The surface of lo may be covered with a layer of ammonia ice containing trace amounts of sodium potassium, and calcium; and atmospheric nitrogen could be formed as a photochemical product of ammonia photolysis. Intense sporadic sodium emission from Io can be excited by collisions involving vibrationally excited nitrogen molecules. These metastable molecules may be formed by electron impact, with electrons energized by an auroral mechanism. In order to account for the intensity ratio of the sodium doublet, it is necessary to invoke scattering in a thick gaseous envelope ejected by Io
Continued effort is reported to improve the emission rates of various emission lines for atomic oxyg...
To explain the unidentified spectral features of Io, as obtained by the Voyager infrared spectromete...
We heated mixtures of sulfur and Na-bearing silicates in evacuated silica glass capsules to temperat...
The surface of lo may be covered with a layer of ammonia ice containing trace amounts of sodium pot...
A variety of models for Io's atmosphere, ionosphere, surface, and environment are developed and disc...
International audienceWe report the results of model simulations performed to explain the nature of ...
International audienceWe report ground-based spectroscopic observations of the Io sodium cloud befor...
Io is surrounded by a halo of atoms which radiate in emission lines. This was discovered by groundb...
It is generally accepted that Io is the source of S, O, Na and K which, after ionization, form the c...
The general objective of this project is to advance theoretical understanding of Io's atmosphere and...
Io is the solar system’s most volcanically active body. This volcanic activity results in the ejecti...
The composition of the sodium-bearing molecular ion cloud in the vicinity of Io may yield clues to I...
line 9 AbstractDramatic changes in the brightness and shape of Jupiter’s extended sodium nebula are ...
Extrasolar satellites are generally too small to be detected by nominal searches. By analogy to the ...
Thanks to high-sensitivity (sub)millimeter spectroscopic observations, KCl and NaCl in gas phase hav...
Continued effort is reported to improve the emission rates of various emission lines for atomic oxyg...
To explain the unidentified spectral features of Io, as obtained by the Voyager infrared spectromete...
We heated mixtures of sulfur and Na-bearing silicates in evacuated silica glass capsules to temperat...
The surface of lo may be covered with a layer of ammonia ice containing trace amounts of sodium pot...
A variety of models for Io's atmosphere, ionosphere, surface, and environment are developed and disc...
International audienceWe report the results of model simulations performed to explain the nature of ...
International audienceWe report ground-based spectroscopic observations of the Io sodium cloud befor...
Io is surrounded by a halo of atoms which radiate in emission lines. This was discovered by groundb...
It is generally accepted that Io is the source of S, O, Na and K which, after ionization, form the c...
The general objective of this project is to advance theoretical understanding of Io's atmosphere and...
Io is the solar system’s most volcanically active body. This volcanic activity results in the ejecti...
The composition of the sodium-bearing molecular ion cloud in the vicinity of Io may yield clues to I...
line 9 AbstractDramatic changes in the brightness and shape of Jupiter’s extended sodium nebula are ...
Extrasolar satellites are generally too small to be detected by nominal searches. By analogy to the ...
Thanks to high-sensitivity (sub)millimeter spectroscopic observations, KCl and NaCl in gas phase hav...
Continued effort is reported to improve the emission rates of various emission lines for atomic oxyg...
To explain the unidentified spectral features of Io, as obtained by the Voyager infrared spectromete...
We heated mixtures of sulfur and Na-bearing silicates in evacuated silica glass capsules to temperat...