MHD model results of solar wind interaction with Mars and comparison with MAVEN plasma observations

E-ISSN： 1944-8007|42|21|9113-9120

ISSN： 0094-8276

Source： GEOPHYSICAL RESEARCH LETTERS, Vol.42, Iss.21, 2015-11, pp. : 9113-9120

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

MAVEN observations of solar wind hydrogen deposition in the atmosphere of Mars

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 8901-8909

John Wiley & Sons Inc

Access to resources Recommend Favorite

A comparison of 3‐D model predictions of Mars' oxygen corona with early MAVEN IUVS observations

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 9015-9022

John Wiley & Sons Inc

Access to resources Recommend Favorite

Multifluid MHD study of the solar wind interaction with Mars' upper atmosphere during the 2015 March 8th ICME event

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 9103-9112

John Wiley & Sons Inc

Access to resources Recommend Favorite

Comparison of model predictions for the composition of the ionosphere of Mars to MAVEN NGIMS data

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 8966-8976

John Wiley & Sons Inc

Access to resources Recommend Favorite

X rays from solar wind charge exchange at Mars: A comparison of simulations and observations

GEOPHYSICAL RESEARCH LETTERS, Vol. 31, Iss. 22, 2004-11 ,pp. : n/a-n/a

John Wiley & Sons Inc

Access to resources Recommend Favorite