Numerical investigation of fluid models with full electron and proton thermal conduction equations for the quiet solar wind

1984 ◽  
Vol 286 ◽  
pp. 763 ◽  
Author(s):  
S. Cuperman ◽  
I. Tzur ◽  
M. Dryer

2018 ◽  
Vol 145 ◽  
pp. 03003
Author(s):  
Polya Dobreva ◽  
Monio Kartalev ◽  
Olga Nitcheva ◽  
Natalia Borodkova ◽  
Georgy Zastenker

We investigate the behaviour of the plasma parameters in the magnetosheath in a case when Interball-1 satellite stayed in the magnetosheath, crossing the tail magnetopause. In our analysis we apply the numerical magnetosheath-magnetosphere model as a theoretical tool. The bow shock and the magnetopause are self-consistently determined in the process of the solution. The flow in the magnetosheath is governed by the Euler equations of compressible ideal gas. The magnetic field in the magnetosphere is calculated by a variant of the Tsyganenko model, modified to account for an asymmetric magnetopause. Also, the magnetopause currents in Tsyganenko model are replaced by numericaly calulated ones. Measurements from WIND spacecraft are used as a solar wind monitor. The results demonstrate a good agreement between the model-calculated and measured values of the parameters under investigation.



2015 ◽  
Vol 114 (24) ◽  
Author(s):  
K. Horaites ◽  
S. Boldyrev ◽  
S. I. Krasheninnikov ◽  
C. Salem ◽  
S. D. Bale ◽  
...  


1978 ◽  
Vol 83 (A8) ◽  
pp. 3729 ◽  
Author(s):  
Steven Nerney ◽  
Aaron Barnes


1988 ◽  
Vol 93 (A9) ◽  
pp. 9547 ◽  
Author(s):  
Joseph V. Hollweg ◽  
Walter Johnson


2016 ◽  
Vol 154 ◽  
pp. 319-333 ◽  
Author(s):  
Kai Dong ◽  
Kui Liu ◽  
Lijian Pan ◽  
Bohong Gu ◽  
Baozhong Sun


1973 ◽  
Vol 20 (2) ◽  
pp. 519-520 ◽  
Author(s):  
S. Cuperman
Keyword(s):  




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