Three-dimensional features of the outer heliosphere due to coupling between the interstellar and interplanetary magnetic fields. I. Magnetohydrodynamic model: Interstellar perspective

Astrophysical Journal

Volumn 614, Issue 2 I, 2004, Pages 1007-1021

  Pogorelov, Nikolai V ^a,c   Zank, Gary P ^b   Ogino, Tatsuki ^c  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b NAGOYA UNIVERSITY   (Japan)

^c INSTITUTE FOR PROBLEMS IN MECHANICS   (Russian Federation)

Author keywords

ISM: kinematics and dynamics; ISM: magnetic fields; MHD; Shock waves; Solar wind

Indexed keywords

EID: 10044223505     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/423798     Document Type: Article

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