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Dependence of ionospheric response on the local time of sudden commencement and the intensity of geomagnetic storms
Institution:1. Radio and Atmospheric Physics Lab, Rajdhani College, University of Delhi, India;2. Department of Physics and Astrophysics, University of Delhi, India;3. Space Physics Laboratory, VSSC, Trivandrum, India;4. COSMIC Program Office, University Corporation for Atmospheric Research, Boulder, CO, USA;5. AORI, University of Tokyo, Japan;6. Department of Geophysics, Kyoto University, Kyoto, Japan
Abstract:A study has been designed specifically to investigate the dependence of the ionospheric response on the time of occurrence of sudden commencement (SC) and the intensity of the magnetic storms for a low- and a mid-latitude station by considering total electron content and peak electron density data for more than 60 SC-type geomagnetic storms. The nature of the response, whether positive or negative, is found to be determined largely by the local time of SC, although there is a local time shift of about six hours between low- and mid-latitudes. The time delays associated with the positive responses are low for daytime SCs and high for night-time SCs, whereas the opposite applies for negative responses. The time delays are significantly shorter for mid-latitudes than for low-latitudes and, at both latitudes, are inversely related to the intensity of the storm. There is a positive correlation between the intensity of the ionospheric response and that of the magnetic storm, the correlation being greater at mid-latitudes. The results are discussed in the light of the possible processes which might contribute to the storm-associated ionospheric variations.
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