Pulse compression vl4, velocity bunching with the LLNL Thomson x-ray source photoinjector

Author(s):  
S.G. Anderson ◽  
W.J. Brown ◽  
A.M. Trernaine ◽  
P. Musurneci ◽  
J.B. Rosenzweig
Keyword(s):  
1984 ◽  
Vol 23 (Part 2, No. 1) ◽  
pp. L57-L58 ◽  
Author(s):  
Takashi Yabe
Keyword(s):  
Ion Beam ◽  

1985 ◽  
Vol 24 (Part 2, No. 2) ◽  
pp. L104-L106 ◽  
Author(s):  
Takashi Yabe
Keyword(s):  
Ion Beam ◽  

2013 ◽  
Vol 20 (4) ◽  
pp. 550-554 ◽  
Author(s):  
Jaromir Hrdý ◽  
Peter Oberta

It is shown theoretically that the asymmetric or inclined double-crystal X-ray monochromator may be used for X-ray pulse compression if the pulse is properly chirped. By adjusting the mutual distance of the two asymmetric or inclined crystals it should be possible to achieve even a sub-femtosecond compression of a chirped free-electron laser pulse. The smalld-spacing of the crystal enables a more compact scheme compared with the currently used grating compression scheme. The asymmetric cut of the crystal enables the acceptance of a larger bandwidth. The inclined cut has larger tunability.


2002 ◽  
Vol 205 (4-6) ◽  
pp. 351-359 ◽  
Author(s):  
H.N. Chapman ◽  
K.A. Nugent
Keyword(s):  

Author(s):  
M.E. Cuneo ◽  
D.B. Sinars ◽  
G.R. Bennett ◽  
B.M. Jones ◽  
E.P. Yu ◽  
...  
Keyword(s):  
X Ray ◽  

1994 ◽  
Vol 144 ◽  
pp. 275-277
Author(s):  
M. Karlický ◽  
J. C. Hénoux

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.


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