In this work we present a methodology to calculate the temperature in the upper mesosphere using a spectral OH (6-2) airglow temperature imager. The temperature imager system consists of a CCD camera and an optical head (including an interferometer filter, Fresnel lens and objective lens) which was developed by Airglow group of INPE in São José dos Campos, Brazil. The instrument calibration was performed at National Institute of Polar Research, Japan, using a 2 m diameter integrating sphere. The airglow test observations were carried out at Cachoeira Paulista Observatory (22.7ºS), Brazil, from March to May 2005, and the results were compared to that obtained by a tilting-filter zenith photometer (MC2) at the same place. Some results are pre...
Ground-based observations of OH (6, 2) Meinel band nightglow were carried out at Ranchi (23.3° N, 8...
The Institute for Atmospheric and Environmental Research at the University of Wuppertal and the Inst...
Spectra of the O2(a1 Δg) airglow emission band at 1.27 μm have been recorded during twilight at May...
The physics of the hydroxyl (OH) layer located in the Mesosphere and Lower Thermosphere (MLT) has be...
We have performed ground-based airglow observations with a tilting filter spectrometer to determine ...
The airglow OH (8-3) and (6-2) band rotational temperatures were measured and compared using two sca...
Ground based measurements of the hydroxyl airglow started in Trondheim (63.4 N, 10.4 E) 20. November...
The research studied the comparison of the night air temperatures and the atomic oxygen airglow inte...
At nighttime the strongest source of radiation is the hydroxyl night glow. By measuringthe different...
The Cariri Airglow Observatory has been in operation since November, 1997. This observatory has a mu...
We report calibration of the optical instruments of the Optical Mesosphere Thermosphere Imagers (OMT...
The Cariri Airglow Observatory has been in operation since November, 1997. This observatory has a mu...
A method has been developed for the retrieval of mesospheric temperatures in the 65–90 km altitude r...
Abstract Fabry–Perot interferometer (FPI) is an instrument that can measure the temperature and wind...
OH airglow observed by the ISUAL (Imager of Sprites and Upper Atmospheric Lightning) instrument on b...
Ground-based observations of OH (6, 2) Meinel band nightglow were carried out at Ranchi (23.3° N, 8...
The Institute for Atmospheric and Environmental Research at the University of Wuppertal and the Inst...
Spectra of the O2(a1 Δg) airglow emission band at 1.27 μm have been recorded during twilight at May...
The physics of the hydroxyl (OH) layer located in the Mesosphere and Lower Thermosphere (MLT) has be...
We have performed ground-based airglow observations with a tilting filter spectrometer to determine ...
The airglow OH (8-3) and (6-2) band rotational temperatures were measured and compared using two sca...
Ground based measurements of the hydroxyl airglow started in Trondheim (63.4 N, 10.4 E) 20. November...
The research studied the comparison of the night air temperatures and the atomic oxygen airglow inte...
At nighttime the strongest source of radiation is the hydroxyl night glow. By measuringthe different...
The Cariri Airglow Observatory has been in operation since November, 1997. This observatory has a mu...
We report calibration of the optical instruments of the Optical Mesosphere Thermosphere Imagers (OMT...
The Cariri Airglow Observatory has been in operation since November, 1997. This observatory has a mu...
A method has been developed for the retrieval of mesospheric temperatures in the 65–90 km altitude r...
Abstract Fabry–Perot interferometer (FPI) is an instrument that can measure the temperature and wind...
OH airglow observed by the ISUAL (Imager of Sprites and Upper Atmospheric Lightning) instrument on b...
Ground-based observations of OH (6, 2) Meinel band nightglow were carried out at Ranchi (23.3° N, 8...
The Institute for Atmospheric and Environmental Research at the University of Wuppertal and the Inst...
Spectra of the O2(a1 Δg) airglow emission band at 1.27 μm have been recorded during twilight at May...