplanetary coronal mass ejections (ICMEs). One of the outstanding questions is how do ICMEs, either the ejecta or sheath portions, impact (1) the Venusian magnetic topology and (2) escape rates of planetary ions? One of the... 
VO  -  
IS  -  
SP  -  
OP  -  
KW  - SOLAR-WIND INTERACTION; MAGNETIC-FIELD; BOW SHOCK; ION ESCAPE; PIONEER VENUS; O+ IONS; WAVES; UPSTREAM; MISSION; MARS; 115 Astronomy, Space science 
N1  -   
PP  -  
ER  -