Explosive Events: Swirling Transition Region Jets

被引:33
作者
Curdt, W. [1 ]
Tian, H. [2 ]
Kamio, S. [1 ]
机构
[1] Max Planck Inst Solar Syst Res, D-37191 Katlenburg Lindau, Germany
[2] High Altitude Observ NCAR, Boulder, CO 80307 USA
基金
美国国家科学基金会;
关键词
Flares; microflares and nanoflares; Helicity; observations; Jets; Transition region; Spectrum; ultraviolet; Chromosphere; active; EXTREME-ULTRAVIOLET; SOLAR; TELESCOPE; FEATURES;
D O I
10.1007/s11207-012-9940-9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we extend our earlier work to provide additional evidence for an alternative scenario to explain the nature of events called 'explosive events'. The bidirected, fast Doppler motion of explosive events observed spectroscopically in the transition region emission is classically interpreted as a pair of bidirectional jets moving upward and downward from a reconnection site. We discuss the problems of this model. In our previous work, we focused basically on the discrepancy of fast Doppler motion without detectable motion in the image plane. We now suggest an alternative scenario for the explosive events, based on our observations of spectral line tilts and bifurcated structure in some events. Both features are indicative of rotational motion in narrow structures. We explain the bifurcation as the result of rotation of hollow cylindrical structures and demonstrate that this kind of sheath model can also be applied to explain the nature of the puzzling 'explosive events'. We find that the spectral tilt, the lack of apparent motion, the bifurcation, and a rapidly growing number of direct observations support an alternative scenario of linear, spicular-sized jets with a strong spinning motion.
引用
收藏
页码:417 / 424
页数:8
相关论文
共 29 条
[1]   Spectroscopy at the solar limb I. Average off-limb profiles and Doppler shifts of Ca II H [J].
Beck, C. A. R. ;
Rezaei, R. .
ASTRONOMY & ASTROPHYSICS, 2011, 531
[2]  
Beckers J.M., 1964, 49 AIR FORC CAMBR RE
[3]   SOLAR SPICULES [J].
BECKERS, JM .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1972, 10 :73-&
[4]   Statistical comparison of transition region blinkers and explosive events [J].
Brkovic, A ;
Peter, H .
ASTRONOMY & ASTROPHYSICS, 2004, 422 (02) :709-716
[5]  
Budnik F, 1998, ASTRON ASTROPHYS, V334, pL77
[6]  
Cook J. W., 1984, Advances in Space Research, V4, P59, DOI 10.1016/0273-1177(84)90366-1
[7]   Spectroscopic evidence for helicity in explosive events [J].
Curdt, W. ;
Tian, H. .
ASTRONOMY & ASTROPHYSICS, 2011, 532
[8]   HIGH-RESOLUTION TELESCOPE AND SPECTROGRAPH OBSERVATIONS OF THE QUIET SOLAR CHROMOSPHERE AND TRANSITION ZONE [J].
DERE, KP ;
BARTOE, JDF ;
BRUECKNER, GE .
ASTROPHYSICAL JOURNAL, 1984, 281 (02) :870-883
[9]   EXPLOSIVE EVENTS IN THE SOLAR TRANSITION ZONE [J].
DERE, KP ;
BARTOE, JDF ;
BRUECKNER, GE .
SOLAR PHYSICS, 1989, 123 (01) :41-68
[10]   Simulations of small-scale explosive events on the Sun [J].
Innes, DE ;
Tóth, G .
SOLAR PHYSICS, 1999, 185 (01) :127-141