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Two-Step Forecast of Geomagnetic Storm Using Coronal Mass Ejection and Solar Wind ConditionTo forecast geomagnetic storms, we had examined initially observed parameters of coronal mass ejections (CMEs) and introduced an empirical storm forecast model in a previous study. Now we suggest a two-step forecast considering not only CME parameters observed in the solar vicinity but also solar wind conditions near Earth to improve the forecast capability. We consider the empirical solar wind criteria derived in this study (Bz ≤ −5 nT or Ey ≥ 3 mV/m for t ≥ 2 h for moderate storms with minimum Dst less than −50 nT) (i.e. Magnetic Field Magnitude, B (sub z) less than or equal to -5 nanoTeslas or duskward Electrical Field, E (sub y) greater than or equal to 3 millivolts per meter for time greater than or equal to 2 hours for moderate storms with Minimum Disturbance Storm Time, Dst less than -50 nanoTeslas) and a Dst model developed by Temerin and Li (2002, 2006) (TL [i.e. Temerin Li] model). Using 55 CME-Dst pairs during 1997 to 2003, our solar wind criteria produce slightly better forecasts for 31 storm events (90 percent) than the forecasts based on the TL model (87 percent). However, the latter produces better forecasts for 24 nonstorm events (88 percent), while the former correctly forecasts only 71 percent of them. We then performed the two-step forecast. The results are as follows: (i) for 15 events that are incorrectly forecasted using CME parameters, 12 cases (80 percent) can be properly predicted based on solar wind conditions; (ii) if we forecast a storm when both CME and solar wind conditions are satisfied (∩, i.e. cap operator - the intersection set that is comprised of all the elements that are common to both), the critical success index becomes higher than that from the forecast using CME parameters alone, however, only 25 storm events (81 percent) are correctly forecasted; and (iii) if we forecast a storm when either set of these conditions is satisfied (∪, i.e. cup operator - the union set that is comprised of all the elements of either or both), all geomagnetic storms are correctly forecasted.
Document ID
20150007958
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kim, R.-S.
(Korea Astronomy and Space Science Inst. Korea, Republic of)
Moon, Y.-J.
(Kyung Hee Univ. Yongin, Korea, Republic of)
Gopalswamy, N.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Park, Y.-D.
(Korea Astronomy and Space Science Inst. Korea, Republic of)
Kim, Y.-H.
(Korea Astronomy and Space Science Inst. Korea, Republic of)
Date Acquired
May 12, 2015
Publication Date
April 14, 2014
Publication Information
Publication: Space Weather
Publisher: American Geophysical Union
Volume: No. 4
Issue: Volume 12
Subject Category
Solar Physics
Geophysics
Report/Patent Number
GSFC-2015013P
GSFC-E-DAA-TN22609
Report Number: GSFC-2015013P
Report Number: GSFC-E-DAA-TN22609
Funding Number(s)
CONTRACT_GRANT: Korea-NRF-BRPF-20090071744
CONTRACT_GRANT: Korea-NRF-BRPF-20100014501
CONTRACT_GRANT: Korea-WCU-R31-10016
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
geomagnetic storm forecast
solar wind
coronal mass ejection
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