Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-26T03:16:24.947Z Has data issue: false hasContentIssue false
  • English
  • Français

70. Some properties of solar radio-transients on fast 200 Mc./s. records

Published online by Cambridge University Press:  14 August 2015

C. De Jager  and
F. Van 'T Veer
C. De Jager
Affiliation:
Astronomical Observatory, Zonnenburg, Utrecht, Netherlands
F. Van 'T Veer
Affiliation:
Astronomical Observatory, Zonnenburg, Utrecht, Netherlands

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.

Some 6 km. of high-speed (Brush) records of the solar radio radiation at 200 Mc./s. made at Cornell University by Ch. L. Seeger in 1949 and 1950 have been kindly put at our disposal. They were made with a paper speed of 0·5 cm./sec., sometimes with 2·5 cm./sec. The response time of the recording pen was 0s·02. Some records have been made simultaneously at 205 Mc./s. and at 200 Mc./s. This paper gives some results of a discussion of these records. The properties that were studied are: the clustering tendencies among the radio-pips, their band-widths, the echo-phenomena and the duration of the pips.

Type
Part V: The Active Sun
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 366 - 370
Copyright
Copyright © Cambridge University Press 1957 

References

1. Jager, , de, C. and Veer, F. van 't. B.A.N. (in the Press).Google Scholar
2. Reber, G. Nature , 175, 132, 1955.CrossRefGoogle Scholar