A solar radio spectrograph with high time resolution

Solar Physics ◽  
1972 ◽  
Vol 26 (2) ◽  
pp. 386-392 ◽  
Author(s):  
B. L. Gotwols ◽  
J. Phipps
1994 ◽  
Vol 144 ◽  
pp. 285-287
Author(s):  
K. Jiřička ◽  
M. Karlický ◽  
O. Kepka ◽  
A. Tlamicha

AbstractNew Ondřejov solar radio observational system consisting of a high-time resolution 3000 MHz receiver and of a 100-4200 MHz radiospectrograph is described and some results of observation of fast drift bursts, spikes, and continua are presented.


1994 ◽  
Vol 144 ◽  
pp. 431-434
Author(s):  
M. Minarovjech ◽  
M. Rybanský

AbstractThis paper deals with a possibility to use the ground-based method of observation in order to solve basic problems connected with the solar corona research. Namely:1.heating of the solar corona2.course of the global cycle in the corona3.rotation of the solar corona and development of active regions.There is stressed a possibility of high-time resolution of the coronal line photometer at Lomnický Peak coronal station, and use of the latter to obtain crucial observations.


2010 ◽  
Vol 180 (4) ◽  
pp. 424 ◽  
Author(s):  
G.M. Beskin ◽  
S.V. Karpov ◽  
S.F. Bondar ◽  
V.L. Plokhotnichenko ◽  
A. Guarnieri ◽  
...  

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