Unified weak‐field magnetoresistance phenomenology for cubic and noncubic (001)‐ and (111)‐oriented epitaxial films and surface layers

1979 ◽  
Vol 34 (2) ◽  
pp. 158-159 ◽  
Author(s):  
R. S. Allgaier ◽  
J. B. Restorff ◽  
Bland Houston
1978 ◽  
Vol 49 (8) ◽  
pp. 4442-4445 ◽  
Author(s):  
R. S. Allgaier ◽  
Bland Houston ◽  
J. B. Restorff

1978 ◽  
Vol 47 (1) ◽  
pp. K31-K34 ◽  
Author(s):  
C. Albers ◽  
Ch. Walkowiak ◽  
P. Schäfer ◽  
I. Rechenberg

1989 ◽  
Vol 33 ◽  
pp. 13-23 ◽  
Author(s):  
D. Keith Bowen

AbstractThe techniques of X-ray topography are reviewed, with special reference to their application to the study of surface layers and thin films. The methods of section topography, white radiation topography and double and triple crystal topography are shown to be the most appropriate, with grazing or glancing incidence methods assuming special importance. Applications to the questions of epilayer mismatch and dislocation content, process-induced defects and surface damage are discussed.


1980 ◽  
Vol 51 (4) ◽  
pp. 2119 ◽  
Author(s):  
R. S. Allgaier ◽  
J. B. Restorff ◽  
Bland Houston ◽  
J. D. Jensen ◽  
A. Lopez-Otero
Keyword(s):  

1984 ◽  
Vol 75 ◽  
pp. 407-422
Author(s):  
William K. Hartmann

ABSTRACTThe nature of collisions within ring systems is reviewed with emphasis on Saturn's rings. The particles may have coherent icy cores and less coherent granular or frosty surface layers, consistent with thermal eclipse observations. Present-day collisions of such ring particles do not cause catastrophic fragmentation of the particles, although some minor surface erosion and reaccretion is possible. Evolution by collisional fragmentation is thus not as important as in the asteroid belt.


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