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Duration of Transients in Solar Radio Noise

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Abstract

SINCE February this year, high-speed records have been obtained at a frequency of 200 Mc./sec. during solar radio noise storms. The equipment used for the registrations consists of a receiver with bandwidth of 0.3 Mc./sec. and time constant 0.01 sec. and a Brush recorder. Records were secured at various paper speeds, with a speed of 25 mm./sec. as that mostly used, since this speed seems to give the best compromise between the competing factors resolving power, amount of information and paper consumption.

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References

  1. de Groot, T., Nature, 180, 382 (1957).

    Article  ADS  Google Scholar 

  2. Reber, G., Nature, 175, 132 (1955).

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Authors and Affiliations

  1. Solar Observatory, Institute of Theoretical Astrophysics, University of Oslo,

    Ö. ELGARÖY

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  1. Ö. ELGARÖY
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ELGARÖY, Ö. Duration of Transients in Solar Radio Noise. Nature 180, 808–809 (1957). https://doi.org/10.1038/180808b0

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