Dependence of Great Geomagnetic Storm ($\Delta $SYM-H$\le -200$ nT) on Associated Solar Wind Parameters
Authors:
- 15 April 2021
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 296 (4) , 1-14
Abstract
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Funding Information
- National Natural Science Foundation of China (41474166, 41074132, 41274193, 41774195, 41774085)
This publication has 28 references indexed in Scilit:
- Geoeffectiveness (Dst and Kp) of interplanetary coronal mass ejections during 1995–2009 and implications for storm forecastingSpace Weather, 2011
- Statistical Analysis of the Relationships among Coronal Holes, Corotating Interaction Regions, and Geomagnetic StormsSolar Physics, 2008
- Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23Geophysical Research Letters, 2008
- Magnetosheath variations during the storm main phase on 20 November 2003: Evidence for solar wind density control of energy transfer to the magnetosphereGeophysical Research Letters, 2005
- Solar wind density control of energy transfer to the magnetosphereGeophysical Research Letters, 2004
- An empirical formula relating the geomagnetic storm's intensity to the interplanetary parameters: − and ΔtGeophysical Research Letters, 2003
- Influence of the solar wind dynamic pressure on the decay and injection of the ring currentJournal of Geophysical Research, 2003
- Effect of solar wind velocity on magnetic cloud‐associated magnetic storm intensityJournal of Geophysical Research, 2002
- An empirical phase space analysis of ring current dynamics: Solar wind control of injection and decayJournal of Geophysical Research, 2000
- Geomagnetic response to magnetic clouds of different polarityGeophysical Research Letters, 1998