scholarly journals Diagnostics of warm dense matter by high-resolution X-ray spectroscopy of hollow ions

2014 ◽  
Vol 33 (1) ◽  
pp. 27-39 ◽  
Author(s):  
A. Ya. Faenov ◽  
I. Yu. Skobelev ◽  
T. A. Pikuz ◽  
S. A. Pikuz ◽  
R. Kodama ◽  
...  

AbstractThe short review on the possible applications of the hollow ion spectra for the diagnostics of the high-temperature plasma created by intensive laser and particle beams is presented. Because of the hollow ion spectra features are defined mainly by the mechanisms of their excitation, we consider the various types of the high-temperature plasma where different excitation processes are important. It is shown that like ordinary spectral lines, spectra of the hollow ions offer considerable diagnostic opportunities. At the present time, hollow ion spectra are used mainly to investigate plasma heated by X-ray radiation, but the hollow ions must be generated when plasma is heated by fast heavy ion beams too. In this case, the resultant substance state will be also characterized by solid-state density, and some spatial regions of targets will have relatively low temperatures, i.e., will be a nonideal plasma. It is emphasized that hollow ion spectra are promising diagnostic tool for both nonideal plasma and warm dense matter.

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.


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

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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