The multi-fluid pressures downstream of the solar wind termination shock

Author： Fahr H.-J.   Siewert M.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|558|issue|A41-A41

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.558, Iss.issue, 2013-10, pp. : A41-A41

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Entropy generation at multi-fluid magnetohydrodynamic shocks with emphasis to the solar wind termination shock

By Fahr H.-J.   Siewert M.  

Astronomy & Astrophysics, Vol. 576, Iss. issue, 2015-04 ,pp. : A100-A100

Edp Sciences

Access to resources Recommend Favorite

The electron distribution function downstream of the solar-wind termination shock: Where are the hot electrons?

By Fahr Hans J.   Richardson John D.   Verscharen Daniel  

Astronomy & Astrophysics, Vol. 579, Iss. issue, 2015-06 ,pp. : A18-A18

Edp Sciences

Access to resources Recommend Favorite

Supersonic solar wind ion flows downstream of the terminationshock explained by a two-fluid shock model

By  

Astronomy & Astrophysics, Vol. 490, Iss. 3, 2008-11 ,pp. : L35-L38

Edp Sciences

Access to resources Recommend Favorite

On the “injection problem” at the solar wind termination shock

By  

Astronomy & Astrophysics, Vol. 439, Iss. 1, 2005-08 ,pp. : 1-22

Edp Sciences

Access to resources Recommend Favorite

A kinetic description of the dissipative quasi-parallel solar wind termination shock

By  

Astronomy & Astrophysics, Vol. 487, Iss. 2, 2008-08 ,pp. : 723-729

Edp Sciences

Access to resources Recommend Favorite