Oscillations of a loop prominence preceding a limb flare

Solar Physics ◽  
1981 ◽  
Vol 70 (1) ◽  
pp. 115-128 ◽  
Author(s):  
J. McKim Malville ◽  
Mark Schindler
Keyword(s):  
Limb Flare ◽  
Loop Prominence

X-ray imaging of a solar limb flare on 1982 January 22

Solar Physics ◽  
1986 ◽  
Vol 107 (1) ◽  
pp. 109-121 ◽  
Author(s):  
T. Takakura ◽  
K. Tanaka ◽  
N. Nitta ◽  
K. Kai ◽  
K. Ohki
Keyword(s):  
Solar Limb ◽  
X Ray ◽  
X Ray Imaging ◽  
Limb Flare

Velocity of the shock generated by a large east limb flare on August 18, 1979

1982 ◽  
Vol 9 (8) ◽  
pp. 897-900 ◽  
Author(s):  
H. V. Cane ◽  
R. G. Stone ◽  
R. Woo
Keyword(s):  
Limb Flare ◽  
East Limb

Motions in a loop prominence

Solar Physics ◽  
1980 ◽  
Vol 66 (1) ◽  
pp. 89-104 ◽  
Author(s):  
M. M. Makhmudov ◽  
G. M. Nikolsky ◽  
Yu. D. Zhugzhda
Keyword(s):  
Loop Prominence

2002 AUGUST 24 LIMB FLARE LOOP: DYNAMICS OF MICROWAVE BRIGHTNESS DISTRIBUTION

2009 ◽  
Vol 697 (1) ◽  
pp. 735-746 ◽  
Author(s):  
V. E. Reznikova ◽  
V. F. Melnikov ◽  
K. Shibasaki ◽  
S. P. Gorbikov ◽  
N. P. Pyatakov ◽  
...  
Keyword(s):  
Brightness Distribution ◽  
Flare Loop ◽  
Loop Dynamics ◽  
Limb Flare

scholarly journals Spectroscopic Signatures of a Flare Observed by SUMER Onboard SOHO

2001 ◽  
Vol 203 ◽  
pp. 264-266
Author(s):  
I. E. Dammasch ◽  
W. Curdt ◽  
B. Kliem ◽  
B. N. Dwivedi ◽  
K. Wilhelm
Keyword(s):  
Time Series ◽  
Spatial Relationship ◽  
Solar Limb ◽  
Dynamical Behaviour ◽  
X Rays ◽  
Flare Loops ◽  
Limb Flare ◽  
Raster Scans ◽  
Lower Height ◽  
Spectroscopic Signatures

We report on EUV observations of a solar limb flare obtained by the SUMER spectrometer. A time series was taken with fixed slit position and several spectral windows that covered a wide temperature range (104-107 K), preceded and followed by contextual raster scans in a He I line. During the time series, a C4.6 flare occurred in the region, also imaged in the EUV by SOHO/EIT and in soft X rays by YOHKOH/SXT. The temporal evolution seen in the SUMER spectra reveals a close spatial relationship and a correlated dynamical behaviour of the hot (T ≈ 107 K) and cool (T ≈ 104 K) material, which are difficult to reconcile with the notion (based on the Kopp-Pneuman flare model) that cool loops form at a lower height than the hot flare loops.

Multi-Wavelength Observation Results of the C5.6 Limb Flare of 1 August 2003

Solar Physics ◽  
2004 ◽  
Vol 225 (1) ◽  
pp. 75-90 ◽  
Author(s):  
Hui Li ◽  
Jianqi You ◽  
Qiusheng Du ◽  
Xingfeng Yu
Keyword(s):  
Limb Flare ◽  
Multi Wavelength ◽  
Observation Results
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