Contrasting behavior of the thermosphere and ionosphere in response to the 28 October 2003 solar flare

Author:

Liu Huixin1,Lühr Hermann2,Watanabe Shigeto1,Köhler Wolfgang2,Manoj C.3

Affiliation:

1. Earth and Planetary Science Division; Hokkaido University; Sapporo Japan

2. GeoForschungZentrum Potsdam; Potsdam Germany

3. Magnetotellurics Division; National Geophysical Research Institute; Hyderabad India

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference29 articles.

1. The response of the ionosphere to faint and bright solar flares as deduced from global GPS network data;Afraimovich;Ann. Geophys.,2002

2. Thermosphere density response to the 20-21 November 2003 solar and geomagnetic storm from CHAMP and GRACE accelerometer data;Bruinsma;J. Geophys. Res.,2006

3. Assimilated observations of thermospheric winds, the aurora, and ionospheric currents over Alaska;Conde;J. Geophys. Res.,2001

4. Ionospheric Radio

5. Contribution of X-ray and EUV bursts of solar flares to sudden frequency deviations;Donnelly;J. Geophys. Res.,1969

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