Overlayer-induced Auger Line-shape Changes: The Case of the PL2, 3VVTransition at the InP(110)/Sb interface

1992 ◽  
Vol T41 ◽  
pp. 259-264 ◽  
Author(s):  
L Calliari ◽  
M Sancrotti ◽  
L Duò ◽  
R Cosse ◽  
P Weightman ◽  
...  
Keyword(s):  
1980 ◽  
Vol 100 (3) ◽  
pp. A403
Author(s):  
S.S. Chao ◽  
E.-A. Knabbe ◽  
R.W. Vook
Keyword(s):  
Cu Films ◽  

1980 ◽  
Vol 100 (3) ◽  
pp. 581-589 ◽  
Author(s):  
S.S. Chao ◽  
E.-A. Knabbe ◽  
R.W. Vook
Keyword(s):  
Cu Films ◽  

1977 ◽  
Vol 14 (1) ◽  
pp. 232-235 ◽  
Author(s):  
J. T. Grant ◽  
R. G. Wolfe ◽  
M. P. Hooker ◽  
R. W. Springer ◽  
T. W. Haas

Carbon ◽  
1984 ◽  
Vol 22 (2) ◽  
pp. 216
Author(s):  
M Lagues ◽  
D Marchand ◽  
C Fretigny ◽  
A.P Legrand

1996 ◽  
Vol 150 ◽  
pp. 337-340
Author(s):  
David Clarke

AbstractThe scattering function of Hong's successful model for the brightness variation with elongation, B(ε), of the Zodiacal Light has been used to calculate profiles of Doppler shifted Fraunhofer lines. Substantial line shape changes with ε are predicted with an indication of a bifurcation at ε < 30°, so offering an explanation for reported F corona observations.


1984 ◽  
Vol 138 (2-3) ◽  
pp. 549-560 ◽  
Author(s):  
M. Dayan ◽  
S.V. Pepper
Keyword(s):  

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