Latitudinal dependence of the radial IMF component: Coronal imprint

Geophysical Research Letters

Volumn 23, Issue 22, 1996, Pages 3267-3270

  Suess, S T ^a   Smith, E J ^b  

^a NASA MARSHALL SPACE FLIGHT CENTER   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELD MEASUREMENT; MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS; SOLAR RADIATION; SUN; MAGNETISM;

CORONAL MAGNETIC FIELDS; INTERPLANETARY MAGNETIC FIELD; SOLAR WIND; TRANSVERSE MAGNETIC PRESSURE GRADIENT FORCE;

MAGNETIC FIELDS; MAGNETOPLASMA;

IN-FIELD; INTERPLANETARY MAGNETIC FIELDS; LATITUDINAL GRADIENTS; MHD SIMULATION; RADIAL COMPONENT; TRANSVERSE MAGNETIC; ULYSSES;

EID: 0030284157     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/96GL02908     Document Type: Article

References (5)

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3. Burton, M. E., E. J. Smith, A. Balogh, and N. Murphy, Heliomagnetic latitude dependence of the heliospheric magnetic field, proc. of Solar Wind 8 (D. Winterhalter, D. McComas, N. Murphy, and J. Phillips, eds.), in press, 1995.
4. Wolfson, R., A coronal magnetic field model with volume and sheet currents, Astrophys. J., 288, 769, 1985.
5. Zhao, X.-P., and J. T. Hoeksema, Prediction of the interplanetary magnetic field strength, J. Geophys. Res., 100, 19-33, 1995.