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An airborne UV and visible spectrometer for DOAS and radiometric measurements

Contributo in Atti di convegno
Data di Pubblicazione:
1999
Abstract:
A UV/Vis spectrometer (named GASCOD) for Differential Optical Absorption Spectroscopy (DOAS) has been developed at ISAO Institute and deployed for ground based measurements of stratospheric trace gases for several years at mid-latitudes and the Antarctic region. An airborne version, called GASCOD/A has been installed on board a M55-Geophysica airplane, a stratospheric research platform, capable of flying at an altitude of up to 20 Km. After a test campaign in Italy, the GASCOD/A performed successfully during the Airborne Polar Experiment in the winter 95/96. More recently, the instrument was upgraded to achieve higher sensitivity and reliability. Two additional radiometric channels were added. The input optics can turn in order to collect solar radiation from five different channels: one for detection of the zenith scattered radiation through the roof window (for DOAS measurement), two for direct and diffused radiation through two lateral windows and two for radiometric measurements through two 2 pi optical heads mounted on the upper and bottom part of the aircraft and linked to the instrument by means of optical guides. The radiometric channels give us the possibility of calculating the photodissociation rate coefficients (J-values) of photochemical reactions involving ozone and nitrogen dioxides. The mechanical and optical layout of the instrument are presented and discussed, as well as laboratory tests and preliminary results obtained during flights onboard the M55-Geophysica.
Tipologia CRIS:
04.01 Contributo in Atti di convegno
Elenco autori:
Bortoli, Daniele; Petritoli, Andrea; Kostadinov, Ivan; Ravegnani, Fabrizio; Giovanelli, Giorgio
Autori di Ateneo:
RAVEGNANI FABRIZIO
Link alla scheda completa:
https://iris.cnr.it/handle/20.500.14243/15898
Titolo del libro:
OPTICAL SPECTROSCOPIC TECHNIQUES AND INSTRUMENTATION FOR ATMOSPHERIC AND SPACE RESEARCH III
Pubblicato in:
PROCEEDINGS OF SPIE, THE INTERNATIONAL SOCIETY FOR OPTICAL ENGINEERING
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