Temporal and spatial variations in the Io torus
References (52)
Jovian SII torus: Its longitudinal asymmetry
Icarus
(1980)The Inner Magnetosphere of Jupiter and the Io Plasma Torus
Variable Plasma Conditions Inside Io's Orbit: Voyager Measurements
(1984)- et al.
Direct plasma measurements in the Io torus and inner magnetosphere of Jupiter
J. Geophys. Res.
(1981) - et al.
Coulomb Thermal Properties and Stability of the Io Plasma Torus
(1983) - et al.
Dawn-dusk electric field asymmetry of the Io plasma torus
Geophys. Res. Lett.
(1983) The low-energy plasma in the Jovian magnetosphere
A model of Jupiter's sulfur nebula
Astrophys. J.
(1976)Measurements of SII optical emission from the thermal plasma of Jupiter
Astrophys. J.
(1978)Observed departure of the Io plasma torus from rigid corotation with Jupiter
Astrophys. J. Lett.
(1983)
Spectrophotometric studies of the Io torus
On the nature of SII emission from the Io plasma torus
Astrophys. J.
(1982)
Latitudinal oscillations of plasma within the Io torus
J. Geophys. Res.
(1980)
Atomic processes with special application to gaseous nebulae
Aerosol measurements in the troposphere and stratosphere
Appl. Opt.
(1966)
Radial diffusion in Io's torus: Some implications from Voyager 1
Geophys. Res. Lett.
(1980)
Strong [NII] emission and abundances in the ring nebula
Astrophys. J.
(1977)
A rediscussion of the atmospheric extinction and the absolute spectral-energy distribution of Vega
Astrophys. J.
(1975)
Longitudinal asymmetry of the Io plasma torus
Geophys. Res. Lett.
(1984)
Heavy ions from the Galilean satellites and the centrifugal distortion of the Jovian magnetosphere
J. Geophys. Res.
(1976)
Detection of ionized sulfur in the Jovian magnetosphere
Astrophys. J.
(1976)
Theory of motion of Jupiter's Galilean satellites
Astron. Astrophys.
(1977)
Optics of the Atmosphere
(1976)
Thermal electron density in the Jovian magnetosphere
J. Geophys. Res.
(1978)
Transition probabilities for forbidden lines in the 3p3 configuration
Mon. Not. R. Astron. Soc.
(1982)
The [OII]-[SII] Spectra of Active Galactic Nuclei
(1983)
Cited by (33)
Cassini UVIS observations of the Io plasma torus. III. Observations of temporal and azimuthal variability
2006, IcarusCitation Excerpt :While the individual particles of the torus lag corotation by an amount appropriate for their radial distance, the group velocity of the compositional wave lags rigid corotation by 1.5%. The detection of azimuthal variability in the brightness of the [S II] 6716/6731 Å and 4069/4076 Å doublets but not in the brightness of the [O II] 3726/3729 Å doublet (Morgan, 1985), arises from the fact that the amplitude of the azimuthal variation of the S II mixing ratio ranges from 10 to 25% while the amplitude of the azimuthal variation of the O II mixing ratio is ⩽5%. The correlation of S II brightness with S III brightness observed by Rauer et al. (1993) is also consistent with the correlation of the S II and S III mixing ratios observed by UVIS.
Io magnetospheric phenomena
1995, Advances in Space ResearchSolar system exploration from the moon: Synoptic and comparative study of bodies in our planetary system
1994, Advances in Space ResearchLow-resolution spectra of the Io plasma torus 2 days after the Ulysses encounter
1993, Planetary and Space Science
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