pulse behavior
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2020 ◽  
Vol 37 (11) ◽  
pp. 3358
Author(s):  
William Kamgaing Mabou ◽  
Chancelor Pokam Nguewawe ◽  
David Yemélé

2020 ◽  
Vol 53 (3) ◽  
pp. 623-628
Author(s):  
Jaromír Hrdý

The development of ultrashort X-ray pulse sources requires optics that keep the pulse length as short as possible. One source of pulse stretching is the penetration of the pulse into a crystal during diffraction. Another source is the inclination of the intensity front when the diffraction is asymmetric. The theory of short X-ray pulse diffraction has been well developed by many authors. As it is rather complicated, it is sometimes difficult to foresee the pulse behavior (mainly stretching) during diffraction in various crystal arrangements. In this article, a simple model is suggested that gives a qualitatively similar shape to the diffracted pulse which follows from exact theory. It allows proposal of what experimental arrangement is optimal to minimize the pulse stretching during diffraction. First, the effect of pulse stretching due to penetration into a crystal surface is studied. On the basis of this, the pulse profile change during diffraction by two crystals, either symmetric or asymmetric, is predicted.


2017 ◽  
Vol 13 (S337) ◽  
pp. 263-266
Author(s):  
S. Chatterjee ◽  
R. S. Wharton ◽  
J. M. Cordes ◽  
G. C. Bower ◽  
B. J. Butler ◽  
...  

AbstractPhased VLA observations of the Galactic center magnetar J1745-2900 over 8-12 GHz reveal rich single pulse behavior. The average profile is comprised of several distinct components and is fairly stable over day timescales and GHz frequencies. The average profile is dominated by the jitter of relatively narrow pulses. The pulses in each of the four profile components are uncorrelated in phase and amplitude, although the occurrence of pulse components 1 and 2 appear to be correlated. Using a collection of the brightest individual pulses, we verify that the index of the dispersion law is consistent with the expected cold plasma value of 2. The scattering time is weakly constrained, but consistent with previous measurements, while the dispersion measure DM = 1763+3−10 pc cm−3 is lower than previous measurements, which could be a result of time variability in the line-of-sight column density or changing pulse profile shape over time or frequency.


2017 ◽  
Vol 24 (4) ◽  
pp. 2034-2040 ◽  
Author(s):  
David French ◽  
Susan Heidger ◽  
Daniel Enderich ◽  
David Lepell ◽  
Robert Richter-Sand
Keyword(s):  

2015 ◽  
Vol 35 (3) ◽  
pp. 167-176
Author(s):  
Assaf Bitman ◽  
Shaul Pearl ◽  
Inon Moshe ◽  
Zeev Zalevsky

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