Muller-Wodarg, ICF;
Aylward, AD;
Lockwood, M;
(1998)
Effects of a mid-latitude solar eclipse on the thermosphere and ionosphere - A modelling study.
Geophysical Research Letters
, 25
(20)
3787 - 3790.
10.1029/1998GL900045.
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Abstract
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.
Type: | Article |
---|---|
Title: | Effects of a mid-latitude solar eclipse on the thermosphere and ionosphere - A modelling study |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1029/1998GL900045 |
Publisher version: | http://dx.doi.org/10.1029/1998GL900045 |
Language: | English |
Additional information: | Copyright 1998 by the American Geophysical Union |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/100139 |
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