Published November 21, 2017
| Submitted + Published
Journal Article
Open
Ozone measurements with meteors: a revisit
- Creators
-
Ye, Quan-Zhi
- Han, Summer Xia
Chicago
Abstract
Understanding the role of ozone in the mesosphere/lower thermosphere (MLT) region is essential for understanding the atmospheric processes in the upper atmosphere. Earlier studies have shown that it is possible to use overdense meteor trails to measure ozone concentration in the meteor region. Here, we revisit this topic by comparing a compilation of radar observations to satellite measurements. We observe a modest agreement between the values derived from these two methods, which confirm the usefulness of the meteor trail technique for measuring ozone content at certain heights in the MLT region. Future simultaneous measurements will help quantifying the performance of this technique.
Additional Information
© 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2017 July 19; Received 2017 July 6; in original form 2017 April 7; Published: 21 July 2017. We thank several anonymous referees for their comments, as well as Peter Brown, Chen Hai-Sheng, Wang Hong-Lei and Jia Shi-Guo for the discussion. We also thank the SABER team for their work in preparing the SABER data set (available through http://saber.gats-inc.com/index.php) and making it readily available.Attached Files
Published - stx1851.pdf
Submitted - 1707.09594.pdf
Files
stx1851.pdf
Files
(776.4 kB)
Name | Size | Download all |
---|---|---|
md5:852dc2d8efa7c884d4028068a109baa9
|
367.7 kB | Preview Download |
md5:1759af8658e5b0e9449b3318f87227d3
|
408.6 kB | Preview Download |
Additional details
- Eprint ID
- 83286
- Resolver ID
- CaltechAUTHORS:20171117-090913021
- Created
-
2017-11-20Created from EPrint's datestamp field
- Updated
-
2021-11-15Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)