Dust as a versatile matter for high-temperature plasma diagnostic

2008 ◽  
Vol 79 (10) ◽  
pp. 10F333 ◽  
Author(s):  
Zhehui Wang ◽  
Catalin M. Ticos
2001 ◽  
Vol 72 (1) ◽  
pp. 1183-1187 ◽  
Author(s):  
S. Duorah ◽  
A. Ejiri ◽  
S. Lee ◽  
H. Iguchi ◽  
A. Fujisawa ◽  
...  

2016 ◽  
Vol 59 (3) ◽  
pp. 344-350 ◽  
Author(s):  
A. A. Ivanova ◽  
P. V. Zubarev ◽  
S. V. Ivanenko ◽  
A. N. Kvashnin ◽  
A. I. Kotelnikov ◽  
...  

1981 ◽  
Vol 9 (3) ◽  
pp. 237-252 ◽  
Author(s):  
Mitsuo MAEDA ◽  
Katsunori MURAOKA ◽  
Makoto HAMAMOTO ◽  
Masanori AKAZAKI ◽  
Yasushi MIYAZOE

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.


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