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RESISTIVE EMERGENCE OF UNDULATORY FLUX TUBES
E. Pariat, G. Aulanier, and B. Schmieder Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique ( LESIA), Observatoire de Meudon, and M. K. Georgoulis, D. M. Rust, and P. N. Bernasconi Applied Physics Laboratory, Johns Hopkins University The Astrophysical Journal, 614:1099–1112, 2004 October 20
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Flare Genesis Experiment
Balloon-borne Altitude 37km ( Middle Stratosphere ) Primary Mirror : 80cm, Ultra-low expansion Secondary Mirror : Single-crystal Silicon Graphite-epoxy telescope tube Achieved Image quality 0.5”
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Flare Genesis Experiment
FOV : 92” x 92” Liquid-crystal modulator, a 0.16Åtunable etalon, 1.25 order-isolation filters Vector Megnetogram CaI 6122, +/- 0.08Å Dopplergram CaI 6122 Hα-0.8Å Filtergram
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Georgoulis et al. (2002)
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Georgoulis et al. (2002) Area Magnetic Proper Motions Downflows A ˚ Neutral (km s1) (%)(kms1) BPs (%) Lines(%) (<0.2, 0.4) (SG boundary) 86 (-0.4, -0.1) (0.4, >0.8) (cell interior/MDFs) (<0.2, 0.4) (-0.3, -0.1) (<0.2, 0.8) (-0.5)
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Georgoulis et al. (2002)
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Pariat et al. (2004) FGE data What is the magnetic topology of EBs?
Can EBs be sympathetically linked to one another, and why? What is their relation with the flux emergence on the larger scale of the active region?
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Pariat et al. (2004)
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FROM PHOTOSPHERIC VECTOR MAGNETIC FIELDS TO CORONAL FIELDS
Constant α Force Free Field Extrapolation to Corona Boundary Condition ( Bz(x,y,0)) FGE Vector magnetogram Wider field IVM(Mickey) α Free Parameter
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FROM PHOTOSPHERIC VECTOR MAGNETIC FIELDS TO CORONAL FIELDS
Estimation of α B(horizontal) Extrapolated vs Observed Morphology of TRACE Loops αf = 2.2x10-2
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FROM PHOTOSPHERIC VECTOR MAGNETIC FIELDS TO CORONAL FIELDS
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FROM PHOTOSPHERIC VECTOR MAGNETIC FIELDS TO CORONAL FIELDS
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ELLERMAN BOMBS AND MAGNETIC TOPOLOGY
Bald Patch (BP) Bz=0 and B・∇Bz>0 Spatial Correlation ・EB vs BP ・EB vs Separatorix Foot Point
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EB vs BP
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EB vs BP
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EB vs Separatorix Footpoint
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ELLERMAN BOMBS AND MAGNETIC TOPOLOGY
41/47 of the EBs are related to BPs or footpoints of sepatatorix (preferential sites of magnetic reconnection in the low chromosphere).
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SERPENTINE FIELD LINES
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SERPENTINE FIELD LINES
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SERPENTINE FIELD LINES
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THE NATURE OF FLUX EMERGENCE
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THE NATURE OF FLUX EMERGENCE
Possible origin of undulation ・ Convection G Mm MG 5Mm SG 30Mm ・ Parker Instability λ >2Mm
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EFR,EBについて 多数のBPのうち、EBとして見える条件? EBが点状であるのはなぜか? 安定した黒点周辺のミニEBも同じ機構か?
これらの問題については、更なる観測が必要。 光球速度場 horizontal, vertical large scale, local time-scale 光球磁場 EB近傍の高分解能ベクトルB
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