X-ray Compton line scan tomography*

2015 ◽  
Vol 57 (11-12) ◽  
pp. 985-991
Author(s):  
Andreas Kupsch ◽  
Axel Lange ◽  
Manfred P. Hentschel ◽  
Gerd-Rüdiger Jaenisch ◽  
Nikolay Kardjilov ◽  
...  
Keyword(s):  
X Ray ◽  
Author(s):  
P.E. Batson ◽  
C.R.M. Grovenor ◽  
D.A. Smith ◽  
C. Wong

In this work As doped polysilicon was deposited onto (100) silicon wafers by APCVD at 660°C from a silane-arsine mixture, followed by a ten minute anneal at 1000°C, and in one case a further ten minute anneal at 700°C. Specimens for TEM and STEM analysis were prepared by chemical polishing. The microstructure, which is unchanged by the final 700°C anneal,is shown in Figure 1. It consists of numerous randomly oriented grains many of which contain twins.X-ray analysis was carried out in a VG HB5 STEM. As K α x-ray counts were collected from STEM scans across grain and twin boundaries, Figures 2-4. The incident beam size was about 1.5nm in diameter, and each of the 20 channels in the plots was sampled from a 1.6nm length of the approximately 30nm line scan across the boundary. The bright field image profile along the scanned line was monitored during the analysis to allow correlation between the image and the x-ray signal.


1989 ◽  
Vol 16 (1) ◽  
pp. 98-104 ◽  
Author(s):  
Claus-C. Glüer ◽  
Wolf-R. Dix ◽  
Klaus Engelke ◽  
Walter Graeff ◽  
Wolfram Kupper ◽  
...  
Keyword(s):  
X Ray ◽  

1984 ◽  
Vol 31 (1) ◽  
pp. 548-552 ◽  
Author(s):  
H. D. Zeman ◽  
E. B. Hughes ◽  
J. N. Otis ◽  
J. Rolfe ◽  
A. C. Thompson
Keyword(s):  
X Ray ◽  

Author(s):  
Chang-Won Heo ◽  
Ji-Hye Jang ◽  
Liyan Jin ◽  
Sung-Kyn Heo ◽  
Tae-Woo Kim ◽  
...  
Keyword(s):  
X Ray ◽  

1990 ◽  
Author(s):  
Michael Lohmann ◽  
Wolf-Rainer Dix ◽  
Klaus Engelke ◽  
Walter Graeff ◽  
Joachim Heuer ◽  
...  

1986 ◽  
Vol 33 (1) ◽  
pp. 515-518 ◽  
Author(s):  
H. D. Zeman ◽  
E. B. Hughes ◽  
J. N. Otis ◽  
G. S. Brown ◽  
A. C. Thompson

1963 ◽  
Vol 7 ◽  
pp. 382-394 ◽  
Author(s):  
Kurt F. J. Heinrich

AbstractWhile conventional X-ray signal readout systems can be used in connection with the electron probe analyzer, new readout techniques can be applied with advantage, particularly for scanning procedures. Several novel techniques involving photographic recordings of oscilloscope tracings will be described. These techniques are applicable to area scanning (enhanced concentration method, concentration mapping with use of X-ray signals, and target current concentration mapping procedures) as well as line scanning. Combinations of area-scanning images with line-scan registration ate used for representing line-scan results.By using operational amplifiers as signal adders, wavelength scans can be efficiently registered on a Polaroid photogram, with baseline indication and wavelength markers, in a single exposure. Another wavelength scanning technique registers the pulse height of the lines observed during the scanning operation, so that the order of reflection of the lines can be established. The use of an x-y recorder also offers advantages in the registration of line scans. Techniques for registration of multiple scans and for concentration mapping with the x-y recorder will be described.


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.


1994 ◽  
Vol 144 ◽  
pp. 1-9
Author(s):  
A. H. Gabriel

The development of the physics of the solar atmosphere during the last 50 years has been greatly influenced by the increasing capability of observations made from space. Access to images and spectra of the hotter plasma in the UV, XUV and X-ray regions provided a major advance over the few coronal forbidden lines seen in the visible and enabled the cooler chromospheric and photospheric plasma to be seen in its proper perspective, as part of a total system. In this way space observations have stimulated new and important advances, not only in space but also in ground-based observations and theoretical modelling, so that today we find a well-balanced harmony between the three techniques.


Sign in / Sign up

Export Citation Format

Share Document