scholarly journals Hot electron component in the Io plasma torus confirmed through EUV spectral analysis

2011 ◽  
Vol 116 (A9) ◽  
pp. n/a-n/a ◽  
Author(s):  
K. Yoshioka ◽  
I. Yoshikawa ◽  
F. Tsuchiya ◽  
M. Kagitani ◽  
G. Murakami
Keyword(s):  
Spectral Analysis ◽  
Hot Electron ◽  
Electron Component ◽  
Plasma Torus ◽  
Io Plasma Torus

Io plasma torus and the source of jovian narrow-band kilometric radiation

Nature ◽  
1987 ◽  
Vol 327 (6122) ◽  
pp. 492-495 ◽  
Author(s):  
Dyfrig Jones
Keyword(s):  
Narrow Band ◽  
Plasma Torus ◽  
Io Plasma Torus

scholarly journals Cassini UVIS observations of the Io plasma torus

Icarus ◽  
2008 ◽  
Vol 194 (1) ◽  
pp. 153-165 ◽  
Author(s):  
A.J. Steffl ◽  
P.A. Delamere ◽  
F. Bagenal
Keyword(s):  
Plasma Torus ◽  
Io Plasma Torus

The proton concentration in the vicinity of the Io plasma torus

1982 ◽  
Vol 87 (A12) ◽  
pp. 10395 ◽  
Author(s):  
R. L. Tokar ◽  
D. A. Gurnett ◽  
F. Bagenal
Keyword(s):  
Proton Concentration ◽  
Plasma Torus ◽  
Io Plasma Torus

Ground-based observations of the [SII] 6731 Å emission lines of the Io plasma torus

2016 ◽  
Vol 12 (S328) ◽  
pp. 227-229
Author(s):  
P. Magalhães Fabíola ◽  
Walter Gonzalez ◽  
Ezequiel Echer ◽  
Mariza P. Souza-Echer ◽  
Rosaly Lopes ◽  
...  
Keyword(s):  
Charged Particles ◽  
Emission Lines ◽  
Solar Telescope ◽  
The Moon ◽  
Active Object ◽  
Oxygen Ions ◽  
Galilean Moons ◽  
Plasma Torus ◽  
Io Plasma Torus ◽  
Galilean Moons Of Jupiter

AbstractThe Io Plasma Torus (IPT) is a doughnut-shaped structure of charged particles, composed mainly of sulfur and oxygen ions. The main source of the IPT is the moon Io, the most volcanically active object in the Solar System. Io is the innermost of the Galilean moons of Jupiter, the main source of the magnetospheric plasma and responsible for injecting nearly 1 ton/s of ions into Jupiter's magnetosphere. In this work ground-based observations of the [SII] 6731 Å emission lines are observed, obtained at the MacMath-Pierce Solar Telescope. The results shown here were obtained in late 1997 and occurred shortly after a period of important eruptions observed by the Galileo mission (1996-2003). Several outbursts were observed and periods of intense volcanic activity are important to correlate with periods of brightness enhancements observed at the IPT. The time of response between an eruption and enhancement at IPT is still not well understood.

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