The Ionospheric Response to the X-17 Solar Flare on September 07, 05: An Arecibo Perspective

Details The Ionospheric Response to the X-17 Solar Flare on September 07, 05: An Arecibo Perspective The Ionospheric Response to the X-17 Solar Flare on September 07, 05: An Arecibo Perspective

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsa23a..03v&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SA23A-03

Physics

2423 Ionization Processes (7823), 2441 Ionospheric Storms (7949), 2443 Midlatitude Ionosphere, 2447 Modeling And Forecasting

Scientific paper

The Arecibo Incoherent Scatter Radar captured the response of the middle latitude ionosphere to the major X17 class solar flare on September 07, 05 for the first time. Power profile of the radar returned electron density profile in the D, E and F region. The D region is being model using the Data Driven D region as the observed GOES X-ray was used to drive EUV ionization and electron heating, while the E-F region output comes from the Ionospheric Forecast Model. Initial results show good agreement between model output and observational data. The recurrent solar flare on September 8, 05 produced a more challenging data set for model to match as the electric field is being enhanced.

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