Apposite of atmospheric electric parameters with the energy coupling function (ε) during geomagnetic storms at high latitude
Autor: | C. P. Anil Kumar, C. Panneerselvam, H. Johnson Jeyakumar, C. Selvaraj, Chandu Venugopal, K. U. Nair, Subramanian Gurubaran |
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Rok vydání: | 2009 |
Předmět: |
Geomagnetic storm
Atmospheric Science Ionospheric dynamo region Magnetosphere Geophysics Atmospheric sciences Physics::Geophysics Solar wind Earth's magnetic field Physics::Space Physics Astrophysics::Solar and Stellar Astrophysics Environmental science Atmospheric electricity Interplanetary magnetic field Physics::Atmospheric and Oceanic Physics Ring current |
Zdroj: | Atmospheric Research. 91:201-205 |
ISSN: | 0169-8095 |
DOI: | 10.1016/j.atmosres.2008.06.005 |
Popis: | In this paper we are concerned with the variation of the atmospheric electric field and the air–earth current due to the excessive power generated by the solar wind-magnetosphere dynamo during geomagnetic storms, recorded at Maitri in Antarctica during 2004. A major part of the power generated by the solar wind-magnetosphere dynamo is used in the formation of the ring current and the rest is utilized for Joule heating and auroral particle precipitation. The method adopted by Frank-Kamenetsky et al. [Frank-Kamenetsky A.V., Troshichev O.A., Burns G.B., Papitashvili V.O., 2001. Variations of atmospheric electric field in the near-pole region related to the interplanetary magnetic field. J. Geophys. Res. 106, A1, 179–190.] was utilized to delineate the variations due to the signatures of tropical thunderstorm activity from the geoelectric data; while statistical methods used in our earlier studies were used to delimit variation due to the constant buffeting of the solar wind. We find that the solar wind-magnetosphere energy coupling function (e) to be well correlated with the atmospheric electric parameters during the onset of geomagnetic disturbances. However the correlation breaks down during minor storms and sub-storm events. |
Databáze: | OpenAIRE |
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