scholarly journals Some Recollections of the Radio and Electrical Engineering Division of the National Research Council of Canada, 1946-1977

2009 ◽  
Vol 15 (2) ◽  
pp. 155-175
Author(s):  
Arthur E. Covington
Keyword(s):  
Radio Astronomy ◽  
World Wide ◽  
Research Council ◽  
Solar Radio ◽  
Electrical Engineering ◽  
National Research Council ◽  
Radio Noise ◽  
Field Station ◽  
Radio Observatory ◽  
Solar Radio Astronomy

Abstract Studies of extraterrestrial radio noise became world wide after WWII, and were rapidly separated into a number of disciplines. Solar radio astronomy, at a wavelength of 10.7 cm, was initiated in 1946 at the Radio Field Station of the National Research Council. Its development at the Goth Hill Radio Observatory outside Ottawa is outlined until 1962, when the work was transferred to the Algonquin Radio Observatory.

Solar Radio Astronomy at Low Frequencies

2002 ◽  
Vol 199 ◽  
pp. 415-425
Author(s):  
Monique Pick
Keyword(s):  
Radio Telescope ◽  
Radio Astronomy ◽  
Coronal Mass Ejections ◽  
Solar Radio ◽  
Electron Beams ◽  
Solar Physics ◽  
Interplanetary Shocks ◽  
Radio Observations ◽  
Low Frequencies ◽  
Solar Radio Astronomy

This review is concerned to study of sun at frequencies lower than 1.4 GHz. Emphasis is made on results which illustrate the topics in which GMRT could play a major role. Coordinated studies including spectral and imaging radio observations are important for research in solar physics. Joint observations between the Giant Meter Radio Telescope (GMRT) with radio instruments located in the same longitude range are encouraged. This review inludes three distinct topics: Electron beams and radio observations- Radio signatures of Coronal Mass Ejections- Radio signatures of coronal and interplanetary shocks.

scholarly journals 60. Relation between optical solar features and solar radio emission

1957 ◽  
Vol 4 ◽  
pp. 327-333
Author(s):  
H. W. Dodson
Keyword(s):  
Radio Emission ◽  
Radio Frequency ◽  
Research Council ◽  
Solar Radio ◽  
National Research Council ◽  
Solar Radio Emission ◽  
Radio Frequency Radiation ◽  
Cornell University ◽  
Frequency Radiation

During the last five years, we at the McMath-Hulbert Observatory have been attempting to determine the characteristics of radio-frequency radiation associated with certain of the transient solar features that we normally observe on monochromatic spectroheliograms or in integrated light. We have had the privilege of using the original 200 Mc./s. records at Cornell University and the 2800 Mc./s. records at the National Research Council in Ottawa.

Sign in / Sign up

Export Citation Format

Share Document