Physics
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh22a0852o&link_type=abstract
American Geophysical Union, Fall Meeting 2007, abstract #SH22A-0852
Physics
2162 Solar Cycle Variations (7536), 2164 Solar Wind Plasma, 2784 Solar Wind/Magnetosphere Interactions, 7524 Magnetic Fields, 7536 Solar Activity Cycle (2162)
Scientific paper
We reconstruct the magnitude of the interplanetary magnetic field B and solar wind speed v at 1 AU using 1) yearly values of sunspot numbers and geomagnetic index aa; 2) available spacecraft measurements of v and B since 1964. We compare our results with the reconstruction done by Stamper et al. (1999) and also with the reconstruction by Svalgaard et al. (2003). References Stamper, R., M. Lockwood and M.N. Wild, Solar causes of the long-term increase in geomagnetic activity, J. Geophys. Res., Vol.104 (A12), 24325, 1999. Svalgaard, Leif, E. W. Cliver and P. Lesager, In; Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2003, Tatranska Lomnica, Slovak Republic. Ed.:A. Wilson. ESA SP-535, Noorwijk: ESA Publications Division, IBSN 92-9092-845-X, 2003, p. 15 - 23
Fainberg Joe
Osherovich Vladimir A.
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