TH-C-T-6E-08: High Resolution Film Based Finite Pencil Beam Model for MLC Defined Beamlets

2005 ◽  
Vol 32 (6Part21) ◽  
pp. 2168-2168
Author(s):  
B Lynch ◽  
M Ranade ◽  
J Li ◽  
D Low ◽  
J Dempsey
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.


1969 ◽  
Vol 1 (5) ◽  
pp. 216-217
Author(s):  
A. E. Le Marne ◽  
P. A. Shaver

In a current programme at the Molonglo Radio Observatory using the high-resolution pencil beam of the instrument (∼3′ arc) an attempt is being made to extend the measured spectra of known planetary nebulae down to 408 MHz. Of 23 such planetaries already investigated, 14 have been detected. The main results will be given elsewhere; here it is proposed to discuss in detail only the well-known planetary nebula IC 418.


2014 ◽  
Vol 41 (6Part22) ◽  
pp. 384-384
Author(s):  
A Cardin ◽  
S Avery ◽  
M Maryanski ◽  
X Ding ◽  
A Kassaee ◽  
...  

1992 ◽  
Vol 19 (2) ◽  
pp. 263-273 ◽  
Author(s):  
Anders Ahnesjö ◽  
Mikael Saxner ◽  
Avo Trepp

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