The Apollo 17 command service module in lunar orbit will carry a far ultraviolet scanning spectrometer whose prime mission will be to measure the composition of the lunar atmosphere. Additional observations will include the spectral lunar albedo, the temporary atmosphere injected by the engines of the lunar exploration module, the solar system atmosphere, the galactic atmosphere and the spectra of astronomical sources, including the earth. A detailed description of the experimental equipment which observes the spectral range 1180 to 1680 A, the observing program and broad speculation about the possible results of the experiment, are presented
Engineering prototype ion mass spectrometer for mass analysis of lunar atmospher
A rocket-borne Ebert spectrometer and telescope were used for analysis of the solar spectrum. The in...
An experiment using Earth based remote sensing radar, infrared eclipse, and color difference data to...
Proposed supporting studies for the Apollo 17 UV spectrometer include analyses of existing data and ...
The Large Magellanic Cloud was observed by the far ultraviolet camera spectrograph from the lunar su...
The design, development, manufacture, test and calibration of five lunar orbital mass spectrometers ...
Radiation in the wavelength interval 150-350 nm initiates chemical reactions in the lower mesosphere...
Over 700 far UV photos were obtained with the S201 electrographic camera on Skylab 4 (27 Nov. 1973 -...
The Lunar Atmosphere and Dust Environment Explorer (LADEE) is a lunar orbiter launched in September ...
Authors have conducted a program of research focused on studies of the lunar atmosphere. Also presen...
Contains a brief description of each surface experiment including the scientific objectives, the par...
The principal objective is presented of the UV observations, with emphasis placed on hydrogen and he...
Experiments on Apollo missions 15, 16, and 17 were utilized in an attempt to learn about the induced...
The Infrared Scanning Radiometer (ISR) was designed to map the thermal emission of the lunar surface...
Lunar atmosphere research has tended to center on gases with predictably large sources and on those ...
Engineering prototype ion mass spectrometer for mass analysis of lunar atmospher
A rocket-borne Ebert spectrometer and telescope were used for analysis of the solar spectrum. The in...
An experiment using Earth based remote sensing radar, infrared eclipse, and color difference data to...
Proposed supporting studies for the Apollo 17 UV spectrometer include analyses of existing data and ...
The Large Magellanic Cloud was observed by the far ultraviolet camera spectrograph from the lunar su...
The design, development, manufacture, test and calibration of five lunar orbital mass spectrometers ...
Radiation in the wavelength interval 150-350 nm initiates chemical reactions in the lower mesosphere...
Over 700 far UV photos were obtained with the S201 electrographic camera on Skylab 4 (27 Nov. 1973 -...
The Lunar Atmosphere and Dust Environment Explorer (LADEE) is a lunar orbiter launched in September ...
Authors have conducted a program of research focused on studies of the lunar atmosphere. Also presen...
Contains a brief description of each surface experiment including the scientific objectives, the par...
The principal objective is presented of the UV observations, with emphasis placed on hydrogen and he...
Experiments on Apollo missions 15, 16, and 17 were utilized in an attempt to learn about the induced...
The Infrared Scanning Radiometer (ISR) was designed to map the thermal emission of the lunar surface...
Lunar atmosphere research has tended to center on gases with predictably large sources and on those ...
Engineering prototype ion mass spectrometer for mass analysis of lunar atmospher
A rocket-borne Ebert spectrometer and telescope were used for analysis of the solar spectrum. The in...
An experiment using Earth based remote sensing radar, infrared eclipse, and color difference data to...