Determination of energy transport parameters in flat, layered targets irradiated by picosecond Nd-laser pulses

1981 ◽  
Vol 21 (12) ◽  
pp. 1657-1661 ◽  
Author(s):  
J.C. Couturaud ◽  
P.A. Holstein ◽  
M. Louis-Jacquet ◽  
B. Meyer ◽  
G. Thiell
1996 ◽  
Vol 61 (6) ◽  
pp. 844-855 ◽  
Author(s):  
Olga Šolcová ◽  
Petr Schneider

It was shown that the sampling loop, detector and connecting elements in the chromatographic set-up for determination of transport parameters by the dynamic method significantly influence the response peaks from columns packed with porous or nonporous particles. A method, based on the use of convolution theorem, was developed which can take these effects into account. The applicability of this method was demonstrated on the case of axial dispersion in a single-pellet-string column (SPSR) packed with nonporous particles. It is possible to handle also responses from columns packed with porous particles by a similar procedure.


2012 ◽  
Vol 85 (3) ◽  
Author(s):  
M. Wen ◽  
L. L. Jin ◽  
H. Y. Wang ◽  
Z. Wang ◽  
B. F. Shen ◽  
...  

1998 ◽  
Vol 16 (2) ◽  
pp. 397-404 ◽  
Author(s):  
A. Giulietti ◽  
C. Beneduce ◽  
T. Ceccotti ◽  
D. Giulietti ◽  
L.A. Gizzi ◽  
...  

An investigation of second harmonic (SH) and X-ray emissions from Al plasmas produced by 3-ns, 1.064-μm laser pulses at 1014 W/cm2 is reported. The SH and X-ray yields are strongly correlated as a function of the target position with respect to the laser beam focus. The SH originates from the underdense coronal plasma and has a filamentary source, while the X-ray source is uniform. The results suggest that, although the X-ray emission is significantly enhanced by the filamentation of the laser light in the corona, there is a smoothing effect in the energy transport process toward the overdense region.


2011 ◽  
Vol 46 (24) ◽  
pp. 7799-7805
Author(s):  
J. B. Rojas-Trigos ◽  
A. Calderón ◽  
E. Marín

2013 ◽  
Vol 87 (2) ◽  
pp. 025604 ◽  
Author(s):  
Alaa S Al-Kabbi ◽  
Kriti Sharma ◽  
G S S Saini ◽  
S K Tripathi

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