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Geoeffectiveness (Dst and Kp) of interplanetary coronal mass ejections during 1995-2009 and implications for storm forecasting
We summarize the geoeffectiveness (based on the Dst and Kp indices) of the more than 300 interplanetary coronal mass ejections (ICMEs) that passed the Earth during 1996–2009, encompassing solar cycle 23. We subsequently estimate the probability that an ICME will generate geomagnetic activity that ex...
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Published in: | Space weather 2011-07, Vol.9 (7), p.np-n/a |
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Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | We summarize the geoeffectiveness (based on the Dst and Kp indices) of the more than 300 interplanetary coronal mass ejections (ICMEs) that passed the Earth during 1996–2009, encompassing solar cycle 23. We subsequently estimate the probability that an ICME will generate geomagnetic activity that exceeds certain thresholds of Dst or Kp, including the NOAA “G” storm scale, based on maximum values of the southward magnetic field component (Bs), the solar wind speed (V), and the y component (Ey) of the solar wind convective electric field E = −V × B, in the ICME or sheath ahead of the ICME. Consistent with previous studies, the geoeffectiveness of an ICME is correlated with Bs or Ey ≈ VBs in the ICME or sheath, indicating that observations from a solar wind monitor upstream of the Earth are likely to provide the most reliable forecasts of the activity associated with an approaching ICME. There is also a general increase in geoeffectiveness with ICME speed, though the overall event‐to‐event correlation is weaker than for Bs and Ey. Nevertheless, using these results, we suggest that the speed of an ICME approaching the Earth inferred, for example, from routine remote sensing by coronagraphs on spacecraft well separated from the Earth or by all‐sky imagers, could be used to estimate the likely geoeffectiveness of the ICME (our “comprehensive” ICME database provides a proxy for ICMEs identified in this way) with a longer lead time than may be possible using an upstream monitor.
Key Points
Summarize geomagnetic response of >300 ICMEs in cycle 23
Relate response to parameters of ICMEs including Bs, Ey, Vsw
Use Vsw results to estimate likely geoeffectiveness of an ICME observed remotely |
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ISSN: | 1542-7390 1542-7390 |
DOI: | 10.1029/2011SW000670 |