Model results for the ionospheric lower transition height over mid-latitude
Theoretical calculations of the ionospheric lower transition height (LTH), a level of equal O<sup>+</sup> and molecular ion densities, were performed and compared with empirical models by Zhang et al. (1996). This paper represents a substantial extension of the prior work by...
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Copernicus Publications
2004-06-01
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Series: | Annales Geophysicae |
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doaj-1bf97c1585e34d329bc8ea5c5ec021d02020-11-25T00:39:14ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762004-06-01222037204510.5194/angeo-22-2037-2004Model results for the ionospheric lower transition height over mid-latitudeJ. Lei0J. Lei1L. Liu2W. Wan3S.-R. Zhang4Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, ChinaWuhan Ionospheric Observatory, Wuhan Institute of Physics and Mathematics, Chinese Academy of Sciences, Wuhan 430071, ChinaInstitute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, ChinaInstitute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, ChinaHaystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USATheoretical calculations of the ionospheric lower transition height (LTH), a level of equal O<sup>+</sup> and molecular ion densities, were performed and compared with empirical models by Zhang et al. (1996). This paper represents a substantial extension of the prior work by including the AE-C data of ion composition analysis and by detailed quantitative studies of the LTH simulation, and by creating a new LTH empirical model based on our simulations. Results show that: (1) the calculated LTH, in general, is lowest near 11-13LT and reaches the diurnal maximum after midnight (about 01~02LT). The local time asymmetry becomes more evident in summer, when the time of minimum shifts to 16LT. (2) The simulated LTH presents a dominant, semiannual variation during nighttime, and a pronounced annual variation during daytime. (3) The simulated LTH increases with solar activity at night and decreases by day, while the standard IRI option has an opposite tendency at night in summer and equinox. Therefore, the day-night difference of simulated LTH significantly increases with solar activity. (4) Both daytime and nighttime LTHs, tend to increase with the increasing geomagnetic activity <i>A<sub>p</sub></i> index, with a mean slope about 0.1455km per <i>A<sub>p</sub></i> unit. (5) The diurnal variation of LTH is found to be more than 20 km, which is much larger than the seasonal variation under F107=100 and <i>A<sub>p</sub></i>=10. Thus, the diurnal and solar activity variations of LTH are more pronounced than its seasonal and magnetic activity variations.https://www.ann-geophys.net/22/2037/2004/angeo-22-2037-2004.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
J. Lei J. Lei L. Liu W. Wan S.-R. Zhang |
spellingShingle |
J. Lei J. Lei L. Liu W. Wan S.-R. Zhang Model results for the ionospheric lower transition height over mid-latitude Annales Geophysicae |
author_facet |
J. Lei J. Lei L. Liu W. Wan S.-R. Zhang |
author_sort |
J. Lei |
title |
Model results for the ionospheric lower transition height over mid-latitude |
title_short |
Model results for the ionospheric lower transition height over mid-latitude |
title_full |
Model results for the ionospheric lower transition height over mid-latitude |
title_fullStr |
Model results for the ionospheric lower transition height over mid-latitude |
title_full_unstemmed |
Model results for the ionospheric lower transition height over mid-latitude |
title_sort |
model results for the ionospheric lower transition height over mid-latitude |
publisher |
Copernicus Publications |
series |
Annales Geophysicae |
issn |
0992-7689 1432-0576 |
publishDate |
2004-06-01 |
description |
Theoretical calculations of the ionospheric lower
transition height (LTH), a level of equal O<sup>+</sup> and molecular ion
densities, were performed and compared with empirical models by Zhang et
al. (1996). This paper represents a substantial extension of the prior work
by including the AE-C data of ion composition analysis and by detailed
quantitative studies of the LTH simulation, and by creating a new LTH empirical
model based on our simulations. Results show that: (1) the
calculated LTH, in general, is lowest near 11-13LT and reaches the diurnal
maximum after midnight (about 01~02LT). The local time asymmetry
becomes more evident in summer, when the time of minimum shifts to 16LT.
(2) The simulated LTH presents a dominant, semiannual variation
during nighttime, and a pronounced annual variation during daytime.
(3) The simulated LTH increases with solar activity at night and decreases
by day, while the standard IRI option has an opposite tendency at night in
summer and equinox. Therefore, the day-night difference of simulated LTH
significantly increases with solar activity. (4) Both daytime and
nighttime LTHs, tend to increase with the increasing geomagnetic activity <i>A<sub>p</sub></i>
index, with a mean slope about 0.1455km per <i>A<sub>p</sub></i> unit. (5) The
diurnal variation of LTH is found to be more than 20 km, which is much
larger than the seasonal variation under F107=100 and <i>A<sub>p</sub></i>=10. Thus, the
diurnal and solar activity variations of LTH are more pronounced than its
seasonal and magnetic activity variations. |
url |
https://www.ann-geophys.net/22/2037/2004/angeo-22-2037-2004.pdf |
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