Multilayer mirror based soft x-ray spectrometer as a high temperature plasma diagnostic

2001 ◽  
Vol 72 (1) ◽  
pp. 1183-1187 ◽  
Author(s):  
S. Duorah ◽  
A. Ejiri ◽  
S. Lee ◽  
H. Iguchi ◽  
A. Fujisawa ◽  
...  
1985 ◽  
Vol 85 ◽  
pp. 365-368
Author(s):  
S. Ibadov

AbstractThe intensity of solar X-radiation scattered by a comet is calculated and compared to the proper X-radiation of the comet due to impacts of cometary and interplanetary dust particles. Detection of X-radiation of dusty comets at small heliocentric distances (R ≤ 1 a.u.) is found to be an indicator of high-temperature plasma generation as result of grain collisions.


1974 ◽  
Vol 18 ◽  
pp. 1-25
Author(s):  
D. J. Nagel

AbstractThe radiation from plasmas hotter than 106K falls in the x-ray region. Such plasmas are required for fusion power generation. They can also be used as x-ray sources. Measurements of x-ray emission from high temperature plasma yields (a) diagnostic information on the plasma conditions and (b) the characteristics of plasma x-ray sources which determine their applications. Hence, measurements of x-rays from plasmas are finding widespread use.


2001 ◽  
Vol 31 (12) ◽  
pp. 1071-1074 ◽  
Author(s):  
V V Gavrilov ◽  
A Yu Gol'tsov ◽  
N G Koval'skii ◽  
S N Koptyaev ◽  
A I Magunov ◽  
...  

1994 ◽  
Author(s):  
Yuriy Y. Platonov ◽  
Sergei V. Bobashev ◽  
Nikolai N. Salashchenko ◽  
Dmitrii M. Simanovski ◽  
L. A. Shmaenok ◽  
...  

1998 ◽  
Vol 188 ◽  
pp. 256-257
Author(s):  
M. Ozaki ◽  
K. Koyama

From many Galactic supernova remnants (SNRs), X-ray emissions consisting of non-equilibrium ionization (NEI) plasma and additional hard component are detected. The hard emission have been usually interpreted as a high temperature plasma of = 10 keV. However, the recent observation with ASCA made it clear that the hard components of some SNRs are of non-thermal origin. Here we report the ASCA results of SN 1006 and IC 443 observations as an example of such SNRs.


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