What Can We Learn about Geoffectiveness of Solar Wind Turbulence?

Details What Can We Learn about Geoffectiveness of Solar Wind Turbulence? What Can We Learn about Geoffectiveness of Solar Wind Turbulence?

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsm41a0331j&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SM41A-0331

Physics

2784 Solar Wind/Magnetosphere Interactions

Scientific paper

The interest of space weather and its forecasts grow and studies of geoeffective processes in coupled Sun - Solar wind - Magnetosphere - Ionoshere system rises. Recent results in understanding of the dynamical processes within this brought new questions in role of the fluctuations in solar wind plasma. In this paper we asked question whether these fluctuations do not play one of the important roles in geoeffective processes beside all these well-known parameters studied earlier and conditions which lead to the exchanges of mass, energy and momentum via reconnection processes. We examined changes in properties of magnetospheric disturbances characterized by Symh index by changes in properties of solar wind plasma and magnetic field fluctuations.

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