The predictability of the magnetosphere and space weather

Eos

Volumn 84, Issue 37, 2003, Pages

  Li, X ^a   Baker, D N ^b   Larson, D ^c   Temerin, M ^d   Kanekal, S G ^e  

^a UCB 428   (United States)

^b UNIVERSITY OF COLORADO   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d LOS ALAMOS NATIONAL LABORATORY   (United States)

^e CATHOLIC UNIVERSITY OF AMERICA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 70449836518     PISSN: 00963941     EISSN: None     Source Type: Journal    
DOI: 10.1029/2003EO370002     Document Type: Article

References (10)

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2. Baker, D. N., How to cope with space weather, Science, 297, 1486, 2002.
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4. Carrington, R. C, Description of a singular appearance seen in the Sun on September 1, 1859, M. Not. Roy. Ast. Soc., XX. 13, 1859.
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7. Li, X., M. Temerin, D. N. Baker, G. D. Reeves, and D. Larson, Quantitative prediction of radiation belt electrons at geostationary orbit based on solar wind measurements, Geophy. Res. Lett., 28, 1887, 2001.
8. Paulikas, G. A., and J. B. Blake, Effects of the solar wind on magnetospheric dynamics: Energetic electrons at the synchronous orbit, Quantitative Modeling of Magnetospheric Processes, 21, Geophys. Monograph Series, 1979.
9. Temerin M., and X. Li, A new model for the prediction of Dst on the basis of the solar wind, . / Geophys. Phys., 107, 1472, 2002.
10. Tsurutani, B. T., W. D. Gonzales, G. S. Lakhina, and S. Alex, The super magnetic storm of 1-2 September 1859, 7. Geophys. Phys., 2003.