Analysis of tolerances in a grating interferometer for high-resolution displacement measurement

Author(s):  
Marek Dobosz
1969 ◽  
Vol 1 (5) ◽  
pp. 192-194 ◽  
Author(s):  
D. G. Cole ◽  
R. F. Mullaly

The heights of solar radio sources at 1424 MHz and 696 MHz have been measured during the years 1965 and 1966. Solar activity at this time was near minimum. The number of radio sources appearing on the solar disk rarely exceeded three at any time and it thus was possible to resolve the majority of these with a high resolution grating interferometer. Many of the previous height measurements at these frequencies have been made near times of maximum solar activity and the confusion of sources within the beam has limited their accuracy. The number of sources studied here is quite considerably higher than in any previous investigation at these frequencies, and the period of observation has been continuous.


1961 ◽  
Vol 14 (3) ◽  
pp. 403 ◽  
Author(s):  
T Krishnan ◽  
NR Labrum

A study of the brightness distribution on the Sun at 21-cm wavelength on April 8, 1959, is described. High resolution observations were made of the partial eclipse on that day with a simple radiometer of high sensitivity. The brightness distribution of the uneclipsed Sun at the same wavelength was obtained using a cross-grating interferometer, which enabled the bright regions to be located accurately.


2010 ◽  
Vol 21 (11) ◽  
pp. 115304 ◽  
Author(s):  
H L Hsieh ◽  
J Y Lee ◽  
W T Wu ◽  
J C Chen ◽  
R Deturche ◽  
...  

2017 ◽  
Vol 25 (12) ◽  
pp. 2975-2985
Author(s):  
王磊杰 WANG Lei-jie ◽  
张 鸣 ZHANG Ming ◽  
朱 煜 ZHU Yu ◽  
鲁 森 LU Sen ◽  
杨开明 YANG Kai-ming

2017 ◽  
Vol 404 ◽  
pp. 132-138 ◽  
Author(s):  
Jie Lin ◽  
Jian Guan ◽  
Feng Wen ◽  
Jiubin Tan

Author(s):  
W.N. Christiansen ◽  
N.R. Labrum ◽  
K.R. McAlister ◽  
D.S. Mathewson

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