Confronting observations and modeling: The role of the interstellar magnetic field in voyager 1 and 2 asymmetries

Space Science Reviews

Volumn 143, Issue 1-4, 2009, Pages 43-55

  Opher, M ^a   Richardson, J D ^b   Toth, G ^c   Gombosi, T I ^c  

^a GEORGE MASON UNIVERSITY   (United States)

^b MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^c UNIVERSITY OF MICHIGAN   (United States)

Author keywords

Heliosheath; Heliosphere; Solar magnetic field; Solar system: Solar wind; Termination Shock

Indexed keywords

ASTRONOMY; ATOMS; HYDROGEN; MAGNETIC MATERIALS; MAGNETISM; SOLAR EQUIPMENT; SOLAR SYSTEM; SOLAR WIND; SPACE PROBES; SPACECRAFT; THREE DIMENSIONAL;

A PLANES; CURRENT MODELS; ENERGETIC PARTICLES; FIELD ORIENTATIONS; GALACTIC PLANES; HELIOPAUSE; HELIOSHEATH; HELIOSPHERE; HYDROGEN ATOMS; IN-SITU DATUM; IN-SITU MEASUREMENTS; INTERSTELLAR MAGNETIC FIELDS; INTERSTELLAR MEDIUMS; MAGNETIC EFFECTS; NUMERICAL MODELS; OBSERVATIONAL DATUM; OUTER HELIOSPHERE; RADIO EMISSIONS; SOLAR MAGNETIC FIELD; SPACE PHYSICS; STATE-OF-THE ARTS; TERMINATION SHOCK; VOYAGER 1;

MAGNETIC FIELD EFFECTS;

EID: 61449188970     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/s11214-008-9453-x     Document Type: Article

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