Far‐infrared measurements of the mobility and carrier concentration in lightly doped GaAs on Si(100)

1992 ◽  
Vol 72 (2) ◽  
pp. 631-637 ◽  
Author(s):  
S. Morley ◽  
D. R. T. Zahn ◽  
T. Eickhoff ◽  
W. Richter ◽  
D. A. Woolf ◽  
...  
1979 ◽  
Vol 19 (11) ◽  
pp. 5689-5693 ◽  
Author(s):  
S. W. McKnight ◽  
S. Perkowitz ◽  
D. B. Tanner ◽  
L. R. Testardi

1986 ◽  
Vol 6 (4) ◽  
pp. 403-415 ◽  
Author(s):  
Martin A. Pomerantz

AbstractThe geographic South Pole, where the United States maintains a year-round scientific station, affords a number of unique advantages for certain types of astronomical observations. These include: continuous viewing and constant declination of ail objects in the southern celestial hemisphere, exceedingly low humidity, extended periods of coronal seeing, high altitude, and uniform terrain. The areas of research that have already benefited immensely from thèse extraordinary features are helioseismology and submillimeter astronomy. Unparalleled observations of global solar oscillations have already yielded significant information about the structure and dynamics of the Sun’s interior. Far infrared measurements of various galactic and extra-galactic regions have attained an unprecedented level of sensitivity, limited for the first time only by the noise inherent in the detector. In addition to further helioseismological observations, currently planned future activities include observational cosmology and ultra high energy gamma ray astronomy.


2005 ◽  
Vol 430 (1) ◽  
pp. 343-353 ◽  
Author(s):  
Cs. Kiss ◽  
U. Klaas ◽  
D. Lemke

Author(s):  
Jun Wang ◽  
Chan Deng ◽  
Gang Jiazhi ◽  
Yifan Wang ◽  
Qi Wang ◽  
...  

1992 ◽  
Author(s):  
Alfred W. Cooper ◽  
Eugene C. Crittenden, Jr. ◽  
Edmund A. Milne ◽  
Philip L. Walker ◽  
E. Moss ◽  
...  

1983 ◽  
Vol 61 (2) ◽  
pp. 305-308
Author(s):  
M. S. Mathur ◽  
H. C. Card ◽  
K. C. Kao ◽  
S. R. Mejia ◽  
G. C. Tabisz

Hydrogenated amorphous-silicon thin films (a-Si:H) were deposited by microwave plasma chemical-vapour decomposition of SiH4, on thin polyethylene sheets. The high-resolution, far infrared measurements were performed on these films in the 700–50 cm−1 region on a Nicolet far infrared interferometer. The use of polyethylene as the substrate material permitted the determination of the absorption bands at 656.4, 652, 639.4, and 543 cm−1 with a shoulder at 539 cm−1 and a broad feature at 70.8 cm−1. These features provided evidence for SiH, SiH2 (as predicted by Lucovsky et al.), and SiH3 combinations in the film, as well as far more complex systems.


1975 ◽  
Vol 15 (1) ◽  
pp. 45-49 ◽  
Author(s):  
J.A. Alvarez ◽  
R.E. Jennings ◽  
A.F.M. Moorwood

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