An account is given of progress during the period 8/l/96-7/31/97 on work on (a) cross section measurements of O2 S-R using a Fourier transform spectrometer (FTS) at the Photon Factory in Japan; (b) the determination of the predissociation linewidths of the Schumann-Runge bands (S-R) of 02; (c) cross section measurements of 02 Herzberg bands using a Fourier transform spectrometer (FTS) at Imperial College; and (d) cross section measurements of H2O in the wavelength region 120-188 nm. The experimental investigations are effected at high resolution with a 6.65 m scanning spectrometer and with the Fourier transform spectrometer. Below 175 nm, synchrotron radiation is most suitable for cross section measurements in combination with spectrometers...
Results are presented of a comparative study in which three distinct high-resolution experimental te...
Author Institution: Harvard Smithsonian Center for Astrophysics; Imperial College of Science, Techno...
Radiation in the wavelength interval 150-350 nm initiates chemical reactions in the lower mesosphere...
An account is given of progress during the six-month period 1 Nov. 1992 to 30 Apr. 1993 on work on (...
Progress is given on work on: cross section measurements in the transmission window regions of the S...
An account is given of progress during the six month period 1/11/84 to 4/30/85 in work on: (1) rovib...
Results are presented of a comparative study in which three distinct high-resolution experimental te...
Optical measurements of trace species in the atmosphere require precise, accurate spectroscopic data...
State-of-the-art models of the vacuum ultraviolet (VUV) absorbing properties of the atmosphere call ...
A compact, high-resolution Fourier-transform spectrometer for atmospheric near-ultraviolet spectrosc...
The β(6,0) and the γ(3,0) bands of NO near 198 nm were analyzed using the VUV FT spectrometer with s...
A high resolution spectrometer which incorporates a narrow line width tunable dye laser was used to ...
The absorption of ultraviolet solar radiation is of prime importance for the study of planetary atmo...
This research task consists of operating a facility for making spectroscopic observations in support...
A windowless apparatus was constructed and used to measure the photoabsorption and fluorescence cros...
Results are presented of a comparative study in which three distinct high-resolution experimental te...
Author Institution: Harvard Smithsonian Center for Astrophysics; Imperial College of Science, Techno...
Radiation in the wavelength interval 150-350 nm initiates chemical reactions in the lower mesosphere...
An account is given of progress during the six-month period 1 Nov. 1992 to 30 Apr. 1993 on work on (...
Progress is given on work on: cross section measurements in the transmission window regions of the S...
An account is given of progress during the six month period 1/11/84 to 4/30/85 in work on: (1) rovib...
Results are presented of a comparative study in which three distinct high-resolution experimental te...
Optical measurements of trace species in the atmosphere require precise, accurate spectroscopic data...
State-of-the-art models of the vacuum ultraviolet (VUV) absorbing properties of the atmosphere call ...
A compact, high-resolution Fourier-transform spectrometer for atmospheric near-ultraviolet spectrosc...
The β(6,0) and the γ(3,0) bands of NO near 198 nm were analyzed using the VUV FT spectrometer with s...
A high resolution spectrometer which incorporates a narrow line width tunable dye laser was used to ...
The absorption of ultraviolet solar radiation is of prime importance for the study of planetary atmo...
This research task consists of operating a facility for making spectroscopic observations in support...
A windowless apparatus was constructed and used to measure the photoabsorption and fluorescence cros...
Results are presented of a comparative study in which three distinct high-resolution experimental te...
Author Institution: Harvard Smithsonian Center for Astrophysics; Imperial College of Science, Techno...
Radiation in the wavelength interval 150-350 nm initiates chemical reactions in the lower mesosphere...