On Theoretical Modelling of Continuously Inhomogeneous Semiconductor Structures

1985 ◽  
Vol 129 (1) ◽  
pp. 399-406 ◽  
Author(s):  
U. Henniger ◽  
R. Keiper
1995 ◽  
Vol 165 (7) ◽  
pp. 799 ◽  
Author(s):  
Boris A. Volkov ◽  
B.G. Idlis ◽  
M.Sh. Usmanov

1995 ◽  
Vol 38 (7) ◽  
pp. 761-771 ◽  
Author(s):  
Boris A Volkov ◽  
B G Idlis ◽  
M Sh Usmanov

1972 ◽  
Vol 15 (3) ◽  
pp. 385-391
Author(s):  
D. I. Bilenko ◽  
V. S. Il'in ◽  
G. P. Kostyunina ◽  
N. P. Kazanova

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.


1992 ◽  
Vol 139 (5) ◽  
pp. 353 ◽  
Author(s):  
J. Pelayo ◽  
J. Paniello ◽  
N. Gisin ◽  
J.W. Burgmeijer ◽  
M. Blondel ◽  
...  

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