Abstract
Meteor radars detect the ionized trails left by meteors in the mesosphere and lower thermosphere. The trails are advected with the winds at the heights where they form and so can be used as tracers of atmospheric motion. Meteor radars typically measure zonal and meridional winds with time and height resolutions of about 1â h and 3â km, respectively. The radars are often simple and robust, making them ideal for extended deployment at remote sites. They are well suited to studies of background winds, tides, and planetary waves. Recent advances offer the possibility of making statistical measurements of gravity wave fluxes.
Original language | English |
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Title of host publication | Encyclopedia of Atmospheric Sciences |
Publisher | Elsevier Academic Press Inc |
Pages | 438-443 |
Number of pages | 6 |
Edition | 2 |
ISBN (Electronic) | 9780123822260 |
ISBN (Print) | 9780123822253 |
DOIs | |
Publication status | E-pub ahead of print - 18 Sept 2014 |
Keywords
- Gravity waves
- Mesosphere
- Meteors
- Planetary waves
- Radar
- Tides
ASJC Scopus subject areas
- General Physics and Astronomy