| タイトル | Time Delay Between Dst Index and Magnetic Storm Related Structure in the Solar Wind |
| 本文（外部サイト） | http://hdl.handle.net/2060/20150018311 |
| 著者（英） | Fainberg, Joseph; Osherovich, Vladimir A. |
| 発行日 | 2015-05-12 |
| 言語 | eng |
| 内容記述 | Benson et al. (2015, this volume) selected 10 large magnetic storms, with associated Dst minimum values less than or equal to -100 nT, for which high-latitude topside ionospheric electron density profiles are available from topside-sounder satellites. For these 10 storms, we performed a superposition of Dst and interplanetary parameters B, v, N(sub p) and T(sub p). We have found that two interplanetary parameters, namely B and v, are sufficient to reproduce Dst with correlation coefficient cc approximately 0.96 provided that the interplanetary parameter times are taken 0.15 days earlier than the associated Dst times. Thus we have found which part of the solar wind is responsible for each phase of the magnetic storm. This result is also verified for individual storms as well. The total duration of SRS (storm related structure in the solar wind) is 4 - 5 days which is the same as the associated Dst interval of the magnetic storm. |
| NASA分類 | Geophysics |
| レポートNO | GSFC-E-DAA-TN25047 |
| 権利 | Copyright, Distribution under U.S. Government purpose rights |
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