Internal relations between the solar plasma parameters at 1 AU and with the geomagnetic activity

Details Internal relations between the solar plasma parameters at 1 AU and with the geomagnetic activity Internal relations between the solar plasma parameters at 1 AU and with the geomagnetic activity

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3860s&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

We study internal relation and correlation between the plasma parameters observed near 1 AU during the last three cycles. The solar wind proton density N is positively correlated with both of its speed V and temperature T during the odd solar cycle and negatively correlated with them during the even cycles. The linear relation between T and V is independent upon the solar cycle. The solar wind speed V and entropy S as well as the interplanetary magnetic field B are correlated with the geomagnetic activity as characterized by the geomagnetic activity index Ap. The geomagnetic activity is well correlated with the product VB.

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