Response of the auroral ionosphere to solar wind parameter variations

Details Response of the auroral ionosphere to solar wind parameter variations Response of the auroral ionosphere to solar wind parameter variations

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990angeo...8..353s&link_type=abstract

Annales Geophysicae (ISSN 0992-7689), vol. 8, May 1990, p. 353-356.

Physics

Auroral Zones, Ionospheric Electron Density, Solar Terrestrial Interactions, Solar Wind, Cross Correlation, Eiscat Radar System (Europe), Temporal Distribution, Upper Ionosphere

Scientific paper

Cross-correlation studies between solar wind parameters and electron densities in the auroral ionosphere measured by EISCAT show that different regions in the ionosphere respond differently to solar wind parameter changes. The strongest correlation was found for the densities in the upper ionosphere and the solar wind parameter V x Bs which is related to the magnetospheric electric field.

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