The October 22, 1989, solar cosmic ray enhancement: An analysis of the anisotropy and spectral characteristics

Journal of Geophysical Research: Space Physics

Volumn 102, Issue A11, 1997, Pages 24237-24248

  Cramp, J L ^a,b   Duldig, M L ^c   Fluckiger E O ^d   Humble, J E ^a   Shea, M A ^e   Smart, D F ^e  

^a UNIVERSITY OF TASMANIA   (Australia)

^b INST OF PHYS AND CHEMICAL RESEARCH   (Japan)

^c AUSTRALIAN ANTARCTIC DIVISION   (Australia)

^d UNIVERSITY OF BERN   (Switzerland)

^e AIR FORCE RESEARCH LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 37149013368     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/97JA01947     Document Type: Article

References (7)

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3. Bieber, J. W., and P. Evenson, Determination of energy spectra for the large solar particle events of 1989, Conf. Pap. Int. Cosmic Ray Conf. 22nd, 3, 129-132, 1991.
4. Bieber, J. W., P. Evenson, and M. A. Pomerantz, Focusing anisotropy of solar cosmic rays, J. Geophys. Res., 91, 8713-8724, 1986.
5. Torsti, J., A. Anttila, R. Vainio, and L. G. Kocharov, Successive solar energetic particle events in the October 1989, Conf. Pap. Int. Cosmic Ray Conf. 24th, 4, 139-142, 1995.
6. Tsyganenko, N. A., A magnetospheric magnetic field model with a warped tail current sheet, Planet. Sp. Sci., 37, 5-20, 1989.
7. Van Hollebeke, M. A. I., F. B. McDonald, and J. P. Meyer, Solar energetic particle observations of the 1982 June 3 and 1980 June 21 gamma-ray/neutron events, Astrophys. J. Suppl. Ser., 73, 285-296, 1990.