Articles | Volume 36, issue 5
Regular paper
25 Sep 2018
Regular paper |  | 25 Sep 2018

Meteor echo height ceiling effect and mesospheric temperature estimation from meteor radar observations

Changsup Lee, Geonhwa Jee, Jeong-Han Kim, and In-Sun Song


Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to revisions (further review by editor and referees) (10 Jul 2018) by Huixin Liu
AR by Changsup Lee on behalf of the Authors (11 Jul 2018)  Author's response
ED: Referee Nomination & Report Request started (19 Jul 2018) by Huixin Liu
ED: Publish as is (04 Sep 2018) by Huixin Liu
Short summary
This study shows the width of the meteor height distribution (FWHM) is well correlated with the atmospheric pressure, not only experimentally but theoretically. From the correlation analysis, we found that the FWHM provides the best estimation of the temperature at the height layer below the meteor peak height by 2–3 km. We also proved a meteor echo height ceiling effect (MHC) is primarily controlled by the atmospheric conditions, and this enables the FWHM to estimate the temperature accurately.