Ulysses observations of the northward extension of the heliospheric current sheet

Geophysical Research Letters

Volumn 24, Issue 23, 1997, Pages 3101-3104

  Forsyth, R J ^a   Balogh, A ^a   Smith, E J ^b   Gosling, J T ^c  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c LOS ALAMOS NATIONAL LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELDS; SPACECRAFT OBSERVATORIES; SOLAR ENERGY;

HELIOSPHERE CURRENT SHEET; SOLAR WIND;

SUN; MAGNETIC FIELDS;

ACTIVE REGIONS; CURRENT SHEETS; HELIOSPHERES; HELIOSPHERIC CURRENT SHEET; HIGHER LATITUDES; POLAR REGIONS; SOLAR ACTIVITY; ULYSSES SPACECRAFT;

EID: 0031359664     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/97GL03099     Document Type: Article

References (8)

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2. Balogh, A., G. Erdös, R. J. Forsyth, and E. J. Smith, The evolution of the interplanetary' sector structure in 1992, Geophys. Res. Lett., 20, 2331-2334, 1993.
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6. Svalgaard, L., and J. M. Wilcox, The interplanetary magnetic field: A polarity and sunspot cycle variation, Science, 186, 51-53, 1974.
7. Wang, Y.-M., N. R. Sheeley, Jr., R. A. Howard, et al., Origin and evolution of coronal streamer structure during the 1996 minimum activity phase, Astrophys J., 485, 875-889, 1997.
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