Ionospheric and Thermospheric Response to Solar Activity on July 14, 2000.

Details Ionospheric and Thermospheric Response to Solar Activity on July 14, 2000. Ionospheric and Thermospheric Response to Solar Activity on July 14, 2000.

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sa51a07n&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SA51A-07

Physics

0355 Thermosphere--Composition And Chemistry, 2419 Ion Chemistry And Composition (0335), 7538 Solar Irradiance, 7549 Ultraviolet Emissions

Scientific paper

With the launch of the LORAAS sensor aboard the STP/P91-1 ARGOS mission and the follow-on UV sensors on DMSP missions covering the next decade, the scientific and operational communities will be able to assess quantitatively the response of the upper atmosphere to solar and geomagnetic forcing. Coincident observations of solar activity by the LASCO/EIT, CELIAS and SEM instruments aboard SOHO and of the resulting disturbances near Earth by WIND and ACE are analyzed. We report our continuing investigation of the relationships among these sets of observations to determine experimentally the timing and intensity of the thermospheric and ionospheric response to solar-induced geomagnetic forcing. We will focus on the sequence of events beginning with the July 14, 2000 solar flare and ensuing coronal mass ejection.

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