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Journal ArticleDOI

Ordinary and Z-mode emissions from the Jovian polar region

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TLDR
The Ulysses Unified Radio and Plasma (URAP) experiment has detected a new component of Jupiter's radio spectrum in the frequency range from about 10 to 30 kHz, which is emitted in the magnetoionic ordinary mode from a localized corotating source in the northern polar region as mentioned in this paper.
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This article is published in Planetary and Space Science.The article was published on 1993-11-01. It has received 10 citations till now. The article focuses on the topics: Jovian & Jupiter.

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Citations
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Journal ArticleDOI

Auroral radio emissions at the outer planets: Observations and theories

TL;DR: In this article, the authors review both observational and theoretical aspects of the generation of auroral radio emissions at the outer planets, trying to organize the former in a coherent frame set by the latter.
Journal ArticleDOI

Auroral radio emissions, 1. Hisses, roars, and bursts

TL;DR: The Earth's auroral electrons produce copious nonthermal radio emissions of various types, including auroral kilometric radiation (AKR), whistler mode auroral hiss, mode conversion radiation such as auroral roar and MF-burst, and possibly HF/VHF emissions as mentioned in this paper.
Journal ArticleDOI

Z mode waves as the source of Saturn narrowband radio emissions

TL;DR: In this article, the authors reported 5 kHz narrowband Z mode emissions observed by the Cassini Radio and Plasma Waves Science (RPWS) instrument during high latitude perikrone passes.
Journal ArticleDOI

Asymmetries in the Io plasma torus

TL;DR: In this article, Ulysses radio wave data taken during the 1992 Jupiter encounter was used to conclude that there are significant large and small spatial scale azimuthal asymmetries at high latitudes in the Io plasma torus.
Journal ArticleDOI

Narrowband Z-mode emissions interior to Saturn's plasma torus

TL;DR: In this article, a set of narrow bandwidth plasma emissions were detected by the Radio and Plasma Wave Science (RPWS) instrument in the inner magnetosphere, with individual tone bandwidths as low as a few hundred Hertz.
References
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Book

Radio waves in the ionosphere

K. G. Budden, +1 more
Journal ArticleDOI

A theory of the terrestrial kilometric radiation

TL;DR: In this paper, it was found that reflected electrons can result in the amplification of electromagnetic waves via a relativistic normal cyclotron resonance, which may explain the recently discovered terrestrial kilometric radiation.
Journal ArticleDOI

Charged particle distributions in Jupiter's magnetosphere

TL;DR: In situ data from the Pioneer and Voyager spacecraft, supplemented by earth-based observations and theoretical considerations, are used as the basis for the present quantitative, compact model of the 1 eV-several MeV charged particle distribution in the Jovian magnetosphere.
Book ChapterDOI

Phenomenology of magnetospheric radio emissions

TL;DR: The radio spectrum of Jupiter has been observed over 24 octaves of the radio spectrum, from about 0.01 MHz to 300,000 MHz, and three distinct types of radiation are responsible for this radio spectrum: thermal emission from the atmosphere accounts for virtually all the radiation at the high frequency end as mentioned in this paper.
Journal ArticleDOI

Overview of the Voyager ultraviolet spectrometry results through Jupiter encounter

TL;DR: The observations of a number of objects by the Voyager EUV instruments are summarized in this article, and the summary is considered to demonstrate the wide ranging application of the EUV spectroscopy and emphasizes the continuing importance of the search and discovery nature of spectroscopic techniques.
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