Upper stratosphere negative ion composition measurements and inferred trace gas abundances

Computer Science – Sound

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

19

Atmospheric Composition, Atmospheric Sounding, Gas Composition, Negative Ions, Stratosphere, Trace Elements, Atmospheric Chemistry, Reaction Kinetics, Rocket Sounding

Scientific paper

In situ composition measurements of atmospheric negative ions were made at 40.8 km altitude using a balloon-borne mass spectrometer with large mass range and improved mass resolution. The data obtained show marked differences compared to previous data obtained mostly around or below 33 km. It appears that these differences are mostly due to a higher atmospheric temperature, a lower nitric acid vapor abundance and a larger HSO3-vapor abundance prevailing at the higher altitude. A particularly striking feature is the relatively large fractional abundance of HSO3-containing cluster ions. Another interesting result is that nitric acid vapor abundances can be inferred from the negative ion composition data with better accuracy than is possible for lower altitudes. The reason is that collisional ion dissociation occurring during ion sampling is less disturbing. The inferred nitric acid vapor abundance for 40.8 km altitude is consistent with current 2-dimensional model calculations.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Upper stratosphere negative ion composition measurements and inferred trace gas abundances 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 Upper stratosphere negative ion composition measurements and inferred trace gas abundances, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Upper stratosphere negative ion composition measurements and inferred trace gas abundances will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1859075

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.