The thermospheric-ionospheric storm of Dec 8, 1982: Model predictions and observations

G. W. Prölss; S. Werner; M. V. Codrescu; T. J. Fuller-Rowell; A. G. Burns; T. L. Killeen

doi:10.1016/S0273-1177(97)01111-3

The thermospheric-ionospheric storm of Dec 8, 1982: Model predictions and observations

G. W. Prölss, S. Werner, M. V. Codrescu, T. J. Fuller-Rowell, A. G. Burns, T. L. Killeen

Research output: Contribution to journal › Article › peer-review

Abstract

The Thermosphere-Ionosphere General Circulation Model (Roble et al., 1988) and the Coupled Thermosphere-Ionosphere Model (Fuller-Rowell et al., 1987) are used to simulate thermospheric-ionospheric behaviour during the magnetic storm of December 8, 1982. A comparison of these predictions with observations indicates that both models overestimate the daytime increase of the O/N ₂ ratio and the associated positive ionospheric storm effects. Also there is no indication of a large enhancement in the O/N ₂ ratio in the evening sector of the winter hemisphere.

Original language	English (US)
Pages (from-to)	123-128
Number of pages	6
Journal	Advances in Space Research
Volume	22
Issue number	1
DOIs	https://doi.org/10.1016/S0273-1177(97)01111-3
State	Published - 1998

ASJC Scopus subject areas

Aerospace Engineering
Astronomy and Astrophysics
Geophysics
Atmospheric Science
Space and Planetary Science
Earth and Planetary Sciences(all)

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@article{7ec894cba1d34045ad9963b8fde0f54d,

title = "The thermospheric-ionospheric storm of Dec 8, 1982: Model predictions and observations",

abstract = " The Thermosphere-Ionosphere General Circulation Model (Roble et al., 1988) and the Coupled Thermosphere-Ionosphere Model (Fuller-Rowell et al., 1987) are used to simulate thermospheric-ionospheric behaviour during the magnetic storm of December 8, 1982. A comparison of these predictions with observations indicates that both models overestimate the daytime increase of the O/N 2 ratio and the associated positive ionospheric storm effects. Also there is no indication of a large enhancement in the O/N 2 ratio in the evening sector of the winter hemisphere.",

author = "Pr{\"o}lss, {G. W.} and S. Werner and Codrescu, {M. V.} and Fuller-Rowell, {T. J.} and Burns, {A. G.} and Killeen, {T. L.}",

note = "Funding Information: The DE 2 data used in this study were kindly provided by George Carignan. The ionosonde data were obtained with the help of World Data Centers A and Cl. This work was supported by the Deutsche Forschungsgemeinschafutn der grant Pr 276/8-l.",

year = "1998",

doi = "10.1016/S0273-1177(97)01111-3",

language = "English (US)",

volume = "22",

pages = "123--128",

journal = "Advances in Space Research",

issn = "0273-1177",

publisher = "Elsevier Limited",

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TY - JOUR

T1 - The thermospheric-ionospheric storm of Dec 8, 1982

T2 - Model predictions and observations

AU - Prölss, G. W.

AU - Werner, S.

AU - Codrescu, M. V.

AU - Fuller-Rowell, T. J.

AU - Burns, A. G.

AU - Killeen, T. L.

N1 - Funding Information: The DE 2 data used in this study were kindly provided by George Carignan. The ionosonde data were obtained with the help of World Data Centers A and Cl. This work was supported by the Deutsche Forschungsgemeinschafutn der grant Pr 276/8-l.

PY - 1998

Y1 - 1998

N2 - The Thermosphere-Ionosphere General Circulation Model (Roble et al., 1988) and the Coupled Thermosphere-Ionosphere Model (Fuller-Rowell et al., 1987) are used to simulate thermospheric-ionospheric behaviour during the magnetic storm of December 8, 1982. A comparison of these predictions with observations indicates that both models overestimate the daytime increase of the O/N 2 ratio and the associated positive ionospheric storm effects. Also there is no indication of a large enhancement in the O/N 2 ratio in the evening sector of the winter hemisphere.

AB - The Thermosphere-Ionosphere General Circulation Model (Roble et al., 1988) and the Coupled Thermosphere-Ionosphere Model (Fuller-Rowell et al., 1987) are used to simulate thermospheric-ionospheric behaviour during the magnetic storm of December 8, 1982. A comparison of these predictions with observations indicates that both models overestimate the daytime increase of the O/N 2 ratio and the associated positive ionospheric storm effects. Also there is no indication of a large enhancement in the O/N 2 ratio in the evening sector of the winter hemisphere.

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