GUVI Biblio

Impact of Eddy Diffusivity on Seasonal Variations of the Thermosphere

Qian, Liying; Solomon, Stanley; Kane, Timothy;

Published by:       Published on:

YEAR: 2008     DOI:

Variations of Auroral Electron Precipitation Measured by TIMED/GUVI

Luan, X; Wang, W; Burns, A; Zhang, Y; Solomon, S;

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YEAR: 2008     DOI:

The ionospheric and thermospheric response to CMEs: Challenges and successes

Burns, A.G.; Solomon, S.C.; Wang, W.; Killeen, T.L.;

Published by: Journal of Atmospheric and Solar-Terrestrial Physics      Published on: Jan-02-2007

YEAR: 2007     DOI: 10.1016/j.jastp.2006.06.010

Overview of TIMED CEDAR observations showing the MLTI system response to changing drivers from solar maximum to solar minimum

Kozyra, JU; Crowley, G; Doe, RA; Mlynczak, MG; Paxton, LJ; Skinner, WR; Solomon, SC; Talaat, E; Woods, TN; Wu, Q; , others;

Published by:       Published on:

YEAR: 2007     DOI:

Solar Cycle and Seasonal Variation of Thermospheric Density and Composition

Qian, L; Solomon, SC;

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YEAR: 2007     DOI:

Numerical models of the E-region ionosphere

Solomon, Stanley;

Published by: Advances in Space Research      Published on: Jan-01-2006

YEAR: 2006     DOI: 10.1016/j.asr.2005.09.040

The TIGER (thermospheric\textendashionospheric geospheric research) program: Introduction

Schmidtke, G.; Eparvier, F.G.; Solomon, S.C.; Tobiska, W.K.; Woods, T.N.;

Published by: Advances in Space Research      Published on: Jan-01-2006

YEAR: 2006     DOI: 10.1016/j.asr.2005.02.088

Vertical variations in the N2 mass mixing ratio during a thermospheric storm that have been simulated using a coupled magnetosphere-ionosphere-thermosphere model

Burns, AG; Wang, W; Killeen, TL; Solomon, SC; Wiltberger, M;

Published by: Journal of Geophysical Research: Space Physics      Published on:

YEAR: 2006     DOI:

Compositional changes in thermosphere during a geomagnetic storm inferred using ground-based daytime OI 630.0 nm optical airglow emissions

Pallamraju, D; Chakrabarti, S; Solomon, S; Crowley, G;

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YEAR: 2006     DOI:

Geophysical Monograph SeriesRecurrent Magnetic Storms: Corotating Solar Wind StreamsResponse of the upper/middle atmosphere to coronal holes and powerful high-speed solar wind streams in 2003

Kozyra, J.; Crowley, G.; Emery, B.; Fang, X.; Maris, G.; Mlynczak, M.; Niciejewski, R.; Palo, S.; Paxton, L.; Randall, C.; Rong, P.-P.; Russell, J.; Skinner, W.; Solomon, S.; Talaat, E.; Wu, Q.; Yee, J.-H.;

Published by:       Published on:

YEAR: 2006     DOI: 10.1029/GM16710.1029/167GM24

Response of the upper/middle atmosphere to coronal holes and powerful high-speed solar wind streams in 2003

Kozyra, JU; Crowley, G; RONG, P-P; RUSSELL, JM; SKINNER, W; Solomon, SC;

Published by: Geophysical monograph      Published on:

YEAR: 2006     DOI:

TIMED Doppler interferometer (TIDI) observations of migrating diurnal and semidiurnal tides

Wu, Qian; Killeen, TL; Ortland, DA; Solomon, SC; Gablehouse, RD; Johnson, RM; Skinner, WR; Niciejewski, RJ; Franke, SJ;

Published by: Journal of atmospheric and solar-terrestrial physics      Published on:

YEAR: 2006     DOI:

The October 28, 2003 extreme EUV solar flare and resultant extreme ionospheric effects: Comparison to other Halloween events and the Bastille Day event

Some of the most intense solar flares measured in 0.1 to 0.8 nm x-rays in recent history occurred near the end of 2003. The Nov 4 event is the largest in the NOAA records (X28) and the Oct 28 flare was the fourth most intense (X17). The Oct 29 flare was class X7. These flares are compared and contrasted to the July 14, 2000 Bastille Day (X10) event using the SOHO SEM 26.0 to 34.0 nm EUV and TIMED SEE 0.1\textendash194 nm data. High time resolution, \~30s ground-base GPS data and the GUVI FUV dayglow data are used to exami ...

Tsurutani, B.; Judge, D.; Guarnieri, F.; Gangopadhyay, P.; Jones, A.; Nuttall, J.; Zambon, G.A.; Didkovsky, L.; Mannucci, A.J.; Iijima, B.; Meier, R.; Immel, T.J.; Woods, T.; Prasad, S.; Floyd, L.; Huba, J.; Solomon, S.; Straus, P.; Viereck, R.;

Published by: Geophysical Research Letters      Published on: 02/2005

YEAR: 2005     DOI: 10.1029/2004GL021475

Earth FUV Dayglow Response to the 20 January 2005 Solar Flare: TIMED and IMAGE Observations

Retherford, KD; Gladstone, R; Solomon, SC; Immel, TJ;

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YEAR: 2005     DOI:

Solar EUV Experiment (SEE): Mission overview and first results

[1]\ The Solar EUV Experiment (SEE) is one of four scientific instruments on the NASA Thermosphere Ionosphere Mesosphere Energetics Dynamics (TIMED) spacecraft, which has been simultaneously observing the Sun and Earth\textquoterights upper atmosphere since January 2002. The SEE instrument measures the irradiance of the highly variable, solar extreme ultraviolet (EUV) radiation, one of the major energy sources for the upper atmosphere. The primary SEE data product is the solar spectral irradiances from 0.1 to 194 nm ...

Woods, Thomas; Eparvier, Francis; Bailey, Scott; Chamberlin, Phillip; Lean, Judith; Rottman, Gary; Solomon, Stanley; Tobiska, Kent; Woodraska, Donald;

Published by: Journal of Geophysical Research: Space Physics (1978\textendash2012)      Published on:

YEAR: 2005     DOI: 10.1029/2004JA010765

thermosphere; solar activity cycle; solar irradiance; ultraviolet emissions; solar effects

Thermospheric Response to Solar EUV during Quiet and Flare Conditions

Solomon, SC; Qian, L; Gladstone, GR; Bailey, SM; Rodgers, EM;

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YEAR: 2005     DOI:

First Three Years of TIMED: New Results in Sun-Earth Connections

Kozyra, JU; Crowley, G; Goncharenko, LP; Hagan, ME; Lu, G; Mlynczak, MG; Paxton, LJ; RUSSELL, JM; Solomon, SC; Talaat, ER; , others;

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YEAR: 2004     DOI:

Quantification of the spreading effect of auroral proton precipitation

A three-dimensional Monte Carlo model has been developed to study the transverse beam spreading effect of incident energetic auroral protons during their precipitation in the Earth\textquoterights upper atmosphere. Energetic protons with an isotropic angular distribution are injected at 700 km altitude. Two types of incident energy spectra, a monoenergetic and a Maxwellian distribution, are considered. Interaction of fast particles with a three-species atmosphere (O, N₂, and O₂) is included through c ...

Fang, Xiaohua; Liemohn, Michael; Kozyra, Janet; Solomon, Stanley;

Published by: Journal of Geophysical Research: Space Physics (1978\textendash2012)      Published on:

YEAR: 2004     DOI: 10.1029/2003JA010119

Monte Carlo simulation; Proton aurora

New measurements by the TIMED solar extreme-ultraviolet experiment: Implications for thermospheric modeling

Solomon, SC; Bailey, SM; Eparvier, FG; Gladstone, GR; Paxton, LJ; Woods, TN;

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YEAR: 2003     DOI:

The Response of Thermospheric Nitric Oxide to the Geomagnetic Storm of April 2002

Bailey, SM; Crowley, G; Solomon, SC; Baker, DN;

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YEAR: 2002     DOI:

New Solar Extreme-Ultraviolet and Soft X-ray Measurements: Model Comparisons with Thermosphere and Ionosphere Observations

Solomon, SC; Bailey, SM; Christensen, AB; Eparvier, FG; Gladstone, GR; Paxton, LJ; Wolven, BC; Woods, TN;

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YEAR: 2002     DOI:

A Comparison of FUV Auroral Emissions During the April 2002 Events as seen by the IMAGE/FUV and TIMED/GUVI Instruments

Gladstone, G; Retherford, K; Solomon, S; Gerard, J; Hubert, Beno\^\it; Meurant, M; Paxton, L; Wolven, B; Zhang, Yinghong; Morrison, D; , others;

Published by:       Published on:

YEAR: 2002     DOI: