Coupling of the solar wind to measures of magnetic activity

Details Coupling of the solar wind to measures of magnetic activity Coupling of the solar wind to measures of magnetic activity

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.217..161m&link_type=abstract

In ESA Achievements of the Intern. Magnetospheric Study (IMS) p 161-166 (SEE N85-24544 14-46)

Other

3

Coupling Coefficients, Earth Magnetosphere, Linear Prediction, Solar Terrestrial Interactions, Solar Wind, International Magnetospheric Study, Interplanetary Magnetic Fields, Linear Filters, Solar Activity Effects

Scientific paper

Linear prediction filtering was used to generate empirical response functions relating the solar wind electric field to the magnetic indices, AL, AU, Dst and ASYM. The empirical response functions were convolved with solar wind observations obtained during the International Magnetospheric Study to predict the indices. The predictions are compared with the observed indices during two, 3-day intervals. Differences between the observed and predicted indices are discussed in terms of the linear assumption and in terms of physical processes other than direct solar wind-magnetosphere interaction.

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