Observations of Jovian decametric emissions by spaced receiver network

Details Observations of Jovian decametric emissions by spaced receiver network Observations of Jovian decametric emissions by spaced receiver network

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978sterj...2..144t&link_type=abstract

Solar Terrestrial Environmental Research in Japan, vol. 2, July 1, 1978, p. 144-147.

Other

Decametric Waves, Jupiter Atmosphere, Planetary Radiation, Radio Receivers, Reception Diversity, Data Recording, Emission Spectra, Ground Stations, Interplanetary Space, Polarization Characteristics, Power Spectra, Scintillation

Scientific paper

The objectives of the observational study (which began in mid-1977) of Jovian decametric emission (JDE) are to: (1) estimate the angular structure of the JDE sources, (2) identify the causes of JDE intensity fluctuations at frequencies less than 10 Hz, and (3) to search for relationships among interplanetary scintillations and other radiation characteristics obtained from dynamic spectra and polarization measurements. The block diagram of the receiver-recording system used at each station of the spaced network is presented along with some sample results.

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