Latitudinal variation of the heliospheric magnetic field during solar minimum

Geophysical Research Letters

Volumn 23, Issue 22, 1996, Pages 3271-3274

  Bravo, S ^a   Stewart, G A ^a  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS; SOLAR RADIATION; SUN; EARTH SCIENCES; GEOPHYSICS;

INTERPLANETARY MAGNETIC FIELDS; RADIAL FIELD COMPONENT; SOLAR MINIMUM; SOLAR WIND;

MAGNETIC FIELDS;

HELIOSPHERIC MAGNETIC FIELDS; LATITUDINAL VARIATION; LOW LATITUDES; MHD MODELS; RADIAL COMPONENT; SOLAR MINIMA; ULYSSES;

EID: 0030285485     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/96GL03011     Document Type: Article

References (8)

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3. Smith, E. J. and A. Balogh, Ulysses' observations of the radial magnetic field, Geophys. Res. Lett., 22, 3317, 1995.
4. Stewart, G. A. and S. Bravo, Self consistent MHD modeling of the solar wind from polar coronal holes, in Solar Wind Eight, in press, 1996a.
5. Stewart, G. A. and S. Bravo, Latitudinal solar wind velocity variations from polar coronal holes: a self-consistent MHD model, submitted to J. Geophys. Res., 1996b.
6. Wang, Y. M., On the latitude and solar cycle dependence of the interplanetary magnetic field strength, J. Geophys. Res., 98, 3529, 1993.
7. Wolfson, R., A coronal magnetic field model with volume and sheet currents, Astrophys. J., 288, 769, 1985.
8. Zhao, X. and J. T. Hoeksema, Prediction of the interplanetary magnetic field strength, J. Geophys. Res., 100, 19, 1995.