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Effects of a mid-latitude solar eclipse on the thermosphere and ionosphere: a modelling study

Müller-Wodarg, I. C. F., Aylward, A. D. and Lockwood, M. (1998) Effects of a mid-latitude solar eclipse on the thermosphere and ionosphere: a modelling study. Geophysical Research Letters, 25 (20). pp. 3787-3790. ISSN 0094-8276

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To link to this item DOI: 10.1029/1998GL900045

Abstract/Summary

A modelling study is presented which investigates in-situ generated changes of the thermosphere and ionosphere during a solar eclipse. Neutral temperatures are expected to drop by up to 40 degrees K at 240 km height in the totality footprint, with neutral winds of up to 26 m/s responding to the change of pressure. Both temperatures and winds are found to respond with a time lag of 30 min after the passing of the Moon's shadow. A gravity wave is generated in the neutral atmosphere and propagates into the opposite hemisphere at around 300 m/s. The combined effects of thermal cooling and downwelling lead to an overall increase in [O], while [N(2)] initially rises and then for several hours after the eclipse is below the "steady state" level. An enhancement of [NmF2] is found and explained by the atmosphere's contraction during, and the reduced [O]/[N(2)] ratio after the eclipse.

Item Type:Article
Refereed:Yes
Divisions:No Reading authors. Back catalogue items
Faculty of Science > School of Mathematical, Physical and Computational Sciences > Department of Meteorology
ID Code:38757
Additional Information:First published online 2012
Publisher:American Geophysical Union

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