Influence of the interstellar magnetic field and neutrals on the shape of the outer heliosphere

Space Science Reviews

Volumn 143, Issue 1-4, 2009, Pages 31-42

  Pogorelov, N V ^a   Heerikhuisen, J ^a   Zank, G P ^a   Borovikov, S N ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

ISM: kinematics and dynamics; Solar wind

Indexed keywords

CHARGE TRANSFER; DYNAMICS; HYDROGEN; KINEMATICS; MAGNETIC FIELDS; SOLAR SYSTEM; THREE DIMENSIONAL; TWO DIMENSIONAL;

ASPHERICITY; CHARGE EXCHANGES; CHARGED COMPONENTS; CONICAL SURFACES; FLOW VECTORS; GEOMETRICAL SIZES; HELIOPAUSE; HELIOSHEATH; HELIOSPHERE; INTERPLANETARY MAGNETIC FIELDS; INTERSTELLAR MAGNETIC FIELDS; INTERSTELLAR MEDIUMS; ISM: KINEMATICS AND DYNAMICS; MAGNETIC-FIELD; NEUTRAL HYDROGENS; OUTER HELIOSPHERE; PROBABLE ORIENTATIONS; RADIO EMISSIONS; TERMINATION SHOCKS; VELOCITY VECTORS;

SOLAR WIND;

EID: 61449195859     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/s11214-008-9429-x     Document Type: Article

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