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Frequency drift and fine structure of 200-Mc/s solar bursts
Published online by Cambridge University Press: 14 August 2015
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In 1957 high-speed records were obtained at a frequency of 200 Mc/s during solar radio noise storms at the Solar Observatory at Harestua. For the registrations a receiver of bandwidth 0.3 Mc/s and time constant 0.01 seconds was used in connection with a Brush recorder. Most records were secured at a paper speed of 25 mm/second.
- Type
- Part II: The Sun
- Information
- Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 248 - 250
- Copyright
- Copyright © Stanford University Press 1959
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