Observation of atmospheric minor constituents by FTIR at Syowa Station, Antarctica

• Main Authors: Makino, Y., Muramatsu, H., Kawaguchi, S., Yamanouchi, T., Tanaka, M., Ogawa, T.
• Format: Other/Unknown Material
• Language: unknown
• Published: 1985
• Subjects: 46; Antarctic; The Antarctic; Syowa Station; Antarc*; Antarctica
• Online Access: http://ntrs.nasa.gov/search.jsp?R=19860018346

As a part of the Antarctic MAP activity, a ground-based spectroscopic observation of atmospheric infrared transmission was started at Syowa station (69 deg 00'S, 39 deg 35'E) in March 24, 1983. Observations of sunlight as a radiation source were made with a Fourier transform infrared spectrometer having a maximum path difference of 80 mm and an apodized FWHM resolution of approx. 0.12/cm. In routine operation through the year, the resolution of approx. 0.8/cm was applied for economy of data-processing time. The 408 spectra for 72 days were obtained in about 10 months until January 23, 1984. From the absorption features revealed in the spectra over the wave number range of 500 to 7500/cm, a preliminary estimate of N202 gamma sub 1 band absorption was attempted. An apparent transmittance was defined at the wave number 2576/cm, where the absorption by N20 molecules affected the observed intensity strongly. A ray-tracing technique and a line-by-line calculation with a model atmosphere and the AFGL atmospheric absorption line parameters compilation were applied to the calculation of the synthetic spectra.