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Fine Spectral Structure of Solar Radio Storms

Published online by Cambridge University Press:  25 April 2016

D. McConnell
D. McConnell*
Affiliation:
University of Tasmania, Physics Department
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Extract

As part of an investigation of solar radio bursts at high time (≈ 1 msec) and frequency (≈ 10 kHz) resolution, observations have been made between 30 MHz with the Llanherne broadband radio telescope (Ferris 1980). The radio frequency signals in the six frequency ranges 30-33, 33-36, 38-41, 54-57 and 79-82 MHz were recorded on six video tape recorders for about 10 minutes each day near solar transit.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 64 - 67
Copyright
Copyright © Astronomical Society of Australia 1980

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References

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