On the temperature dependence of possible S8 infrared bands in planetary atmospheres

Details On the temperature dependence of possible S8 infrared bands in planetary atmospheres On the temperature dependence of possible S8 infrared bands in planetary atmospheres

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977icar...30..231k&link_type=abstract

Icarus, vol. 30, Jan. 1977, p. 231-233.

Other

1

Atmospheric Temperature, Infrared Spectra, Jupiter Atmosphere, Sulfur, Temperature Measurement, Absorption Spectra, Infrared Spectrometers, Spectrum Analysis

Scientific paper

The temperature dependence between 77 and 333 K of the infrared spectrum of cyclic S8 in the Jupiter atmosphere has been measured. It was found that the 23-micron Jovian feature (identified by Houck et al., 1975), if real, cannot be attributed to cyclic S8. Other features of S8, however, such as the band with a room-temperature central frequency of 835/cm may prove to be useful temperature calibrators in planetary or satellite spectra.

Affiliated with

Also associated with

No associations

Rating

On the temperature dependence of possible S8 infrared bands in planetary atmospheres does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with On the temperature dependence of possible S8 infrared bands in planetary atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the temperature dependence of possible S8 infrared bands in planetary atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-952447