The spectrum and angular distribution of x rays scattered from a water phantom

1995 ◽  
Vol 22 (8) ◽  
pp. 1235-1245 ◽  
Author(s):  
Chee-Wai Cheng ◽  
Kenneth W. Taylor ◽  
Arthur F. Holloway
1957 ◽  
Vol 30 (351) ◽  
pp. 129-135 ◽  
Author(s):  
D. V. Cormack ◽  
T. J. Griffith ◽  
H. E. Johns

1985 ◽  
Vol 110 (9) ◽  
pp. 477-479 ◽  
Author(s):  
V.G. Baryshevsky ◽  
V.A. Danilov ◽  
O.L. Ermakovich ◽  
I.D. Feranchuk ◽  
A.V. Ivashin ◽  
...  
Keyword(s):  

1985 ◽  
Vol 30 (1) ◽  
pp. 21-29 ◽  
Author(s):  
G E Giakoumakis ◽  
D M Miliotis
Keyword(s):  

2006 ◽  
Vol 38 (12-13) ◽  
pp. 1618-1621
Author(s):  
Z. M. Zhang ◽  
T. Chen ◽  
R. Shimizu ◽  
H. Yoshikawa ◽  
T. Koshikawa ◽  
...  

1991 ◽  
Vol 24 (13) ◽  
pp. 3009-3018 ◽  
Author(s):  
A Hitachi ◽  
Y Awaya ◽  
T Kambara ◽  
Y Kanai ◽  
M Kase ◽  
...  

1997 ◽  
Vol 04 (05) ◽  
pp. 919-922 ◽  
Author(s):  
A. FANELSA ◽  
R. SCHELLENBERG ◽  
F. U. HILLEBRECHT ◽  
E. KISKER

Magnetic dichroism has been observed in the angular distribution of p-core level photoemission spectra excited from crystalline ferromagnets by unpolarized X-rays. The angular dependence of the angular and energy-resolved photoemission intensity was recorded as a function of the emission direction with respect to the crystal, revealing a strong variation of the magnetic dichroism with emission angle due to photoelectron diffraction. This variation is particularly strong around the forward scattering peaks, including sign reversals close to these directions. The results demonstrate that any standard X-ray photoelectron spectroscopy apparatus possesses the potential for combined analysis of surface magnetic structure and geometric structure in a chemically specific way.


1991 ◽  
Vol 43 (3) ◽  
pp. 1455-1460 ◽  
Author(s):  
K. S. Kahlon ◽  
H. S. Aulakh ◽  
N. Singh ◽  
R. Mittal ◽  
K. L. Allawadhi ◽  
...  
Keyword(s):  

1972 ◽  
Vol 14 ◽  
pp. 761-762
Author(s):  
G. Elwert ◽  
E. Haug

The polarization and angular distribution of solar hard X radiation above 10 keV was calculated under the assumption that the X rays originate as bremsstrahlung from energetic electrons moving in a preferred direction. The source electrons are supposed to have a power-law spectrum. These conditions are to be expected in the impulsive phase of an X-ray burst. The spiral orbits of the electrons around the magnetic field lines are taken into account.


Sign in / Sign up

Export Citation Format

Share Document