Abstract
AT the radio observatory near Dwingeloo, a beginning has been made with measurements of solar radiation at 400 Mc./s. The aim is to obtain quantitative data about transients of short duration (pips), and possibly some insight into the underlying mechanism which excites the coronal plasma. Some parameters in question are: length of the time interval between half-power points (duration), intensity, asymmetry, frequency band-width and polarization-rate.
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Reber, G., Nature, 175, 132 (1955).
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DE GROOT, T. Short Time Transients in Solar Noise. Nature 180, 382 (1957). https://doi.org/10.1038/180382a0
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DOI: https://doi.org/10.1038/180382a0
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