Solar Cycle Variations Observed in the High-Latitude Ionosphere

Details Solar Cycle Variations Observed in the High-Latitude Ionosphere Solar Cycle Variations Observed in the High-Latitude Ionosphere

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsm44a..04k&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SM44A-04

Other

2435 Ionospheric Disturbances, 2447 Modeling And Forecasting, 2475 Polar Cap Ionosphere

Scientific paper

We have prepared an 11 year record of the high-latitude ionospheric environment using the AMIE data assimilation technique driven primarily by ground magnetometers. Using this data set we examine the difference in the response of the high-latitude ionosphere to similar input events as identified by IMF Bz, By, V, and density profiles. We look at the effect of the phase of the solar cycle, season, and other long time scale variations. We present the results as identified modes of the ionosphere and discuss the evolution from one to another over the scale of a solar cycle.

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