scholarly journals Susceptibility of soft X-ray grazing incidence telescopes to low energy electrons

1989 ◽  
Vol 238 (3) ◽  
pp. 1047-1054 ◽  
Author(s):  
T. J. Sumner ◽  
J. J. Quenby ◽  
R. Lieu ◽  
J. Daniels ◽  
R. Willingale ◽  
...  
1989 ◽  
Vol 67 (4) ◽  
pp. 358-364 ◽  
Author(s):  
G. W. Johnson ◽  
D. E. Brodie ◽  
E. D. Crozier

In this study, thin films of germanium have been vacuum deposited in four regimes. Care was taken to prepare reproducible films, which required that the partial pressure of water be below 10−8 Torr during deposition (1 Torr = 133.3 Pa). First, films deposited onto substrates held during deposition at a temperature Ts that is below 473 K are amorphous. Once annealed above 423 K, their electrical conductivity and optical band gap are independent of deposition temperature and rate, and of whether or not low-energy electron irradiation of the substrate is used during deposition. This suggests that a well-defined and reproducible structure is being prepared. Second, a "precrystallization regime" is obtained when Ts is between 473 and 513 K. Extended X-ray adsorption fine-structure and X-ray diffraction confirm that this regime is a two-phase mixture of amorphous material and crystallites. Third, films deposited with Ts near 513 K, while using low-energy electrons to bombard the substrate, are amorphous, but these films have different electrical and optical properties from the films m the first regime. From this, we infer that a second well-defined amorphous structure exists. Fourth, films deposited with Ts above 513 K are polycrystalline. Extended X-ray adsorption fine-structure and X-ray adsorption near-edge structure could not distinguish between the two amorphous materials in the first and third regimes.


2014 ◽  
Vol 10 (S313) ◽  
pp. 97-98
Author(s):  
Kenji Yoshida

AbstractSymmetric and triangle-shaped flux variability in X-ray and gamma-ray light curves is observed from many blazars. We derived the X-ray spectrum changing in time by using a kinetic equation of high energy electrons. Giving linearly changing the injection of low energy electrons into accelerating and emitting region, we obtained the preliminary results that represent the characteristic X-ray variability of the linear flux increase with hardening in the rise phase and the linear decrease with softening in the decay phase.


2010 ◽  
Vol 95 (2) ◽  
pp. 153-163 ◽  
Author(s):  
Sylvain Massey ◽  
Enrico Gallino ◽  
Pierre Cloutier ◽  
Michaël Tatoulian ◽  
Léon Sanche ◽  
...  

2004 ◽  
Vol 51 (6) ◽  
pp. 3408-3412 ◽  
Author(s):  
F. Lei ◽  
R. Nartallo ◽  
P. Nieminen ◽  
E. Daly ◽  
H. Evans ◽  
...  
Keyword(s):  

1972 ◽  
Vol 5 (3) ◽  
pp. 1016-1020 ◽  
Author(s):  
R. G. Steinhardt ◽  
J. Hudis ◽  
M. L. Perlman

2015 ◽  
Vol 30 (5) ◽  
pp. 1086-1099 ◽  
Author(s):  
Yves Kayser ◽  
Philipp Hönicke ◽  
Dariusz Banaś ◽  
Jean-Claude Dousse ◽  
Joanna Hoszowska ◽  
...  

Grazing XRF measurements allow for a non-destructive investigation of the depth distribution of ion implantations.


Author(s):  
ChangSheng Shi

Abstract We consider the Compton scattering in the optically thick uniform spherical corona around a neutron star in an X-ray binary. In the scattering, the low energy seed photons (0.1 ∼ 2.5 keV) are scattered in low energy electrons (2.5 ∼ 10 keV) in the corona in two conditions, i.e. initial seed photons are scattered in a whole corona and scattered in every layer of the corona that are supposed to be divided into many layers. When the same number of input seed photons, the same corona parameters and the same energy distribution of all photons in the two conditions are considered, the approximately same number of output photons can be obtained, which means that there is approximately a transform invariance of layering the Comptonized corona. Thus the scattering in the layers of a multi-layered corona is approximately equal to the scattering in the whole corona by dividing the whole corona into several layers. It means that Compton scattering for the initial seed photons scattered in a whole optically thick spherical corona with uniformly distributed electrons also can be considered as that the multiple Compton scatterings take place in the layers of a multi-layered corona in order approximately, which can be used to explore some physical process in one part of a corona.


Sign in / Sign up

Export Citation Format

Share Document