EXTREME-ULTRAVIOLET OBSERVATIONS OF GLOBAL CORONAL WAVE ROTATION

被引:3
|
作者
Attrill, G. D. R. [1 ]
Long, D. M. [2 ]
Green, L. M. [2 ]
Harra, L. K. [2 ]
van Driel-Gesztelyi, L. [2 ,3 ,4 ]
机构
[1] Dstl Porton Down, Def Sci & Technol Lab, Salisbury SP4 0JQ, Wilts, England
[2] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[3] Observ Paris, CNRS, LESIA, F-92195 Meudon, France
[4] Hungarian Acad Sci, Konkoly Observ, Budapest, Hungary
来源
ASTROPHYSICAL JOURNAL | 2014年 / 796卷 / 01期
关键词
Sun: corona; Sun: coronal mass ejections (CMEs); Sun: magnetic fields; PHOTOSPHERIC FLUX CANCELLATION; 1997 MAGNETIC CLOUD; MASS EJECTION; EIT WAVES; INTERCHANGE RECONNECTION; PROPAGATING DISTURBANCE; SOLAR ERUPTIONS; SOHO MISSION; CME EVENT; STEREO;
D O I
10.1088/0004-637X/796/1/55
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present evidence of global coronal wave rotation in EUV data from SOHO/EIT, STEREO/EUVI, and SDO/AIA. The sense of rotation is found to be consistent with the helicity of the source region (clockwise for positive helicity, anticlockwise for negative helicity), with the source regions hosting sigmoidal structures. We also study two coronal wave events observed by SDO/AIA where no clear rotation (or sigmoid) is observed. The selected events show supporting evidence that they all originate with flux rope eruptions. We make comparisons across this set of observations (both with and without clear sigmoidal structures). On examining the magnetic configuration of the source regions, we find that the nonrotation events possess a quadrupolar magnetic configuration. The coronal waves that do show a rotation originate from bipolar source regions.
引用
收藏
页数:13
相关论文
共 50 条
  • [41] NEW SOLAR EXTREME-ULTRAVIOLET IRRADIANCE OBSERVATIONS DURING FLARES
    Woods, Thomas N.
    Hock, Rachel
    Eparvier, Frank
    Jones, Andrew R.
    Chamberlin, Phillip C.
    Klimchuk, James A.
    Didkovsky, Leonid
    Judge, Darrell
    Mariska, John
    Warren, Harry
    Schrijver, Carolus J.
    Webb, David F.
    Bailey, Scott
    Tobiska, W. Kent
    ASTROPHYSICAL JOURNAL, 2011, 739 (02):
  • [42] STUDYING EXTREME ULTRAVIOLET WAVE TRANSIENTS WITH A DIGITAL LABORATORY: DIRECT COMPARISON OF EXTREME ULTRAVIOLET WAVE OBSERVATIONS TO GLOBAL MAGNETOHYDRODYNAMIC SIMULATIONS
    Downs, Cooper
    Roussev, Ilia I.
    van der Holst, Bart
    Lugaz, Noe
    Sokolov, Igor V.
    Gombosi, Tamas I.
    ASTROPHYSICAL JOURNAL, 2011, 728 (01):
  • [43] OBSERVATIONS OF PKS 2155-304 WITH THE EXTREME-ULTRAVIOLET EXPLORER
    MARSHALL, HL
    CARONE, TE
    FRUSCIONE, A
    ASTROPHYSICAL JOURNAL, 1993, 414 (02): : L53 - L56
  • [44] Reconciling extreme-ultraviolet and radio observations of the Sun's corona
    Zhang, J
    Kundu, MR
    White, SM
    Dere, KP
    Newmark, JS
    ASTROPHYSICAL JOURNAL, 2001, 561 (01): : 396 - 405
  • [45] THE POTENTIAL FOR PLASMA DIAGNOSTICS FROM STELLAR EXTREME-ULTRAVIOLET OBSERVATIONS
    FELDMAN, U
    MANDELBAUM, P
    SEELY, JF
    DOSCHEK, GA
    GURSKY, H
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1992, 81 (01): : 387 - &
  • [46] FIRST SPECTRAL OBSERVATIONS OF THE DIFFUSE BACKGROUND WITH THE EXTREME-ULTRAVIOLET EXPLORER
    JELINSKY, P
    VALLERGA, JV
    EDELSTEIN, J
    ASTROPHYSICAL JOURNAL, 1995, 442 (02): : 653 - 661
  • [47] TIME VARIATIONS IN EXTREME-ULTRAVIOLET EMISSION-LINES AND PROBLEM OF CORONAL HEATING
    VERNAZZA, JE
    FOUKAL, PV
    HUBER, MCE
    NOYES, RW
    REEVES, EM
    SCHMAHL, EJ
    TIMOTHY, JG
    WITHBROE, GL
    ASTROPHYSICAL JOURNAL, 1975, 199 (02): : L123 - &
  • [48] THE FIRST STRAY LIGHT CORRECTED EXTREME-ULTRAVIOLET IMAGES OF SOLAR CORONAL HOLES
    Shearer, Paul
    Frazin, Richard A.
    Hero, Alfred O., III
    Gilbert, Anna C.
    ASTROPHYSICAL JOURNAL LETTERS, 2012, 749 (01)
  • [50] The inability of steady-flow models to explain the extreme-ultraviolet coronal loops
    Patsourakos, S
    Klimchuk, JA
    MacNeice, PJ
    ASTROPHYSICAL JOURNAL, 2004, 603 (01): : 322 - 329