High-resolution X-ray spectra of solar flares. VII - A long-duration X-ray flare associated with a coronal mass ejection

1985 ◽  
Vol 292 ◽  
pp. 309 ◽  
Author(s):  
R. W. Kreplin ◽  
G. A. Doschek ◽  
U. Feldman ◽  
N. R., Jr. Sheeley ◽  
J. F. Seely
Keyword(s):  
High Resolution ◽  
Coronal Mass Ejection ◽  
Solar Flares ◽  
X Ray ◽  
Long Duration ◽  
Mass Ejection

High-resolution X-ray spectra of solar flares. IX - Mass upflow in the long-duration flare of 1979 June 5

1989 ◽  
Vol 345 ◽  
pp. 1079 ◽  
Author(s):  
G. A. Doschek ◽  
U. Feldman ◽  
J. F. Seely ◽  
D. L. McKenzie
Keyword(s):  
High Resolution ◽  
Solar Flares ◽  
X Ray ◽  
Long Duration

scholarly journals Hydrodynamic Models of Solar and Stellar Flares

1989 ◽  
Vol 104 (1) ◽  
pp. 289-298
Author(s):  
Giovanni Peres
Keyword(s):  
High Resolution ◽  
Light Curve ◽  
Solar Flares ◽  
Impulsive Phase ◽  
Light Curves ◽  
Physical Parameters ◽  
The Sun ◽  
Hydrodynamic Models ◽  
X Ray ◽  
Stellar Flares

AbstractThis paper discusses the hydrodynamic modeling of flaring plasma confined in magnetic loops and its objectives within the broader scope of flare physics. In particular, the Palermo-Harvard model is discussed along with its applications to the detailed fitting of X-ray light curves of solar flares and to the simulation of high-resolution Caxix spectra in the impulsive phase. These two approaches provide complementary constraints on the relevant features of solar flares. The extension to the stellar case, with the fitting of the light curve of an X-ray flare which occurred on Proxima Centauri, demonstrates the feasibility of using this kind of model for stars too. Although the stellar observations do not provide the wealth of details available for the Sun, and, therefore, constrain the model more loosely, there are strong motivations to pursue this line of research: the wider range of physical parameters in stellar flares and the possibility of studying further the solar-stellar connection.

Radio and X‐Ray Studies of a Coronal Mass Ejection Associated with a Very Slow Prominence Eruption

1997 ◽  
Vol 475 (1) ◽  
pp. 348-360 ◽  
Author(s):  
N. Gopalswamy ◽  
Y. Hanaoka ◽  
M. R. Kundu ◽  
S. Enome ◽  
J. R. Lemen ◽  
...  
Keyword(s):  
Coronal Mass Ejection ◽  
X Ray ◽  
Mass Ejection

scholarly journals On the Association between Coronal Mass Ejections and Coronal Holes

1989 ◽  
Vol 104 (2) ◽  
pp. 239-242
Author(s):  
V.K. Verma ◽  
M.C. Pande
Keyword(s):  
Magnetic Field ◽  
Coronal Mass Ejection ◽  
Coronal Mass Ejections ◽  
Solar Flares ◽  
Coronal Holes ◽  
Mass Ejection ◽  
Open Magnetic Field

AbstractThe coronal mass ejection (CME) data and the data for coronal holes for the period 1979-1982 are compared locationwise. Out of 79 CMEs whose locations and spans are known, 48 (61%) CMEs are associated with coronal holes. We make a tentative suggestion that probably the mass ejected during solar flares and active prominences may move along the open magnetic field of the coronal holes and appear as CMEs.

scholarly journals A slow coronal mass ejection with rising X-ray source

2005 ◽  
Vol 434 (2) ◽  
pp. 761-771 ◽  
Author(s):  
C. P. Goff ◽  
L. van Driel-Gesztelyi ◽  
L. K. Harra ◽  
S. A. Matthews ◽  
C. H. Mandrini
Keyword(s):  
Coronal Mass Ejection ◽  
X Ray ◽  
Mass Ejection

Distribution of Solar Flares with Respect to Associated Coronal Mass Ejection (CME) Span During 1996 to 2012

Astrophysics ◽  
2015 ◽  
Vol 58 (3) ◽  
pp. 420-429 ◽  
Author(s):  
B. Bhatt ◽  
L. Prasad ◽  
Hema Mathpal ◽  
R. Mathpal
Keyword(s):  
Coronal Mass Ejection ◽  
Solar Flares ◽  
Mass Ejection

Large Doppler Shifts in X-Ray Plasma: An Explosive Start to Coronal Mass Ejection

2001 ◽  
Vol 549 (2) ◽  
pp. L249-L252 ◽  
Author(s):  
D. E. Innes ◽  
W. Curdt ◽  
R. Schwenn ◽  
S. Solanki ◽  
G. Stenborg ◽  
...  
Keyword(s):  
Coronal Mass Ejection ◽  
X Ray ◽  
Doppler Shifts ◽  
Mass Ejection

A CORONAL MASS EJECTION AND HARD X-RAY EMISSIONS ASSOCIATED WITH THE KINK INSTABILITY

2009 ◽  
Vol 703 (1) ◽  
pp. 1-7 ◽  
Author(s):  
Kyung-Suk Cho ◽  
Jeongwoo Lee ◽  
Su-Chan Bong ◽  
Yeon-Han Kim ◽  
Bhuwan Joshi ◽  
...  
Keyword(s):  
Coronal Mass Ejection ◽  
X Ray ◽  
Kink Instability ◽  
Mass Ejection

Comparing different types of solar flares with radio bursts detected by SMOS

2020 ◽  
Author(s):  
Manuel Flores Soriano ◽  
Consuelo Cid
Keyword(s):  
Space Weather ◽  
Early Warning ◽  
Solar Flares ◽  
Solar Radio ◽  
The Sun ◽  
Radio Bursts ◽  
Radio Observatory ◽  
X Ray ◽  
Different Types ◽  
Mass Ejection

<p>SMOS is an Earth observing satellite that is been adapted to provide full polarization observations of the Sun at 1.4 GHz 24 hours a day. Its solar radio observations from the last decade will be released to the community by the middle of this year. In this presentation we show the capabilities of SMOS as a solar radio observatory and compare some of the most relevant radio bursts with data from GOES, LASCO, SDO and RSTN. We show how SMOS responds to different kinds of solar flares depending on their x-ray flux, and the kind of mass ejection or solar dimming that they have produced, if any. In addition to this we also show the potential of SMOS as a space weather tool to monitor GNSS satellites signal fades and to provide an early warning of Earth-directed coronal mass ejections.</p>

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