The infrared spectrum of Venus in the spectral range 1.6 to 2.8 was measured by means of the spectrometers aboard 'Venera-9' and 'Venera-10' orbital spacecrafts. Approximately 20 series of measurements were made near the pericenter of the orbit, each of which contains 150 spectra for each path intersecting the planet from the terminator to the limb. Phase angles lie within the limits from 60 to 120 deg
Interpretation of mineralogy using VNIR spectroscopy data from orbiters requires spectral libraries ...
Vénus, deuxième planète du système solaire, souvent appelée sœur de la Terre, car présentant des car...
The Pioneer Venus Orbiter Infrared Radiometer and Venera 15 Fourier Transform Spectrometer observati...
The spectra of the daytime sky of Venus were recorded on the Venera-11 and Venera-12 descent vehicle...
The thermal emission of Venus was recorded during the winter of 1970-1971, and in 1973 using the 2.7...
Interpretation of the Fourier-spectrometer experiment gave new knowledge about the structure and var...
Several new infrared absorptions were found in carbon dioxide. All are normally forbidden, and were ...
Experimental measurements by ultraviolet photometers aboard Venera-9 and -10 are presented, discusse...
International audienceSolar Occultation at Infrared (SOIR), which is a part of the Spectroscopy for ...
Ground-based near-infrared observations of the Venus night side reveal anomalous bright features at ...
The authors wish to thank Teclinical Operations Incorporated, particularly Mr. Richard Wilkins, for ...
The development of high spectral resolution and highly sensitive long infrared wavelength instrument...
Venera and Mariner spacecraft and ground based radio astronomy and spectroscopic observations of the...
Thirty well-exposed photographic plates showing the spectrum of the carbon dioxide band at 8689A in ...
A theoretical calculation was made of the CO2 infrared spectra of Earth and Venus atmospheres. The c...
Interpretation of mineralogy using VNIR spectroscopy data from orbiters requires spectral libraries ...
Vénus, deuxième planète du système solaire, souvent appelée sœur de la Terre, car présentant des car...
The Pioneer Venus Orbiter Infrared Radiometer and Venera 15 Fourier Transform Spectrometer observati...
The spectra of the daytime sky of Venus were recorded on the Venera-11 and Venera-12 descent vehicle...
The thermal emission of Venus was recorded during the winter of 1970-1971, and in 1973 using the 2.7...
Interpretation of the Fourier-spectrometer experiment gave new knowledge about the structure and var...
Several new infrared absorptions were found in carbon dioxide. All are normally forbidden, and were ...
Experimental measurements by ultraviolet photometers aboard Venera-9 and -10 are presented, discusse...
International audienceSolar Occultation at Infrared (SOIR), which is a part of the Spectroscopy for ...
Ground-based near-infrared observations of the Venus night side reveal anomalous bright features at ...
The authors wish to thank Teclinical Operations Incorporated, particularly Mr. Richard Wilkins, for ...
The development of high spectral resolution and highly sensitive long infrared wavelength instrument...
Venera and Mariner spacecraft and ground based radio astronomy and spectroscopic observations of the...
Thirty well-exposed photographic plates showing the spectrum of the carbon dioxide band at 8689A in ...
A theoretical calculation was made of the CO2 infrared spectra of Earth and Venus atmospheres. The c...
Interpretation of mineralogy using VNIR spectroscopy data from orbiters requires spectral libraries ...
Vénus, deuxième planète du système solaire, souvent appelée sœur de la Terre, car présentant des car...
The Pioneer Venus Orbiter Infrared Radiometer and Venera 15 Fourier Transform Spectrometer observati...