Measurements of stratospheric OH at 308 nm with the sun as light source using a Fourier transform spectrometer

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 3106, Issue , 1997, Pages 17-22

  Notholt, J ^a   Schutt H ^a   Keens, A ^a  

^a ALFRED WEGENER INSTITUTE FOR POLAR AND MARINE RESEARCH   (Germany)

Author keywords

Doppler shift; FTUV; Interferometer; OH radical; Signal to Noise Ratio; Solar absorption; Stratospheric trace gases

Indexed keywords

DOPPLER EFFECT; FOURIER TRANSFORM INFRARED SPECTROSCOPY; SIGNAL TO NOISE RATIO; SOLAR RADIATION; SUN;

FOURIER TRANSFORM SPECTROMETERS (FTS);

UPPER ATMOSPHERE;

EID: 0031310428     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.274721     Document Type: Conference Paper

References (10)

1. Visible spectroscopy at McMurdo station, Antarctica 2. Observations of OCIO
2. 2
3. Stratospheric trace gas measurements in the near UV and visible spectral range with the sun as light source using a Fourier transform spectrometer
4. 3 in the Arctic
5. Spectroscopic measurements of the vertical column abundance of hydroxyl (OH) in the earth's atmosphere
6. OH pepsios
7. Doppler detection of hydroxyl column abundance in the middle atmosphere
8. Vertical column abundance of atmospheric hydroxyl from 26°, 40°, and 65°N