scholarly journals Extreme Ultraviolet Explorer spectra of the Io plasma torus: Improved spectral resolution and new results

2001 ◽  
Vol 106 (A11) ◽  
pp. 26293-26309 ◽  
Author(s):  
Floyd Herbert ◽  
G. Randall Gladstone ◽  
Gilda E. Ballester
Keyword(s):  
Spectral Resolution ◽  
Extreme Ultraviolet ◽  
Plasma Torus ◽  
Io Plasma Torus

Response of Jupiter's inner magnetosphere to the solar wind derived from extreme ultraviolet monitoring of the Io plasma torus

2016 ◽  
Vol 43 (24) ◽  
pp. 12,308-12,316 ◽  
Author(s):  
Go Murakami ◽  
Kazuo Yoshioka ◽  
Atsushi Yamazaki ◽  
Fuminori Tsuchiya ◽  
Tomoki Kimura ◽  
...  
Keyword(s):  
Solar Wind ◽  
Extreme Ultraviolet ◽  
Inner Magnetosphere ◽  
Plasma Torus ◽  
Io Plasma Torus

scholarly journals Identification of Extreme Ultraviolet Emission Lines of the Io Plasma Torus Observed by Hisaki/EXCEED

2018 ◽  
Vol 123 (7) ◽  
pp. 1723-1731 ◽  
Author(s):  
R. Hikida ◽  
K. Yoshioka ◽  
G. Murakami ◽  
T. Kimura ◽  
F. Tsuchiya ◽  
...  
Keyword(s):  
Extreme Ultraviolet ◽  
Emission Lines ◽  
Ultraviolet Emission ◽  
Plasma Torus ◽  
Io Plasma Torus

Extreme ultraviolet explorer satellite observation of Jupiter's Io plasma torus

1994 ◽  
Vol 426 ◽  
pp. L51 ◽  
Author(s):  
D. T. Hall ◽  
G. R. Gladstone ◽  
H. W. Moos ◽  
F. Bagenal ◽  
J. T. Clarke ◽  
...  
Keyword(s):  
Extreme Ultraviolet ◽  
Satellite Observation ◽  
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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