Journal ArticleDOI
Io Jupiter interaction, millisecond bursts and field-aligned potentials
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TLDR
In this paper, the authors performed an automated analysis of 230 high-resolution dynamic spectra of S-bursts, providing 5 × 10 6 frequency drift measurements and confirmed over a large number of measurements that the frequency drift d f / d t (f ) is in average negative and decreases (in absolute value) at high frequencies, as predicted by the adiabatic theory.About:
This article is published in Planetary and Space Science.The article was published on 2007-01-01. It has received 61 citations till now. The article focuses on the topics: Jupiter & Jovian.read more
Citations
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Journal ArticleDOI
Explanation of dominant oblique radio emission at Jupiter and comparison to the terrestrial case
TL;DR: The Io-Jupiter S-bursts are a series of quasi-periodic impulsive decameter radio emissions from the magnetic flux tube connecting Jupiter to its closest galilean satellite Io as mentioned in this paper.
Journal ArticleDOI
Magnetic coupling of planets and small bodies with a pulsar wind
TL;DR: In this article, the electromagnetic interaction of a relativistic stellar wind with a planet or a smaller body in orbit around a pulsar was investigated, and it was shown that a pair of stationary Alfven waves, called AW, is expected to form on the sides of the planet and they could be strong sources of radio emissions.
Journal ArticleDOI
Fast and slow frequency-drifting millisecond bursts in Jovian decametric radio emissions
Vladimir B. Ryabov,Ph. Zarka,S. Hess,A. A. Konovalenko,G. Litvinenko,V. V. Zakharenko,V. A. Shevchenko,Baptiste Cecconi +7 more
TL;DR: In this article, the authors present an analysis of several Jovian Io-related decametric radio storms recorded in 2004−2012 at the Ukrainian array UTR-2 using the new generation of baseband digital receivers.
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Electron-beam-induced Radio Emission from Ultracool Dwarfs
S. Yu,J. G. Doyle,Alexey A. Kuznetsov,Gregg Hallinan,A. Antonova,Alexander L. MacKinnon,Aaron Golden +6 more
TL;DR: In this article, numerical simulations for an electron-beam-driven and loss-cone-driven electron-cyclotron maser with different plasma parameters and different magnetic field strengths for a relatively small region and short timescale are presented.
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Modulation structures in the dynamic spectra of Jovian radio emission obtained with high time-frequency resolution
G. Litvinenko,Alain Lecacheux,Helmut O. Rucker,A. A. Konovalenko,B. Ryabov,U. Taubenschuss,V. V. Vinogradov,V. E. Shaposhnikov +7 more
TL;DR: In this paper, a wide-band dynamic spectra of Jovian decameter emission obtained over the last decade with high-frequency and high time resolution equipment on the largest decameters band antenna array, the Ukrainian T-shape Radio telescope (UTR-2), is presented.
References
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Journal ArticleDOI
A theory of the terrestrial kilometric radiation
C. S. Wu,Lou-Chuang Lee +1 more
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.
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Observations of paired electrostatic shocks in the polar magnetosphere
F. S. Mozer,C. W. Carlson,Mary K. Hudson,Roy B. Torbert,B. Parady,J. Yatteau,Michael C. Kelley +6 more
TL;DR: In this article, a polar orbiting satellite was used to measure spatially confined regions of extremely large electric fields in the auroral zone at altitudes below 8000 km, which are identified as paired electrostatic shocks which are associated with electrostatic ion cyclotron wave turbulence.
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Nonlinear standing Alfvén wave current system at Io: Theory
TL;DR: In this article, a nonlinear analytical model of the Alfven current tubes continuing the currents through Io (or rather its ionosphere) generated by the unipolar inductor effect due to Io's motion relative to the magnetospheric plasma was presented.
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New models of Jupiter's magnetic field constrained by the Io flux tube footprint
TL;DR: In this paper, a spherical harmonic model of the magnetic field of Jupiter was derived from in situ magnetic field measurements and remote observations of the position of the foot of the Io flux tube in Jupiter's ionosphere.