International audienceMAJIS is the visible-infrared spectral imager of the JUICE mission, scheduled by ESA to explore Jupiter and its three icy Galilean moons starting in 2030. It will encounter a challenging environment, the intense Jovian magnetosphere, which among the various expected effects of radiation on detector operability, raises the major issue of transient signal perturbations generated by electrons during every acquisition. This paper aims at a precise characterization of the consequences of such a flux of high-energy electrons on MAJIS detectors in order to evaluate their impact on their operability. To assess the effects of this environment on MAJIS during the mission, we exposed two candidate detectors for the mission to β- ...
We quantitatively describe the Jovian energetic electron environment using the Solid State Imager (S...
The relationship between electron energy flux and the characteristic energy of electron distribution...
We present observations of 0.1-100 keV electrons from Juno's Jovian Auroral Distributions Experiment...
The JUICE (JUpiter ICy moons Explorer) mission by ESA aims to explore the emergence of habitable wor...
Thesis: Ph. D., Massachusetts Institute of Technology, Department of Aeronautics and Astronautics, 2...
International audienceRadio detection at high time-frequency resolutions is a powerful means of remo...
International audienceRadio detection at high time-frequency resolutions is a powerful means of remo...
A meticulous multi-instrument analysis of Juno observations for the first ten science orbits (PJ1, P...
The Jupiter Icy Moons Explorer is a planetary exploration mission that aims to study the moons of Ju...
The Jupiter Icy Moons Explorer is a planetary exploration mission that aims to study the moons of Ju...
The Jupiter Icy Moons Explorer is a planetary exploration mission that aims to study the moons of Ju...
The relationship between electron energy flux and the characteristic energy of electron distribution...
One of the most intriguing discoveries of Juno is the quasi-systematic detection of up-going electro...
The relationship between electron energy flux and the characteristic energy of electron distribution...
The relationship between electron energy flux and the characteristic energy of electron distribution...
We quantitatively describe the Jovian energetic electron environment using the Solid State Imager (S...
The relationship between electron energy flux and the characteristic energy of electron distribution...
We present observations of 0.1-100 keV electrons from Juno's Jovian Auroral Distributions Experiment...
The JUICE (JUpiter ICy moons Explorer) mission by ESA aims to explore the emergence of habitable wor...
Thesis: Ph. D., Massachusetts Institute of Technology, Department of Aeronautics and Astronautics, 2...
International audienceRadio detection at high time-frequency resolutions is a powerful means of remo...
International audienceRadio detection at high time-frequency resolutions is a powerful means of remo...
A meticulous multi-instrument analysis of Juno observations for the first ten science orbits (PJ1, P...
The Jupiter Icy Moons Explorer is a planetary exploration mission that aims to study the moons of Ju...
The Jupiter Icy Moons Explorer is a planetary exploration mission that aims to study the moons of Ju...
The Jupiter Icy Moons Explorer is a planetary exploration mission that aims to study the moons of Ju...
The relationship between electron energy flux and the characteristic energy of electron distribution...
One of the most intriguing discoveries of Juno is the quasi-systematic detection of up-going electro...
The relationship between electron energy flux and the characteristic energy of electron distribution...
The relationship between electron energy flux and the characteristic energy of electron distribution...
We quantitatively describe the Jovian energetic electron environment using the Solid State Imager (S...
The relationship between electron energy flux and the characteristic energy of electron distribution...
We present observations of 0.1-100 keV electrons from Juno's Jovian Auroral Distributions Experiment...