Iron-Line Emission during Solar Flares

1971 ◽  
Vol 170 ◽  
pp. 573 ◽  
Author(s):  
G. A. Doschek ◽  
J. F. Meekins ◽  
R. W. Kreplin ◽  
T. A. Chubb ◽  
H. Friedman
Keyword(s):  
1970 ◽  
Vol 160 ◽  
pp. 309 ◽  
Author(s):  
J. L. Culhane ◽  
K. J. H. Phillips
Keyword(s):  

2006 ◽  
Vol 453 (1) ◽  
pp. L13-L16 ◽  
Author(s):  
L. Miller ◽  
T. J. Turner ◽  
J. N. Reeves ◽  
I. M. George ◽  
D. Porquet ◽  
...  
Keyword(s):  

2014 ◽  
Vol 10 (S305) ◽  
pp. 114-120
Author(s):  
Janusz Sylwester ◽  
Stefan Płocieniak ◽  
Jarosław Bakała ◽  
Żaneta Szaforz ◽  
Marek Stȩślicki ◽  
...  

AbstractWe present the innovative soft X-ray spectro-polarimeter, SolpeX. This instrument consists of three functionally independent blocks. They are to be included into the Russian instrument KORTES, to be mounted onboard the ISS. The three SolpeX units are: a simple pin-hole X-ray spectral imager, a polarimeter, and a fast-rotating drum multiple-flat-crystal Bragg spectrometer. Such a combination of measuring blocks will offer a new opportunity to reliably measure possible X-ray polarization and spectra of solar flares, in particular during the impulsive phase. Polarized Bremsstrahlung and line emission due to the presence of directed particle beams will be detected, and measurements of the velocities of evaporated hot plasma will be made. In this paper we discuss the details of the construction of the SolpeX units. The delivery of KORTES with SolpeX to the ISS is expected to happen in 2017/2018.


1978 ◽  
Vol 226 ◽  
pp. 282 ◽  
Author(s):  
H. L. Kestenbaum ◽  
W. H.-M. Ku ◽  
K. S. Long ◽  
E. H. Silver ◽  
R. Novick

1973 ◽  
Vol 184 ◽  
pp. L1 ◽  
Author(s):  
P. J. Serlemitsos ◽  
E. A. Boldt ◽  
S. S. Holt ◽  
R. Ramaty ◽  
A. F. Brisken
Keyword(s):  
X Ray ◽  

1982 ◽  
Vol 97 ◽  
pp. 97-106 ◽  
Author(s):  
C. Jones ◽  
W. Forman

The earliest Uhuru observations showed that cluster X-ray sources were not associated with single individual galaxies but were extended sources (Gursky et al. 1971, Kellogg et al. 1972, and Forman et al. 1972). The detection of iron line emission from X-ray spectroscopic observations (Mitchell et al. 1976 and Serlemitsos et al. 1977) showed both that the dominant X-ray emission process was thermal bremsstrahlung and that the gas had been processed through stellar systems before being injected into the intracluster medium.


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