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Proceedings Paper

Development of a geomagnetic storm correction to the international reference ionosphere model E-region electron densities using TIMED/SABER observations
Author(s): C. J. Mertens; X. Xu; J. Fernandez; D. Bilitza; J. M. Russell; M. G. Mlynczak
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Paper Abstract

Auroral infrared emission observed from the TIMED/SABER broadband 4.3 um channel is used to develop an empirical geomagnetic storm correction to the International Reference Ionosphere (IRI) E-region electron densities. The observation-based proxy used to develop the storm model is SABER-derived NO+(v) 4.3 um volume emission rates (VER). A correction factor is defined as the ratio of storm-time NO+(v) 4.3 um VER to a quiet-time climatological averaged NO+(v) 4.3 um VER, which is linearly fit to available geomagnetic activity indices. The initial version of the E-region storm model, called STORM-E, is most applicable within the auroral oval region. The STORM-E predictions of E-region electron densities are compared to incoherent scatter radar electron density measurements during the Halloween 2003 storm events. Future STORM-E updates will extend the model outside the auroral oval.

Paper Details

Date Published: 29 September 2009
PDF: 12 pages
Proc. SPIE 7475, Remote Sensing of Clouds and the Atmosphere XIV, 747508 (29 September 2009); doi: 10.1117/12.829976
Show Author Affiliations
C. J. Mertens, NASA Langley Research Ctr. (United States)
X. Xu, Science Systems and Applications, Inc. (United States)
J. Fernandez, NASA Langley Research Ctr. (United States)
D. Bilitza, George Mason Univ. (United States)
J. M. Russell, Hampton Univ. (United States)
M. G. Mlynczak, NASA Langley Research Ctr. (United States)


Published in SPIE Proceedings Vol. 7475:
Remote Sensing of Clouds and the Atmosphere XIV
Richard H. Picard; Klaus Schäfer; Adolfo Comeron; Evgueni I. Kassianov; Christopher J. Mertens, Editor(s)

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