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太陽雑誌会 2003/4/28 殿岡 英顕. Prominence Eruption and Coronal Mass Ejection: A Statistical Study Using Microwave Observations Gopalswamy, N.; Shimojo,M.; Lu, W.; Yashiro, S.; Shibasaki, K.; Howard, R. A. ApJ, 586, 562-578, 2003. 概要.
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太陽雑誌会 2003/4/28 殿岡 英顕 Prominence Eruption and Coronal Mass Ejection: A Statistical Study Using Microwave ObservationsGopalswamy, N.; Shimojo,M.; Lu, W.; Yashiro, S.; Shibasaki, K.; Howard, R. A.ApJ, 586, 562-578, 2003
概要 • 下条氏のNoRH Prominence catalog と、八代氏の LASCO CME catalog を合わせて、統計的に解析したもの。
2.Data Selection • Automatic detection of limb events at NoRH 17GHz, from 1996 January 1 to 2001 December 31. • SOHO LASCO C2 and C3, corresponding to the prominence events. • 186 events total (excluding SOHO major datagap)
3.1 Prominence trajectoriesFig1: Typical prominence trajectories
Fig2. Time-height plot • T for Transverse, 34/186 • R for Radial, 152/186
Fig6. CME-Prominence relationship with association • An eruptive prominence of 2000 Oct 22.
Fig7. CME-Prominence relationship without association • An prominence erupton event of 2001 Aug 29 • No discernible change on LASCO observations.
Fig8. Height histograms • 134/186 PEs were associated with CMEs,34 no associated CMEs,11 streamer change. • CME+PE events:faster and larger heights
4.1 Source latitudeFig9. Latitude distribution • PE distributions: • 2 peaks • events from almost all latitudes • 3 from eqator • CME distributions: • One broad peak centered on the equator • almost all latitudes
Fig10: Solar cycle variation • CME and PE latitude vs Carrington rotation number • CME and PE occur at all latitudes during solar maxima and close to equator during solar minimum.
4.2 Timing relationshipFig11: The difference between two onset time • Onset times of PEs and CMEs are roughly the same within +/- 0.5hr.
4.3 Spatial relationshipFig12: Spatial relationship • The latitude offsets of PEs and CMEs. • More events with positive offsets • The latitude of CMEs is closer to the equator than that of corresponding prominence. • Positive offset before 2000.
4.4 Core associationFig13:An example of the prominence-CME association • 2001 Dec 19-20 • Radio+EIT195+LASCO
Fig14: Speed distribution of CME, core and PE • 98/134 (73%) had clear whitelight cores.
Fig15: Core speed vs PE speed • Core speed is always greater than PE speed • fast PEs associated with fast cores (?)
4.5 Streamer eventsFig16: An example of streamer event • 1998 June 1 PE • 1.24 Rsun (initial) to 1.28 Rsun (final) • streamer expanded • 11/52 = 21% were associated
5. Discussions • Munro et al. (1979):The prominences with large height have better association with CMEs. • Gilbert et al. (2000): CME associations are different (They are larger). • Hori & Culhane (2002): association with CMEs92% vs 76%. The difference of selection criteira. • Yang & Wang (2002): association rate 10 to 30%,65% for Gopalswamy's check.
6. Summary and conclusions • Radial (eruptive) and Transverse (active) events • Radial events showed close relationship to the CMEs (83%). • 73% of all the PEs were associated with CMEs. • Onsets of PEs and CMEs were nearly simultaneous, within 30min. • CPAs of CMEs and PEs generally did not coincide. CMEs – equator, PEs- AR belt for minimum, no such relationship for solar maximum.