FTS Measurements of Submillimeter-Wave Atmospheric Opacity at Pampa la Bola

Details FTS Measurements of Submillimeter-Wave Atmospheric Opacity at Pampa la Bola FTS Measurements of Submillimeter-Wave Atmospheric Opacity at Pampa la Bola

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pasj...50..359m&link_type=abstract

Publications of the Astronomical Society of Japan, v.50, p.359-366.

Astronomy and Astrophysics

Astronomy

18

Earth: Atmosphere, Instruments, Spectroscopy, Submillimeter-Wave: Opacities

Scientific paper

The first measurements of submillimeter-wave atmospheric opacity spectra at the Pampa la Bola site (Northern Chile, Atacama, 4800 m altitude) have been performed during the winter season using a Fourier transform spectrometer (FTS). Atmospheric emission spectra, as a function of airmass, were measured under various weather conditions. Atmospheric opacity was evaluated from sky temperature at the zenith as well as from tipping measurements, which are independent measures but give consistent results. Correlation diagrams between 220 GHz and 345 GHz, 410 GHz, 492 GHz, 675 GHz, 691 GHz, 809 GHz, 875 GHz are shown. Correlations between millimeter-wave and submillimeter-wave opacities get worse when 220 GHz opacity is larger than 0.1. Deviations from the opacity correlation at each frequency show good correlations themselves, but have different relative variations at each frequency. This indicates that atmospheric transparency cannot be characterized only by millimeter-wave opacity, but requires simultaneous opacity measurements at millimeter and submillimeter-wavelengths.

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