Download - Observations of Magnetic Field Reconnection at the Base of EFR Surges 黒河宏企、 Liu Yu 、清原淳子(京大理 )
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Observations of Magnetic Field Reconnection at the Base of EFR Surges
Liu Yu)
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. Brief Review of Surge StudyRoy(1973)surge: Chromospheric explosion:
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(1) Satellite Polarity: Rust(1968): IAU symp. Vol.35, 77
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(2) Evoluving magnetic feature: Roy(1973): S.P.28, 951412UT1913UT2046UTH+1.4H-2H-0.9HH+1.4H-0.6H+0.6
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(3) Emerging Flux Region:EFR surge surgeKurokawa and Kawai(1993):IAU Colloq.Kurokawa(1988):2015UTBBSO2047UTBBSO83/6/16/20050UTHida0053UTHIdaContinuum0221UTHidaH+0.80605UTHida
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2240UTSurge is the first manifestation of the birth of an active regionKurokawa(2005)H centerH centerH centerMagneticfieldMagneticfield
MagneticfieldCaline wingintensityCaline wingintensity
Big Bear Solar Observatory
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EFR-surge (kurokawa and Kawai 1993)EFRelementary surgeHblue-wingHred-wingEFRSurge
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Hsurge: EFR(Kurokawa and Kawai 1993)
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Soft X-ray Jet (Yohkoh SXT)shibata et al. (1992) Shimojo et al. (1996) Yokoyama and Shibata(1996)EFR
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Surge
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Detailed comparison between Hida H and Huairou Magnetogram
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Flux changes of the isolated magnetic polarity near the footpoint of the H surge
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Correction of errors included in the raw data(1)(2)(3)Magnetic flux change: increase
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Summary of Flux Changes in the Surge RegionsSurgeEFR is essential for surge!
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High resolution observation ofthe footpoints of HsurgesBrooks, Kurokawa and Burger(2005)With Lockheed SOUP and Swedish 50cm telescope at La PalmaTRACE171 magnetic fieldH-0.7H+0.7. Solar B
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TRACE171contour on the H-0.7at 14:07 UTTRACE171contour on the magnetogram at 14:08UTH-0.7imagesTRACE171imagesHot coronal plasma observed in Fe171 at the base of an HsurgeEvidence of reconnection
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Before reconnectionAfter reconnectionEFRSchematic model of the surge of 30 May, 1998
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Changes of transverse field at the surge base Liu and Kurokawa(2004:Ap.J. 610, 1136)30Aug,2001Surge
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(1)Transient appearance of transverse magnetic field during the surge activity(2) Formation of transverse field after the surge activity? (Liu and Kurokawa 2004)surgeafter surgeFormation of two types of transverse magnetic field
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. Solar BHdark surge, Hbright point, XRT-hot reconnected loop, -evaporation jet transeverse
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Surge SMART(Solar Magnetic ActivityResearch Telescope) at Hida ObservatoryDSTSMART