Demonstration of Transient Collisional Excitation X-Ray Lasers in Gases

2002 ◽  
Author(s):  
P. Lu
2001 ◽  
Vol 11 (PR2) ◽  
pp. Pr2-39-Pr2-42 ◽  
Author(s):  
M. Kado ◽  
T. Kawachi ◽  
N. Hasegawa ◽  
M. Tanaka ◽  
K. Sukegawa ◽  
...  

2001 ◽  
Vol 11 (PR2) ◽  
pp. Pr2-55-Pr2-57
Author(s):  
M. Tanaka ◽  
T. Kawachi ◽  
M. Kado ◽  
N. Hasegawa ◽  
K. Sukegawa ◽  
...  

1991 ◽  
Vol 9 (2) ◽  
pp. 493-499
Author(s):  
D. Naccache ◽  
J-L. Bourgade ◽  
P. Combis ◽  
C. J. Keane ◽  
J-P. Le Breton ◽  
...  

We present some significant results of collisional excitation X-ray laser experiments in plasmas produced by a laser. We studied the amplification in Ne- and Ni-like ions by varying both the nature and the thickness of targets, the irradiation, and the wavelength of the driving laser. Some potentially interesting scalings as a function of the atomic number of the lasing element are demonstrated in the Ne-like system. An order-of-magnitude increase in gain in the Ni-like experiments was determined.


1999 ◽  
Vol 5 (6) ◽  
pp. 1441-1446 ◽  
Author(s):  
J. Dunn ◽  
A.I. Osterheld ◽  
Yuelin Li ◽  
J. Nilsen ◽  
V.N. Shlyaptsev
Keyword(s):  

2001 ◽  
Vol 40 (Part 1, No. 2B) ◽  
pp. 1018-1021 ◽  
Author(s):  
Tsuneyuki Ozaki ◽  
Keiichi Yamamoto ◽  
Ruxin Li ◽  
Hiroto Kuroda

1990 ◽  
Vol 115 ◽  
pp. 21-31
Author(s):  
W. H. Goldstein

AbstractPrecision spectroscopy of solar plasmas has historically been the goad for advances in calculating the atomic physics and dynamics of highly ionized atoms. Recent efforts to understand the laboratory plasmas associated with magnetic and inertial confinement fusion, and with X-ray laser research, have played a similar role. Developments spurred by laboratory plasma research are applicable to the modeling of high-resolution spectra from both solar and cosmic X-ray sources, such as the photo-ionized plasmas associated with accretion disks. Three of these developments in large scale atomic modeling are reviewed: a new method for calculating large arrays of collisional excitation rates, a sum rule based method for extending collisional-radiative models and modeling the effects of autoionizing resonances, and a detailed level accounting calculation of resonant excitation rates in FeXVII.


2002 ◽  
Vol 09 (01) ◽  
pp. 641-644 ◽  
Author(s):  
MOMOKO TANAKA ◽  
TETSUYA KAWACHI ◽  
MASATAKA KADO ◽  
NOBORU HASEGAWA ◽  
KOUTA SUKEGAWA ◽  
...  

The spatial profile of the transient collisional excitation Ni-like Ag X-ray laser in various plasma lengths was observed using the near field imaging method. The gain region was the size of 50 μm and 30–50 μm distant from the target surface. The shapes of the gain region were crescent shape or consisted of two spots.


1996 ◽  
Vol 33 (1-3) ◽  
pp. 255-260
Author(s):  
Yoshiaki Kato ◽  
Hiroyuki Daido ◽  
Ryosuke Kodama ◽  
Kensuke Murai ◽  
Fumihiro Koike
Keyword(s):  

1988 ◽  
Vol 102 ◽  
pp. 221
Author(s):  
R.A. London ◽  
N.M. Ceglio ◽  
D.C. Eder ◽  
A.U. Hazi ◽  
C.J. Keane ◽  
...  

AbstractWe describe the experiments and supporting theoretical modelling to develop and characterize soft x-ray lasers. The x-ray lasers are created in dense plasmas produced by optical laser irradiation of solid targets with line focussed beams. We use mainly thin foil targets, which upon appropriate illumination, produce rather uniform plasmas. We consider laser schemes pumped by electron collisional excitation and dielectronic recombination in Ne-like and Ni-like ions, and schemes pumped by collisional and radiative recombination following rapid cooling for H-like and Li-like ions.Experimental measurements of the time and space resolved spectra taken both along the lasing axis and at other viewing angles, in addition to data on the angular pattern of x-ray laser radiation and on the absorption and scattering of the optical laser light are presented. These data allow us the determine the characteristics of the plasmas which have been created, as well as the properties of the x-ray lasers, such as the gain coefficients for the inverted transitions, and their spatial and temporal distributions. The modelling includes calculations of the absorption of the optical laser light, the hearing and hydrodynamics of the targets and the evolution of the atomic level populations within the plasma. Transfer of the emitted radiation is calculated, including resonance line trapping, amplification for inverted transitions, and refraction of the x-ray laser beam due to electron density gradients. Results are used to optimize x-ray laser designs before the experiments and to interpret the measured spectra.The latest experimental results from the NOVA laser facility on the performance of several laser schemes and on the use of multilayer mirrors to produce x-ray laser cavities are reported. These results arc compared to the models to test and improve our understanding of the complex physics involved in making x-ray lasers. Based on current experiments, we show how the modelling can be use to design shorter wavelength and more efficient schemes for use in applications such as x-ray holography.


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