Auger line shape changes in epitaxial (111)Pd/(111)Cu films

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 ◽  

1992 ◽  
Vol T41 ◽  
pp. 259-264 ◽  
Author(s):  
L Calliari ◽  
M Sancrotti ◽  
L Duò ◽  
R Cosse ◽  
P Weightman ◽  
...  
Keyword(s):  

1981 ◽  
Vol 109 (2) ◽  
pp. A308
Author(s):  
Y. Namba ◽  
R.W. Vook ◽  
S.S. Chao
Keyword(s):  

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

1981 ◽  
Vol 109 (2) ◽  
pp. 320-330 ◽  
Author(s):  
Y. Namba ◽  
R.W. Vook ◽  
S.S. Chao
Keyword(s):  

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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