SLOW RISE AND PARTIAL ERUPTION OF A DOUBLE-DECKER FILAMENT. I. OBSERVATIONS AND INTERPRETATION

被引:130
作者
Liu, Rui [1 ,2 ]
Kliem, Bernhard [3 ,4 ]
Toeroek, Tibor [5 ]
Liu, Chang [2 ]
Titov, Viacheslav S. [5 ]
Lionello, Roberto [5 ]
Linker, Jon A. [5 ]
Wang, Haimin [2 ,6 ]
机构
[1] Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei 230026, Peoples R China
[2] New Jersey Inst Technol, Ctr Solar Terr Res, Space Weather Res Lab, Newark, NJ 07102 USA
[3] Univ Potsdam, Inst Phys & Astron, D-14476 Potsdam, Germany
[4] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[5] Predictive Sci Inc, San Diego, CA 92121 USA
[6] Natl Astron Observ, Key Lab Solar Act, Beijing, Peoples R China
基金
美国国家科学基金会;
关键词
Sun: coronal mass ejections (CMEs); Sun:; filaments; prominences; Sun: flares; CONFIGURATIONS SUPPORTING PROMINENCES; HELICAL MAGNETIC-FIELDS; HYPERBOLIC FLUX TUBES; X-RAY-EMISSION; KINK INSTABILITY; ACTIVE-REGION; SOLAR CORONA; NUMERICAL SIMULATIONS; SIGMOIDAL STRUCTURE; MASS EJECTION;
D O I
10.1088/0004-637X/756/1/59
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study an active-region dextral filament that was composed of two branches separated in height by about 13 Mm, as inferred from three-dimensional reconstruction by combining SDO and STEREO-B observations. This "double-decker" configuration sustained for days before the upper branch erupted with a GOES-class M1.0 flare on 2010 August 7. Analyzing this evolution, we obtain the following main results. (1) During the hours before the eruption, filament threads within the lower branch were observed to intermittently brighten up, lift upward, and then merge with the upper branch. The merging process contributed magnetic flux and current to the upper branch, resulting in its quasi-static ascent. (2) This transfer might serve as the key mechanism for the upper branch to lose equilibrium by reaching the limiting flux that can be stably held down by the overlying field or by reaching the threshold of the torus instability. (3) The erupting branch first straightened from a reverse S shape that followed the polarity inversion line and then writhed into a forward S shape. This shows a transfer of left-handed helicity in a sequence of writhe-twist-writhe. The fact that the initial writhe is converted into the twist of the flux rope excludes the helical kink instability as the trigger process of the eruption, but supports the occurrence of the instability in the main phase, which is indeed indicated by the very strong writhing motion. (4) A hard X-ray sigmoid, likely of coronal origin, formed in the gap between the two original filament branches in the impulsive phase of the associated flare. This supports a model of transient sigmoids forming in the vertical flare current sheet. (5) Left-handed magnetic helicity is inferred for both branches of the dextral filament. (6) Two types of force-free magnetic configurations are compatible with the data, a double flux rope equilibrium and a single flux rope situated above a loop arcade.
引用
收藏
页数:14
相关论文
共 104 条
[1]   Hard X-ray production in a failed filament eruption [J].
Alexander, David ;
Liu, Rui ;
Gilbert, Holly R. .
ASTROPHYSICAL JOURNAL, 2006, 653 (01) :719-724
[2]   THE MAGNETIC-FIELD OF SOLAR PROMINENCES [J].
ANTIOCHOS, SK ;
DAHLBURG, RB ;
KLIMCHUK, JA .
ASTROPHYSICAL JOURNAL, 1994, 420 (01) :L41-L44
[3]   A model for solar coronal mass ejections [J].
Antiochos, SK ;
DeVore, CR ;
Klimchuk, JA .
ASTROPHYSICAL JOURNAL, 1999, 510 (01) :485-493
[4]  
Anzer U, 1989, ASTROPHYSICS SPACE S, V150, P143
[5]   ON THE STRUCTURE AND EVOLUTION OF COMPLEXITY IN SIGMOIDS: A FLUX EMERGENCE MODEL [J].
Archontis, V. ;
Hood, A. W. ;
Savcheva, A. ;
Golub, L. ;
Deluca, E. .
ASTROPHYSICAL JOURNAL, 2009, 691 (02) :1276-1291
[6]   SOLAR CORONA LOOP STUDIES WITH THE ATMOSPHERIC IMAGING ASSEMBLY. I. CROSS-SECTIONAL TEMPERATURE STRUCTURE [J].
Aschwanden, Markus J. ;
Boerner, Paul .
ASTROPHYSICAL JOURNAL, 2011, 732 (02)
[7]  
Aulanier G, 1998, ASTRON ASTROPHYS, V335, P309
[8]   Current sheet formation in quasi-separatrix layers and hyperbolic flux tubes [J].
Aulanier, G ;
Pariat, E ;
Démoulin, P .
ASTRONOMY & ASTROPHYSICS, 2005, 444 (03) :961-976
[9]   FORMATION OF TORUS-UNSTABLE FLUX ROPES AND ELECTRIC CURRENTS IN ERUPTING SIGMOIDS [J].
Aulanier, G. ;
Toeroek, T. ;
Demoulin, P. ;
DeLuca, E. E. .
ASTROPHYSICAL JOURNAL, 2010, 708 (01) :314-333
[10]  
Aulanier G, 1998, ASTRON ASTROPHYS, V329, P1125