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Beam structure of Jupiter's decametric radiation

Journal Article:

Abstract

The well-defined zones of central meridian longitude within which the probability of jovian radio emission at frequencies near 22 MHz is relatively high are known as sources A, B and C. Each consists of a component for which the emission probability is strongly correlated with Io's orbital position, and another that is Io-unrelated. The paper presents convincing evidence based on concurrent observations from two Voyager spacecraft and a terrestrial observatory that the component of source A radiation that is not correlated with Io's position is generally emitted in co-rotating searchlight beams of distinctive cross-sectional shape.
Authors:
Publication Date:
Mar 08, 1984
Product Type:
Journal Article
Reference Number:
AIX-15-060351; EDB-84-171770
Resource Relation:
Journal Name: Nature (London); (United Kingdom); Journal Volume: 308:5955
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; JUPITER PLANET; RADIOWAVE RADIATION; ANISOTROPY; BEAMS; EMISSION; EXPERIMENTAL DATA; FLUX DENSITY; JAPAN; MHZ RANGE 01-100; ORBIT STABILITY; TIME DEPENDENCE; VOYAGER SPACE PROBES; ASIA; DATA; ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; INFORMATION; MHZ RANGE; NUMERICAL DATA; PLANETS; RADIATIONS; SPACE VEHICLES; STABILITY; VEHICLES; 640107* - Astrophysics & Cosmology- Planetary Phenomena
OSTI ID:
6542687
Research Organizations:
Hyogo Coll. of Medicine, Japan
Country of Origin:
United Kingdom
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: NATUA
Submitting Site:
HEDB
Size:
Pages: 166-169
Announcement Date:
Oct 01, 1984

Journal Article:

Citation Formats

Maeda, K, and Carr, T D. Beam structure of Jupiter's decametric radiation. United Kingdom: N. p., 1984. Web. doi:10.1038/308166a0.
Maeda, K, & Carr, T D. Beam structure of Jupiter's decametric radiation. United Kingdom. doi:10.1038/308166a0.
Maeda, K, and Carr, T D. 1984. "Beam structure of Jupiter's decametric radiation." United Kingdom. doi:10.1038/308166a0. https://www.osti.gov/servlets/purl/10.1038/308166a0.
@misc{etde_6542687,
title = {Beam structure of Jupiter's decametric radiation}
author = {Maeda, K, and Carr, T D}
abstractNote = {The well-defined zones of central meridian longitude within which the probability of jovian radio emission at frequencies near 22 MHz is relatively high are known as sources A, B and C. Each consists of a component for which the emission probability is strongly correlated with Io's orbital position, and another that is Io-unrelated. The paper presents convincing evidence based on concurrent observations from two Voyager spacecraft and a terrestrial observatory that the component of source A radiation that is not correlated with Io's position is generally emitted in co-rotating searchlight beams of distinctive cross-sectional shape.}
doi = {10.1038/308166a0}
journal = {Nature (London); (United Kingdom)}
volume = {308:5955}
journal type = {AC}
place = {United Kingdom}
year = {1984}
month = {Mar}
}