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

E-ISSN： 1944-8007|42|21|9103-9112

ISSN： 0094-8276

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

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

Response of Mars O+ pickup ions to the 8 March 2015 ICME: Inferences from MAVEN data‐based models

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 9095-9102

John Wiley & Sons Inc

Access to resources Recommend Favorite

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

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

John Wiley & Sons Inc

Access to resources Recommend Favorite

The importance of pickup oxygen ion precipitation to the Mars upper atmosphere under extreme solar wind conditions

GEOPHYSICAL RESEARCH LETTERS, Vol. 40, Iss. 10, 2013-05 ,pp. : 1922-1927

John Wiley & Sons Inc

Access to resources Recommend Favorite

Solar wind interaction with the Martian upper atmosphere: Crustal field orientation, solar cycle, and seasonal variations

JOURNAL OF GEOPHYSICAL RESEARCH: SPACE PHYSICS, Vol. 120, Iss. 9, 2015-09 ,pp. : 7857-7872

John Wiley & Sons Inc

Access to resources Recommend Favorite

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