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Solar observations by the large pulkovo radio telescope at 3.2-cm wavelength
Published online by Cambridge University Press: 14 August 2015
Extract
The observations of the sun by the large Pulkovo radio telescope [1] began in 1956 December. In accordance with the antenna dimensions, a fan-beam diagram about one minute of arc in width and one degree in height was expected (at λ = 3.2 cm).
- Type
- Part II: The Sun
- Information
- Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 171 - 173
- Copyright
- Copyright © Stanford University Press 1959
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