Simultaneous observations of solar transition region blinkers and explosive events by SUMER, CDS and BBSO - Are blinkers, explosive events and spicules the same phenomenon?

被引:40
作者
Madjarska, MS [1 ]
Doyle, JG [1 ]
机构
[1] Armagh Observ, Armagh BT61 9DG, North Ireland
关键词
Sun : corona; Sun : transition region; Sun : activity : Sun : UV radiation;
D O I
10.1051/0004-6361:20030397
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The SoHO discovery of the new "blinker" phenomena focused our study on the search of its relation to already known phenomena such as explosive events and spicules. The study was performed using a specially planned joint observing program involving the Coronal Diagnostic Spectrometer (CDS), Solar Ultraviolet Measurements of Emitted Radiation spectrograph (SUMER) and Big Bear Solar Observatory (BBSO) magnetograph. Within each blinker, the SUMER data reveal the presence of small-scale (3"-5"), short-lived (2 -3 min) bright features not seen in the CDS data which has sometimes being interpreted as oscillations in SUMER data. With this data we have clearly identified UV explosive events in CDS data. The explosive events show a size close to the small-scale brightenings forming the blinker core. However, they appear in the SUMER data with their typical strong blue and red wings while the blinker shows at best only a small increase in the emission of the blue and red wings and in most instances the typical transition region red-shift in the center of the line. In all cases the explosive events cover one pixel in CDS corresponding to a size of 4" x 4"-6". All identified explosive events were located at the border of the bright network i.e. the blinker, in the network or even in the internetwork. From this data, we believe that blinkers and explosive events are two separate phenomena not directly related or triggering each other. In this study, the Doppler shift was derived in a blinker phenomenon for the first time. It ranges from - 5 to 25 km s(-1) and is predominantly red-shifted. The observed magnetic flux increase during the blinker phenomena seems to play a crucial role in the development of this event. We suggest that "blinkers" maybe the on-disk signature of spicules.
引用
收藏
页码:731 / 741
页数:11
相关论文
共 34 条
[1]   The nature of network oscillations [J].
Banerjee, D ;
O'Shea, E ;
Doyle, JG ;
Goossens, M .
ASTRONOMY & ASTROPHYSICS, 2001, 371 (03) :1137-1149
[2]   Transition region blinkers - I. Quiet-Sun properties [J].
Bewsher, D ;
Parnell, CE ;
Harrison, RA .
SOLAR PHYSICS, 2002, 206 (01) :21-43
[3]   Analysis of blinkers and EUV brightenings in the quiet Sun observed with CDS [J].
Brkovic, A ;
Solanki, SK ;
Rüedi, I .
ASTRONOMY & ASTROPHYSICS, 2001, 373 (03) :1056-1072
[4]  
Brooks DH, 1999, ASTRON ASTROPHYS, V347, P277
[5]   OBSERVATIONS OF HIGH-ENERGY JETS IN THE CORONA ABOVE THE QUIET SUN, THE HEATING OF THE CORONA, AND THE ACCELERATION OF THE SOLAR-WIND [J].
BRUECKNER, GE ;
BARTOE, JDF .
ASTROPHYSICAL JOURNAL, 1983, 272 (01) :329-348
[6]  
CHAE J, 2000, APJ, V528, P119
[7]   Photospheric magnetic field changes associated with transition region explosive events [J].
Chae, JC ;
Wang, HM ;
Lee, CY ;
Goode, PR ;
Schuhle, U .
ASTROPHYSICAL JOURNAL, 1998, 497 (02) :L109-+
[8]   The SUMER spectral atlas of solar-disk features [J].
Curdt, W ;
Brekke, P ;
Feldman, U ;
Wilhelm, K ;
Dwivedi, BN ;
Schühle, U ;
Lemaire, P .
ASTRONOMY & ASTROPHYSICS, 2001, 375 (02) :591-613
[9]   EXPLOSIVE EVENTS AND MAGNETIC RECONNECTION IN THE SOLAR ATMOSPHERE [J].
DERE, KP ;
BARTOE, JDF ;
BRUECKNER, GE ;
EWING, J ;
LUND, P .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1991, 96 (A6) :9399-9407
[10]   EXPLOSIVE EVENTS IN THE SOLAR TRANSITION ZONE [J].
DERE, KP ;
BARTOE, JDF ;
BRUECKNER, GE .
SOLAR PHYSICS, 1989, 123 (01) :41-68