Atmospheric temperature profiles and ray paths from occultation spectra

Details Atmospheric temperature profiles and ray paths from occultation spectra Atmospheric temperature profiles and ray paths from occultation spectra

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apopt..24.1309h&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 24, May 1, 1985, p. 1309-1312.

Computer Science

Sound

4

Absorption Spectra, Atmospheric Temperature, Optical Paths, Remote Sensing, Solar Spectra, Temperature Profiles, Atmospheric Sounding, Carbon Dioxide, Molecular Absorption, Signal To Noise Ratios, Stellar Occultation, Temperature Measurement

Scientific paper

Simulated equivalent width data of weak lines in occultation spectra have been analyzed to retrieve both the atmospheric temperature profile and the tangent heights of the rays. The SNR of these widths varied from 5 to 100. The mixing ratio of the absorbing gas and sea level pressure were assumed but not the satellite position. Temperature and tangent heights with accuracies of 1 K and 0.25 km, respectively, were determined from lines with temperature-dependent and temperature-independent intensities.

Affiliated with

Also associated with

No associations

Rating

Atmospheric temperature profiles and ray paths from occultation spectra 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 Atmospheric temperature profiles and ray paths from occultation spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Atmospheric temperature profiles and ray paths from occultation spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1631527