Determination of the general ozone abundance from spectrophotometric UV observations of the Sun

Details Determination of the general ozone abundance from spectrophotometric UV observations of the Sun Determination of the general ozone abundance from spectrophotometric UV observations of the Sun

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnt...16..266b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 16, no. 3, p. 266-273

Other

Scientific paper

We describe a new version of the multiwave technique for determinating the total ozone content in Earth's atmosphere. The technique is based on the assumption that the aerosol attenuation depends arbitrarily on wavelength. It was used for the processing of solar spectrophotometric observations in the near-UV region (305-340 nm) in 1989 and 1998 at the High-Altitude Station Terskol of the Main Astronomical Observatory of the Academy of Sciences of Ukraine. The data processing showed that not only the total ozone content could be determined with the technique but a number of other trace gases as well including SO2, NO2, along with the spectral dependence of aerosol absorption.

Affiliated with

Also associated with

No associations

Rating

Determination of the general ozone abundance from spectrophotometric UV observations of the Sun 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 Determination of the general ozone abundance from spectrophotometric UV observations of the Sun, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Determination of the general ozone abundance from spectrophotometric UV observations of the Sun will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-740782