Measured Polarization Components of Nonlinear Thomson Scattering

Author(s):  
J. Peatross ◽  
N. Atkinson ◽  
D. Hodge ◽  
B. Pratt ◽  
M. Romero ◽  
...  
1967 ◽  
Vol 31 ◽  
pp. 355-356
Author(s):  
R. D. Davies

Observations at various frequencies between 136 and 1400 MHz indicate a considerable amount of structure in the galactic disk. This result appears consistent both with measured polarization percentages and with considerations of the strength of the galactic magnetic field.


1979 ◽  
Vol 40 (C7) ◽  
pp. C7-851-C7-852
Author(s):  
B. Van der Sijde ◽  
T. Poorter ◽  
S. Adema ◽  
B. F.M. Pots ◽  
D. C. Schram

2016 ◽  
Vol 11 (01) ◽  
pp. C01052-C01052 ◽  
Author(s):  
M. Bassan ◽  
P. Andrew ◽  
G. Kurskiev ◽  
E. Mukhin ◽  
T. Hatae ◽  
...  

2021 ◽  
Vol 103 (6) ◽  
Author(s):  
Krzysztof Dzierżęga ◽  
Franciszek Sobczuk ◽  
Evgeny Stambulchik ◽  
Bartłomiej Pokrzywka

Crystals ◽  
2021 ◽  
Vol 11 (5) ◽  
pp. 528
Author(s):  
Marcel Ruijter ◽  
Vittoria Petrillo ◽  
Thomas C. Teter ◽  
Maksim Valialshchikov ◽  
Sergey Rykovanov

High-energy radiation can be generated by colliding a relativistic electron bunch with a high-intensity laser pulse—a process known as Thomson scattering. In the nonlinear regime the emitted radiation contains harmonics. For a laser pulse whose length is comparable to its wavelength, the carrier envelope phase changes the behavior of the motion of the electron and therefore the radiation spectrum. Here we show theoretically and numerically the dependency of the spectrum on the intensity of the laser and the carrier envelope phase. Additionally, we also discuss what experimental parameters are required to measure the effects for a beamed pulse.


2021 ◽  
Vol 92 (3) ◽  
pp. 033542
Author(s):  
L. G. Suttle ◽  
J. D. Hare ◽  
J. W. D. Halliday ◽  
S. Merlini ◽  
D. R. Russell ◽  
...  

2021 ◽  
Vol 92 (5) ◽  
pp. 053532
Author(s):  
M. Tomes ◽  
M. Carr ◽  
A. Meakins ◽  
M. Sos ◽  
P. Bohm ◽  
...  

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