Hostname: page-component-745bb68f8f-grxwn Total loading time: 0 Render date: 2025-02-06T22:19:37.113Z Has data issue: false hasContentIssue false
  • English
  • Français

Frequency drift and fine structure of 200-Mc/s solar bursts

Published online by Cambridge University Press:  14 August 2015

Ø. Elgarøy
Ø. Elgarøy*
Affiliation:
Institute of Theoretical Astrophysics, Oslo, Norway

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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