Add to ORKGThe predicted infrared brightness temperature of Mars using the 1976 model of Wright is tabulated here for the period 1983 to 2103. This model was developed for far-infrared calibration, and is still being used for JCMT calibration
This is a dataset of meteorological variables for the atmosphere of Mars, obtained by assimilating m...
IBM 7074 computer program for computation of insolation tables for surface of Mar
The Cameron bands and the UV doublet are two of the most prominent emission systems in the UV in Mar...
Preliminary 10- and 20-μm brightness temperatures of Mars are presented. More than 35% of the Martia...
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...
New measurements of the microwave temperature of Mars are reported. The brightness temperatures meas...
New measurements of the microwave temperature of Mars are reported. The brightness temperatures meas...
Thirteen spectra of Mars, in the 7.5 to 12.8 micron wavelength were obtained on 7 Dec. 1990 from the...
During the period October 1997 to September 1999 we obtained and analyzed over 100 millimeter-wave o...
The Mariner 6/7 Infrared Spectrometer (IRS) experiment data from the 1969 Mars flyby encounters repr...
The thermal interia of the surface of Mars varies spatially by a factor of eight. This is attributab...
A series of far infrared (FIR) spectra of Mars between 43 and 196 μm was taken with the Long Wavelen...
Observations of Mars at wavelengths of 2 and 6cm were made using the VLA in its A configuration. Two...
The Thermal Emission Imaging System (THEMIS) on Mars Odyssey has produced infrared to visible wavele...
This is a dataset of meteorological variables for the atmosphere of Mars, obtained by assimilating m...
IBM 7074 computer program for computation of insolation tables for surface of Mar
The Cameron bands and the UV doublet are two of the most prominent emission systems in the UV in Mar...
Preliminary 10- and 20-μm brightness temperatures of Mars are presented. More than 35% of the Martia...
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...
New measurements of the microwave temperature of Mars are reported. The brightness temperatures meas...
New measurements of the microwave temperature of Mars are reported. The brightness temperatures meas...
Thirteen spectra of Mars, in the 7.5 to 12.8 micron wavelength were obtained on 7 Dec. 1990 from the...
During the period October 1997 to September 1999 we obtained and analyzed over 100 millimeter-wave o...
The Mariner 6/7 Infrared Spectrometer (IRS) experiment data from the 1969 Mars flyby encounters repr...
The thermal interia of the surface of Mars varies spatially by a factor of eight. This is attributab...
A series of far infrared (FIR) spectra of Mars between 43 and 196 μm was taken with the Long Wavelen...
Observations of Mars at wavelengths of 2 and 6cm were made using the VLA in its A configuration. Two...
The Thermal Emission Imaging System (THEMIS) on Mars Odyssey has produced infrared to visible wavele...
This is a dataset of meteorological variables for the atmosphere of Mars, obtained by assimilating m...
IBM 7074 computer program for computation of insolation tables for surface of Mar
The Cameron bands and the UV doublet are two of the most prominent emission systems in the UV in Mar...