Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/79731
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Type: Journal article
Title: The effect of recombination and attachment on meteor radar diffusion coefficient profiles
Author: Lee, C.
Younger, J.
Reid, I.
Kim, Y.
Kim, J.
Citation: Journal of Geophysical Research: Atmospheres, 2013; 118(7):3037-3043
Publisher: American Geophysical Union
Issue Date: 2013
ISSN: 2169-897X
2169-8996
Statement of
Responsibility: 
C. S. Lee, J. P. Younger, I. M. Reid, Y. H. Kim, and J. -H. Kim
Abstract: <jats:p>Estimates of the ambipolar diffusion coefficient producedusing meteor radar echo decay times display an increasing trend below 80–85 km, which is inconsistent with a diffusion‐only theory of the evolution of meteor trails. Data from the 33 MHz meteor radar at King Sejong Station, Antarctica, have been compared with observations from the Aura Earth Observing System Microwave Limb Sounder satellite instrument. It has been found that the height at which the diffusion coefficient gradient reverses follows the height of a constant neutral atmospheric density surface. Numerical simulations of meteor trail diffusion including dissociative recombination with atmospheric ions and three‐body attachment of free electrons to neutral molecules indicate that three‐body attachment is responsible for the distortion of meteor radar diffusion coefficient profiles at heights below 90 km, including the gradient reversal below 80–85 km. Further investigation has revealed that meteor trails with low initial electron line density produce decay times more consistent with a diffusion‐only model of meteor trail evolution.</jats:p>
Keywords: meteors
radar
diffusion
recombination
Rights: ©2013. American Geophysical Union. All Rights Reserved.
DOI: 10.1002/jgrd.50315
Grant ID: http://purl.org/au-research/grants/arc/DP1096901
http://purl.org/au-research/grants/arc/DP1096901
Published version: http://dx.doi.org/10.1002/jgrd.50315
Appears in Collections:Aurora harvest 4
Chemistry and Physics publications

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