Absolute x-ray calibration of a gated x-ray framing camera for the Laser MegaJoule facility in the 0.1 keV–1 keV spectral range

2021 ◽  
Vol 92 (3) ◽  
pp. 035101
Author(s):  
S. Hubert ◽  
F. Boubault
Keyword(s):  
X Ray ◽  
1984 ◽  
Vol 86 ◽  
pp. 215-218
Author(s):  
P. Mandelbaum ◽  
M. Klapisch ◽  
A. Krasnitz ◽  
A. Zigler

X-ray spectra of highly ionized atoms (Tm to Pt) emitted from Laser produced plasma are characterized by the simple structure given by resonant transitions of the Nil-like ions, accompanied by the more complex pattern of satellite transitions emitted by ions in the neighbouring states of ionization. An analysis of these structures has been given recently for the satellites of the 3d10 − 3d94p[l] and of the 3p63dl0 − 3p53d104s, 4d[2] transitions of the Nil-like inns. However, most of the radiation emitted in this spectral range [4–10Å] concentrate in a wide, rather structureless satellite feature in the long wavelength side of the 3d10 −3d94f Ni-I like transition, on which some lines are superimposed. Line identification has been achieved successfully with the methods of [1], [2] and will be published separately. In this communication, we deal only with the pseudocontinuum.


2004 ◽  
Author(s):  
John A. Oertel ◽  
Tom Archuleta ◽  
Mike S. Bakeman ◽  
Phillip Sanchez ◽  
George Sandoval ◽  
...  
Keyword(s):  
X Ray ◽  

2014 ◽  
Vol 26 (10) ◽  
pp. 102001
Author(s):  
李晋 Li Jin ◽  
杨志文 Yang Zhiwen ◽  
杨品 Yang Pin ◽  
杨正华 Yang Zhenghua ◽  
董建军 Dong Jianjun ◽  
...  

Author(s):  
Allan S. Johnson ◽  
Timur Avni ◽  
Esben W. Larsen ◽  
Dane R. Austin ◽  
Jon P. Marangos

High harmonic generation (HHG) of an intense laser pulse is a highly nonlinear optical phenomenon that provides the only proven source of tabletop attosecond pulses, and it is the key technology in attosecond science. Recent developments in high-intensity infrared lasers have extended HHG beyond its traditional domain of the XUV spectral range (10–150 eV) into the soft X-ray regime (150 eV to 3 keV), allowing the compactness, stability and sub-femtosecond duration of HHG to be combined with the atomic site specificity and electronic/structural sensitivity of X-ray spectroscopy. HHG in the soft X-ray spectral region has significant differences from HHG in the XUV, which necessitate new approaches to generating and characterizing attosecond pulses. Here, we examine the challenges and opportunities of soft X-ray HHG, and we use simulations to examine the optimal generating conditions for the development of high-flux, attosecond-duration pulses in the soft X-ray spectral range. This article is part of the theme issue ‘Measurement of ultrafast electronic and structural dynamics with X-rays’.


1983 ◽  
Vol 105 (4) ◽  
pp. 316-320 ◽  
Author(s):  
J. M. Kabo ◽  
W. Goldsmith ◽  
N. M. Harris

Two unembalmed and one embalmed human cadaveric head-neck systems were instrumented and subjected to central forehead impact of ballistically suspended 3.07-kg aluminum shell at velocities ranging from 50 to 345 cm/s. Occipital skull accelerations and disk pressures were measured by transducers, while the deformation of the system was determined by framing camera data. The results were found to be in accord with those from corresponding tests in artifical head-neck replica. Initial and terminal X-ray examination of the structure revealed no evidence of either skull or vertebral fractures.


2018 ◽  
Vol 57 (07) ◽  
pp. 1 ◽  
Author(s):  
Zheng Yuan ◽  
Tao Chen ◽  
Zhiwen Yang ◽  
Jin Li ◽  
Zhurong Cao ◽  
...  

Optik ◽  
2019 ◽  
Vol 186 ◽  
pp. 374-378 ◽  
Author(s):  
Wenyong Fu ◽  
Houzhi Cai ◽  
Dong Wang ◽  
Yunfei Lei ◽  
Jinyuan Liu

1987 ◽  
Vol 93 ◽  
pp. 207-223
Author(s):  
J.P. Osborne

AbstractThe X-ray observatory EXOSAT spent over 1000 hours observing cataclysmic variables. Some of the major results reviewed here are: soft X-ray light curve changes in AM Her objects, orbital effects in the X-ray light curves of intermediate polars and U Gem, regular behaviour in the inter-outburst X-ray flux of VW Hyi, and X-ray emission from the tenuous remnant of the recent recurrent nova RS Oph. The ability of EXOSAT to make long uninterupted observations at high sensitivity over a broad spectral range and to react quickly to cosmic events has yielded a dataset of a quality that will not be surpassed for many years.


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