X-ray lasing by optical-field-induced ionization

1991 ◽  
Vol 66 (20) ◽  
pp. 2589-2592 ◽  
Author(s):  
Peter Amendt ◽  
David C. Eder ◽  
Scott C. Wilks
Keyword(s):  
1997 ◽  
Vol 56 (6) ◽  
pp. 5183-5186 ◽  
Author(s):  
K. Nagashima ◽  
T. Matoba ◽  
H. Takuma

Author(s):  
Eric W. Flesch
Keyword(s):  
X Ray ◽  

AbstractThis automated catalogue combines all the largest published optical, radio, and X-ray sky catalogues to find probable radio/X-ray associations to optical objects, plus double radio lobes, using uniform processing against all input data. The total count is 1 002 855 optical objects so presented. Each object is displayed with J2000 astrometry, optical and radio/X-ray identifiers, red and blue photometry, and calculated probabilities and optical field solutions of the associations. This is the third and final edition of this method.


Author(s):  
M.-C. Chou ◽  
T.-S. Hung ◽  
J.-Y. Lin ◽  
P.-H. Lin ◽  
S.-Y. Chen ◽  
...  
Keyword(s):  

2001 ◽  
Author(s):  
Katsuya Oguri ◽  
Hidetoshi Nakano ◽  
Tadashi Nishikawa ◽  
Naoshi Uesugi

1995 ◽  
Author(s):  
Katsumi Midorikawa ◽  
Yutaka Nagata ◽  
Minoru Obara ◽  
Hideo Tashiro ◽  
Koichi Toyoda
Keyword(s):  

Author(s):  
M. -C. Chou ◽  
P. -H. Lin ◽  
R. -P. Huang ◽  
S. -Y. Chen ◽  
H. -H. Chu ◽  
...  

1995 ◽  
Vol 13 (4) ◽  
pp. 459-468 ◽  
Author(s):  
S. Borgström ◽  
T. Starczewski ◽  
S. Svanberg ◽  
C.-G. Wahlström ◽  
E. Fill ◽  
...  

The time-dependent soft X-ray emission of helium and nitrogen plasmas generated by optical-field ionization is reported. The experiments were carried out by focusing pulses of the high-power Ti:sapphire laser of the Lund Institute of Technology (λ = 796 nm, pulse duration 150 fs, pulse energy 150 mJ) to a 50-μm diameter spot close to a nozzle, using He and N2 as target gases. The emission on He+, N4+, and N3+ resonance lines was recorded by means of a flat-field grating spectrometer coupled to an X-ray streak camera. A pronounced difference in the temporal shape of the emission of the Lyman-α line of hydrogen-like helium and of the 2p−3d resonance lines of lithium-like and beryllium-like nitrogen was observed. The helium line exhibited an initial spike followed by a slow revival of the emission, whereas the nitrogen lines showed a slow decay after a fast initial rise. These observations are explained with the help of simulations.


1995 ◽  
Author(s):  
D. C. Eder ◽  
P. Amendt ◽  
L. B. DaSilva ◽  
T. D. Donnelly ◽  
R. W. Falcone ◽  
...  
Keyword(s):  

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