Add to ORKGThe Mariner 9 spacecraft was successfully inserted into orbit around Mars. One of the five instruments on board, an infrared interferometer spectrometer is used to record the thermal emission spectrum of Mars between 200 and 2000 cm/1. The spatial resolution for vertical viewing is a circular area of approximately 110 km diameter for a periapsis height of 1400 km. The total number of calibrated spectra included in the final data set is 21167. The final calibrated thermal emission spectra contained in the reduced data records are reported
Time dependent vertical distributions of atmospheric temperature and static stability were determine...
The Mars infrared thermal mapper (IRTM) will be carried on the scan platform of the orbiter of the V...
Focuses on identification of critical gaps. The two most critical gaps are in coordinated end-to-end...
The design, development and testing of the infrared interferometer spectrometer is reported with emp...
Mars surface and atmosphere characteristics from thermal emission spectrum measurement by infrared i...
Preliminary 10- and 20-μm brightness temperatures of Mars are presented. More than 35% of the Martia...
The Mariner 9 infrared spectroscopy experiment has provided good quality spectra of many areas of Ma...
The reduced data of the Mariner 6 and 7 Infrared Radiometer Experiments are presented, along with a ...
The infrared radiometer is designed to provide brightness temperatures of the surface of Mars by mea...
The Mariner 6/7 Infrared Spectrometer (IRS) experiment data from the 1969 Mars flyby encounters repr...
After a schematic representation of the IRIS experiment, objectives of the program are outlined. Spe...
Calibrated infrared emission spectra of earth and atmosphere using high resolution interferometer sp...
IRIS - infrared interferometer spectrometer measurements of atmosphere vertical structure - humidity...
The science objectives, development history, functional description, and testing of the Mariner Venu...
Thirteen spectra of Mars, in the 7.5 to 12.8 micron wavelength were obtained on 7 Dec. 1990 from the...
Time dependent vertical distributions of atmospheric temperature and static stability were determine...
The Mars infrared thermal mapper (IRTM) will be carried on the scan platform of the orbiter of the V...
Focuses on identification of critical gaps. The two most critical gaps are in coordinated end-to-end...
The design, development and testing of the infrared interferometer spectrometer is reported with emp...
Mars surface and atmosphere characteristics from thermal emission spectrum measurement by infrared i...
Preliminary 10- and 20-μm brightness temperatures of Mars are presented. More than 35% of the Martia...
The Mariner 9 infrared spectroscopy experiment has provided good quality spectra of many areas of Ma...
The reduced data of the Mariner 6 and 7 Infrared Radiometer Experiments are presented, along with a ...
The infrared radiometer is designed to provide brightness temperatures of the surface of Mars by mea...
The Mariner 6/7 Infrared Spectrometer (IRS) experiment data from the 1969 Mars flyby encounters repr...
After a schematic representation of the IRIS experiment, objectives of the program are outlined. Spe...
Calibrated infrared emission spectra of earth and atmosphere using high resolution interferometer sp...
IRIS - infrared interferometer spectrometer measurements of atmosphere vertical structure - humidity...
The science objectives, development history, functional description, and testing of the Mariner Venu...
Thirteen spectra of Mars, in the 7.5 to 12.8 micron wavelength were obtained on 7 Dec. 1990 from the...
Time dependent vertical distributions of atmospheric temperature and static stability were determine...
The Mars infrared thermal mapper (IRTM) will be carried on the scan platform of the orbiter of the V...
Focuses on identification of critical gaps. The two most critical gaps are in coordinated end-to-end...