Attenuation and forward scattering of short-duration laser radiation in a strongly scattering medium

1997 ◽  
Vol 27 (7) ◽  
pp. 649-652 ◽  
Author(s):  
Nikolai S Vorob'ev ◽  
Vitalii M Podgaetskii ◽  
A V Smirnov ◽  
Sergei A Tereshchenko
1993 ◽  
Vol 48 (2) ◽  
pp. 1369-1377 ◽  
Author(s):  
P. Jungner ◽  
Å. Lindberg ◽  
B. Ståhlberg

2010 ◽  
Vol 28 (3) ◽  
pp. 371-375 ◽  
Author(s):  
A.N. Starodub ◽  
N.G. Borisenko ◽  
A.A. Fronya ◽  
Yu.A. Merkuliev ◽  
M.V. Osipov ◽  
...  

AbstractExperimental results obtained with “Kanal-2” facility under the study of powerful laser pulse interaction with the low density microstructure media are presented and discussed in this paper. Forward scattering, back scattering, and transmission of laser radiation by aerogel foil plasma have been investigated. The temporal, spectral, and energy characteristics of both the radiation scattering in the direction of heating radiation beam and the back scattering radiation were studied; the directional diagrams of forward and back scattering radiation were obtained for ω0 and 2ω0 frequencies. Analysis of intensity redistribution on the heating beam cross-section after passing through a polymer microstructure target was carried out.


1997 ◽  
Vol 55 (3) ◽  
pp. 330-333
Author(s):  
E A Alipieva ◽  
I Mandadjiev ◽  
V A Polischuk

1999 ◽  
Author(s):  
Vitaly M. Podgaetsky ◽  
Sergei A. Tereshchenko ◽  
Sergey V. Selishchev ◽  
Alexander V. Smirnov ◽  
Nikolai S. Vorobiev

1999 ◽  
Vol 173 ◽  
pp. 249-254
Author(s):  
A.M. Silva ◽  
R.D. Miró

AbstractWe have developed a model for theH2OandOHevolution in a comet outburst, assuming that together with the gas, a distribution of icy grains is ejected. With an initial mass of icy grains of 108kg released, theH2OandOHproductions are increased up to a factor two, and the growth curves change drastically in the first two days. The model is applied to eruptions detected in theOHradio monitorings and fits well with the slow variations in the flux. On the other hand, several events of short duration appear, consisting of a sudden rise ofOHflux, followed by a sudden decay on the second day. These apparent short bursts are frequently found as precursors of a more durable eruption. We suggest that both of them are part of a unique eruption, and that the sudden decay is due to collisions that de-excite theOHmaser, when it reaches the Cometopause region located at 1.35 × 105kmfrom the nucleus.


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