Spectral Types of Decametric Radiation from Jupiter

Details Spectral Types of Decametric Radiation from Jupiter Spectral Types of Decametric Radiation from Jupiter

Dec 1966

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1966natur.212.1338r&link_type=abstract

Nature, Volume 212, Issue 5068, pp. 1338-1339 (1966).

Astronomy and Astrophysics

Astronomy

7

Scientific paper

EXPERIMENTS relating to the spectral fine structure of decametric radiation from Jupiter have been described1,2. During the opposition of the planet in 1965 the high-resolution spectral experiment was repeated. The main equipment was the 14-channel spectrograph2 with channel-to-channel spacing of 50 kc/s and a frequency centred on 19.1 Mc/s. Some modifications were made to the antenna and display system so that the recording time constant was approximately 40 msec. I operated the spectrograph for 3-4 h each night from October 1 to December 31, 1965, at the Radio Astronomy Station of the University of Helsinki.

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