Influence of the expansion velocity of laser plasma bunches on the intensity of a plasma jet and quasistationary waves generated in a magnetic tube

2020 ◽  
Author(s):  
V. N. Tishchenko ◽  
A. G. Berezutsky ◽  
L. R. Dmitrieva ◽  
I. B. Miroshnichenko ◽  
I. F. Shaikhislamov
1994 ◽  
Vol 24 (12) ◽  
pp. 1100-1101 ◽  
Author(s):  
V M Dyakin ◽  
T A Pikuz ◽  
I Yu Skobelev ◽  
A Ya Faenov ◽  
J Wolowski ◽  
...  

1985 ◽  
Vol 15 (2) ◽  
pp. 255-256 ◽  
Author(s):  
Yurii V Afanas'ev ◽  
R A Ibraev ◽  
Andrey P Kanavin ◽  
B N Chetverushkin

1999 ◽  
Vol 6 (7) ◽  
pp. 2855-2861 ◽  
Author(s):  
Y. Sentoku ◽  
H. Ruhl ◽  
K. Mima ◽  
R. Kodama ◽  
K. A. Tanaka ◽  
...  

2017 ◽  
Vol 119 (25) ◽  
Author(s):  
D. P. Higginson ◽  
B. Khiar ◽  
G. Revet ◽  
J. Béard ◽  
M. Blecher ◽  
...  
Keyword(s):  

PLoS ONE ◽  
2012 ◽  
Vol 7 (11) ◽  
pp. e50823 ◽  
Author(s):  
Viren Menezes ◽  
Yohan Mathew ◽  
Kazuyoshi Takayama ◽  
Akira Kanno ◽  
Hamid Hosseini

1984 ◽  
Vol 14 (2) ◽  
pp. 292-294
Author(s):  
Yurii V Afanas'ev ◽  
Andrey P Kanavin
Keyword(s):  

1974 ◽  
Vol 22 ◽  
pp. 307 ◽  
Author(s):  
Zdenek Sekanina

AbstractIt is suggested that the outbursts of Periodic Comet Schwassmann-Wachmann 1 are triggered by impacts of interplanetary boulders on the surface of the comet’s nucleus. The existence of a cloud of such boulders in interplanetary space was predicted by Harwit (1967). We have used the hypothesis to calculate the characteristics of the outbursts – such as their mean rate, optically important dimensions of ejected debris, expansion velocity of the ejecta, maximum diameter of the expanding cloud before it fades out, and the magnitude of the accompanying orbital impulse – and found them reasonably consistent with observations, if the solid constituent of the comet is assumed in the form of a porous matrix of lowstrength meteoric material. A Monte Carlo method was applied to simulate the distributions of impacts, their directions and impact velocities.


1988 ◽  
Vol 102 ◽  
pp. 243-246
Author(s):  
J.T. Costello ◽  
W.G. Lynam ◽  
P.K. Carroll

AbstractThe dual laser-produced plasma technique for the study of ionic absorption spectra has been developed by the use of two Q-switched ruby lasers to enable independent generation of the absorbing and back-lighting plasmas. Optical pulse handling is used in the coupling cicuits to enable reproducible pulse delays from 250 nsec. to 10 msec, to be achieved. At delay times > 700 nsec. spectra of essentially pure neutral species are observed. The technique is valuable, not only for obtaining the neutral spectra of highly refractory and/or corrosive materials but also for studying behaviour of ionic species as a function of time. Typical spectra are shown in Fig. 1.


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