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.
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.
https://doi.org/10.1038/308166a0
Maeda, K, and Carr, T D.
1984.
"Beam structure of Jupiter's decametric radiation."
United Kingdom.
https://doi.org/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 = []
volume = {308:5955}
journal type = {AC}
place = {United Kingdom}
year = {1984}
month = {Mar}
}
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 = []
volume = {308:5955}
journal type = {AC}
place = {United Kingdom}
year = {1984}
month = {Mar}
}