Narrow-band interference filter images were obtained for the Io torus at the S II wavelengths of 6716, 6731 and at the wavelenght of the S III, 9532 spectrum. The purpose of these observations is to study the short term temporal behavior of the torus and to gain a better understanding of the systematic morphology of the torus. From these images, estimates were obtained for the electron and ion densities and ion temperatures as a function of longitude, latitude, radius from Jupiter, and time. From the analysis of images taken in 1983 and 1984, extremely sharp longitudinal variations in plasma density were detected, subcorotational velocities were measures in the torus plasma, the presence of an optical east-west brightness asymmetry was conf...
Jupiter hosts very intense auroral emissions, which originates from various magnetospheric processes...
The jovian moon Io disperses about 1 ton/s of material in the planetary magnetosphere, mainly b...
Observations of the Io plasma torus made before, during, and after the impact of Comet Shoemaker‐Lev...
Ground‐based high‐resolution spectra of emission from the Io plasma torus obtained during 53 nights ...
The short wavelength spectrography on the IUE satellite was used to obtain spectra of the plasma tor...
A Fabry-Perot spectrometer was used to obtain images of the Io torus in emission lines of S II (wave...
In this third paper in a series presenting observations by the Cassini Ultraviolet Imaging Spectrome...
The research performed in this project is divided in two main investigations: (1) the synthesis and ...
We present a 6-month baseline of spatially resolved measurements of the Io plasma torus intensity an...
Implications of recent developments for the neutral particle environment of Jupiter are considered. ...
Io is the solar system’s most volcanically active body. This volcanic activity results in the ejecti...
In this third paper in a series presenting observations by the Cassini Ultraviolet Imaging Spectrome...
A synoptic campaign of Io and Io plasma torus observations were conducted near the Jupiter 2007 and ...
International audienceWe study the Jovian hectometric (HOM) emissions recorded by the RPWS (Radio an...
Io is the primary source of plasma in the Jovian magnetosphere, continuously releasing approximately...
Jupiter hosts very intense auroral emissions, which originates from various magnetospheric processes...
The jovian moon Io disperses about 1 ton/s of material in the planetary magnetosphere, mainly b...
Observations of the Io plasma torus made before, during, and after the impact of Comet Shoemaker‐Lev...
Ground‐based high‐resolution spectra of emission from the Io plasma torus obtained during 53 nights ...
The short wavelength spectrography on the IUE satellite was used to obtain spectra of the plasma tor...
A Fabry-Perot spectrometer was used to obtain images of the Io torus in emission lines of S II (wave...
In this third paper in a series presenting observations by the Cassini Ultraviolet Imaging Spectrome...
The research performed in this project is divided in two main investigations: (1) the synthesis and ...
We present a 6-month baseline of spatially resolved measurements of the Io plasma torus intensity an...
Implications of recent developments for the neutral particle environment of Jupiter are considered. ...
Io is the solar system’s most volcanically active body. This volcanic activity results in the ejecti...
In this third paper in a series presenting observations by the Cassini Ultraviolet Imaging Spectrome...
A synoptic campaign of Io and Io plasma torus observations were conducted near the Jupiter 2007 and ...
International audienceWe study the Jovian hectometric (HOM) emissions recorded by the RPWS (Radio an...
Io is the primary source of plasma in the Jovian magnetosphere, continuously releasing approximately...
Jupiter hosts very intense auroral emissions, which originates from various magnetospheric processes...
The jovian moon Io disperses about 1 ton/s of material in the planetary magnetosphere, mainly b...
Observations of the Io plasma torus made before, during, and after the impact of Comet Shoemaker‐Lev...