Laser-induced plasma formation in water at nanosecond to femtosecond time scales: calculation of thresholds, absorption coefficients, and energy density

1999 ◽  
Vol 35 (8) ◽  
pp. 1156-1167 ◽  
Author(s):  
J. Noack ◽  
A. Vogel
1993 ◽  
Vol 69 (1-4) ◽  
pp. 290-298 ◽  
Author(s):  
W. Marine ◽  
M. Gerri ◽  
P. Thomsen-Schmidt ◽  
J.M. Scotto d'Aniello

1998 ◽  
Author(s):  
Alfred Vogel ◽  
Kester Nahen ◽  
Dirk Theisen ◽  
Reginald Birngruber ◽  
Robert J. Thomas ◽  
...  

1989 ◽  
Vol 8 (2) ◽  
pp. 172-175 ◽  
Author(s):  
S. W. Amy ◽  
M. I. Large ◽  
A. E. Vaughan

AbstractThe Molonglo Observatory Synthesis Telescope is equipped with a transient event monitoring system which operates during normal synthesis observations. The device is designed to respond to impulsive signals which occur within the passband (843.0 ± 1.5 MHz) with time scales between 0.001 ms and 800 ms. The multiple beam facility of the telescope provides some discrimination against local interference. An upper limit of 1.7 × 10−2 events s−1 sr−1 has been placed on celestial events with durations between 1 ms and 25 ms and energy density ≥ 10−28 J m−2 Hz−1. The monitoring system has been recently reconfigured to improve the recognition and rejection of impulsive signals of non-celestial origin.


1989 ◽  
Vol 48 (3) ◽  
pp. 283-287 ◽  
Author(s):  
S. Jovićević ◽  
N. Konjević ◽  
N. I. Chapliev ◽  
V. I. Konov ◽  
S. M. Pimenov

1999 ◽  
Vol 38 (16) ◽  
pp. 3636 ◽  
Author(s):  
Alfred Vogel ◽  
Kester Nahen ◽  
Dirk Theisen ◽  
Reginald Birngruber ◽  
Robert J. Thomas ◽  
...  

2002 ◽  
Vol 88 (7) ◽  
Author(s):  
Vasan Venugopalan ◽  
Arnold Guerra ◽  
Kester Nahen ◽  
Alfred Vogel

2003 ◽  
Vol 28 (3) ◽  
pp. 206 ◽  
Author(s):  
François Courvoisier ◽  
Véronique Boutou ◽  
Catherine Favre ◽  
Steven C. Hill ◽  
Jean-Pierre Wolf

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