Is the geoeffectiveness of the 6 January 1997 CME predictable from solar observations?

Geophysical Research Letters

Volumn 24, Issue 23, 1997, Pages 2965-2968

  Zhao, X P ^a   Hoeksema, J T ^a  

^a STANFORD UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

GEOPHYSICS; MAGNETIC FIELD EFFECTS; SOLAR RADIATION;

CORONAL MASS EJECTION; GEOEFFECTIVENESS; MAGNETIC CLOUDS; MAXIMUM STRENGTH; PHOTOSPHERIC MAGNETIC FIELD; PREDICTION SCHEMES; SOLAR OBSERVATIONS;

EARTH SCIENCES; SUN;

CORONAL MASS EJECTION (CME); MAGNETIC CLOUDS; PHOTOSPHERIC MAGNETIC FIELD;

EID: 0031381005     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/97GL03000     Document Type: Article

References (6)

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2. Bothmer, V. and R. Schwenn, The interplanetary and solar causes of major magnetic storms, J. Geomag. Geoelectr., 47, 1127, 1995.
3. Tsurutani, B. T., W. D. Gonzalez, F. Tang, and Y. T. Lee, Great magnetic storms, Geophys. Res. Lett., 19, 73-76, 1992.
4. Wright, C. S., Catalog of solar filament disappearances 1964-1980, Report UAG-100, World Data Center A Solar Terrestrial physics, NOAA, Boulder, 1991.
5. Zhao, X. P., J. T. Hoeksema, J. T. Gosling, and J. L. Phillips, Statistics of IMF Bz events, in Solar-Terrestrial Predictions Workshop-IV, edited by J. Hruska et al., pp. 712-719, Natl. Oceanic and Atmospheric Administration, Boulder, Vol. 2, 1993.
6. Zhao, X. P. and J. T. Hoeksema, The central axial field direction in magnetic clouds and its relation to southward IMF events and dependence on disappearing solar filaments, J. Geophys. Res., , in press, 1997.