The principal objective is presented of the UV observations, with emphasis placed on hydrogen and helium. Calculations are given for airglow and occultation. Mission requirements and trajectories are also reported for future observations
Radiation in the wavelength interval 150-350 nm initiates chemical reactions in the lower mesosphere...
The Apollo 17 command service module in lunar orbit will carry a far ultraviolet scanning spectromet...
The following subject areas are covered: (1) the science program (star formation and origins of plan...
The Voyager Ultraviolet Spectrometer (UVS) is an objective grating spectrometer covering the wavelen...
Atmospheric properties of Saturn's rings as measured by an ultraviolet spectrometer onboard the Mari...
Ultraviolet spectra fo the comet West obtained by sounding rocket experiments in 1976 are reproduced...
International audienceThe study of the Solar System is fundamental to answer key questions from spac...
We compare International Ultraviolet Explorer (IUE) spectral observations of Jupiter's UltraViolet (...
An intensive program of observations of the Comet Halley during the week of the Vega 2 and Giotto en...
UV-SCOPE is a mission concept to determine the causes of atmospheric mass loss in exoplanets, invest...
Radiation in the wavelength interval 150-350 nm initiates chemical reactions in the lower mesosphere...
The Apollo 17 command service module in lunar orbit will carry a far ultraviolet scanning spectromet...
The following subject areas are covered: (1) the science program (star formation and origins of plan...
The Voyager Ultraviolet Spectrometer (UVS) is an objective grating spectrometer covering the wavelen...
Atmospheric properties of Saturn's rings as measured by an ultraviolet spectrometer onboard the Mari...
Ultraviolet spectra fo the comet West obtained by sounding rocket experiments in 1976 are reproduced...
International audienceThe study of the Solar System is fundamental to answer key questions from spac...
We compare International Ultraviolet Explorer (IUE) spectral observations of Jupiter's UltraViolet (...
An intensive program of observations of the Comet Halley during the week of the Vega 2 and Giotto en...
UV-SCOPE is a mission concept to determine the causes of atmospheric mass loss in exoplanets, invest...
Radiation in the wavelength interval 150-350 nm initiates chemical reactions in the lower mesosphere...
The Apollo 17 command service module in lunar orbit will carry a far ultraviolet scanning spectromet...
The following subject areas are covered: (1) the science program (star formation and origins of plan...