QUASI-PERIODIC FLUCTUATIONS AND CHROMOSPHERIC EVAPORATION IN A SOLAR FLARE RIBBON OBSERVED BYHINODE/EIS,IRIS, ANDRHESSI

2016 ◽  
Vol 830 (2) ◽  
pp. 101 ◽  
Author(s):  
Jeffrey W. Brosius ◽  
Adrian N. Daw ◽  
Andrew R. Inglis
Keyword(s):  
Solar Flare ◽  
Chromospheric Evaporation ◽  
Periodic Fluctuations ◽  
Flare Ribbon

scholarly journals IMAGING AND SPECTROSCOPIC OBSERVATIONS OF MAGNETIC RECONNECTION AND CHROMOSPHERIC EVAPORATION IN A SOLAR FLARE

2014 ◽  
Vol 797 (2) ◽  
pp. L14 ◽  
Author(s):  
Hui Tian ◽  
Gang Li ◽  
Katharine K. Reeves ◽  
John C. Raymond ◽  
Fan Guo ◽  
...  
Keyword(s):  
Solar Flare ◽  
Magnetic Reconnection ◽  
Spectroscopic Observations ◽  
Chromospheric Evaporation

scholarly journals Enhanced Turbulence and Heating Observed Preceding the Impulsive Phase in a Solar Flare

1989 ◽  
Vol 104 (2) ◽  
pp. 231-234
Author(s):  
Chung-Chieh Cheng ◽  
K.G. Widing
Keyword(s):  
Solar Flare ◽  
Transition Region ◽  
Normal Incidence ◽  
Impulsive Phase ◽  
Energetic Particles ◽  
Line Profiles ◽  
Chromospheric Evaporation

AbstractWe studied the unique EUV spectra of the 21 Jan. 1974 flare observed by the NRL Normal-Incidence Slit Spectrometer (SO 82B) onboard the Skylab. The results show that the pre-impulsive transition region plasmas exhibited enhanced turbulence and heating before the acceleration of energetic particles. The absence of blue-shifted components in the Fe XXI line profiles shows that the chromospheric evaporation is not important in this flare.

Conduction-driven chromospheric evaporation in a solar flare

1988 ◽  
Vol 329 ◽  
pp. 456 ◽  
Author(s):  
Dominic M. Zarro ◽  
James R. Lemen
Keyword(s):  
Solar Flare ◽  
Chromospheric Evaporation

scholarly journals New Evidence of Chromospheric Evaporation

1998 ◽  
Vol 167 ◽  
pp. 397-400 ◽  
Author(s):  
J. Kašparová ◽  
P. Kotrč ◽  
P. Heinzel ◽  
I.F. Nikulin ◽  
P. Rudawy
Keyword(s):  
Astronomical Institute ◽  
Gradual Phase ◽  
Chromospheric Evaporation ◽  
Sternberg Astronomical Institute ◽  
Blue Wing ◽  
Flare Ribbon ◽  
New Evidence ◽  
Flare Model

AbstractHα spectra obtained at Sternberg Astronomical Institute in Moscow during the gradual phase of the flare on May 16, 1981 are analysed. The flare-ribbon profiles show a red asymmetry of the emission peaks, and we interpret this as an absorption in the blue wing of the profile due to expected upflows. We demonstrate a good correlation between the observed Hα profiles and those computed with the flare model Fl and upflows reaching 10 km s−1.

scholarly journals MULTIWAVELENGTH IMAGING AND SPECTROSCOPY OF CHROMOSPHERIC EVAPORATION IN AN M-CLASS SOLAR FLARE

2010 ◽  
Vol 719 (1) ◽  
pp. 655-670 ◽  
Author(s):  
A. M. Veronig ◽  
J. Rybák ◽  
P. Gömöry ◽  
S. Berkebile-Stoiser ◽  
M. Temmer ◽  
...  
Keyword(s):  
Solar Flare ◽  
Chromospheric Evaporation ◽  
Imaging And Spectroscopy ◽  
Multiwavelength Imaging

scholarly journals Imaging the Chromospheric Evaporation of the 1994 June 30 Solar Flare

1997 ◽  
Vol 481 (2) ◽  
pp. 978-987 ◽  
Author(s):  
Adriana V. R. Silva ◽  
Haimin Wang ◽  
Dale E. Gary ◽  
Nariaki Nitta ◽  
Harold Zirin
Keyword(s):  
Solar Flare ◽  
Chromospheric Evaporation
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