GUVI Biblio | guvitimed.jhuapl.edu

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Found 19 entries in the Bibliography.

Showing entries from 1 through 19

2018

Thermospheric Neutral Composition Response to External Forcings

Fedrizzi, Mariangel; Karol, Svetlana; Yudin, Valery; Fuller-Rowell, Timothy; Codrescu, Mihail; Olsen, Jack; Paxton, Larry; Zhang, Yongliang;

Published by: Published on:

YEAR: 2018 DOI:

2016

Disturbances in the Thermosphere and Ionosphere: Current Understanding and Operational Impacts II Posters

Zhang, Yongliang; Paxton, Larry; Fuller-Rowell, Timothy; Jones, James;

Published by: Published on:

YEAR: 2016 DOI:

2014

Comparative studies of theoretical models in the equatorial ionosphere

Fang, Tzu-Wei; Anderson, David; Fuller-Rowell, Tim; Akmaev, Rashid; Codrescu, Mihail; Millward, George; Sojka, Jan; Scherliess, Ludger; Eccles, Vince; Retterer, John; , others;

Published by: Modeling the ionosphere—thermosphere system Published on:

YEAR: 2014 DOI:

Ensemble Assimilation Using Three First-Principles Thermospheric Models as a Tool for 72-hour Density and Satellite Drag Forecasts

Hunton, Don; Pilinski, Marcin; Crowley, Geoff; Azeem, I; Fuller-Rowell, Timothy; Matsuo, Tomoko; Fedrizzi, Mariangel; Solomon, Stanley; Qian, Liying; Thayer, Jeffrey; , others;

Published by: Published on:

YEAR: 2014 DOI:

Predictability and Ensemble Modeling of the Space-Atmosphere Interaction Region

Matsuo, Tomoko; Fuller-Rowell, Timothy; Akmaev, Rashid; Wang, Houjun; Fang, Tzu-Wei; Ide, Kayo; Kleist, Daryl; Whitaker, JS; Yue, Xinan; Codrescu, Mihail; , others;

Published by: Published on:

YEAR: 2014 DOI:

Thermospheric Composition Variability and Its Coupling to the Ionosphere I

Zhang, Yongliang; Paxton, Larry; Fuller-Rowell, Timothy; Knipp, Delores;

Published by: Published on:

YEAR: 2014 DOI:

2013

Is Space Weather Different Over Africa, and If So, Why? An AGU Chapman Conference Report

With the increasing reliance on technology, the impact of space weather on engineered systems will certainly increase unless suitable protective measures are taken. Understanding the physics behind space weather impacts and improving the forecasting are the major objectives of the space science community. It is well recognized that many space weather impacts, especially on communications systems, arise from structures in the ionosphere. The equatorial ionosphere, in particular, is one of the most complex and is host to nu ...

Yizengaw, Endawoke; Doherty, Patricia; Fuller-Rowell, Tim;

Published by: Space Weather Published on: 07/2013

YEAR: 2013 DOI: 10.1002/swe.20063

atmosphere ionosphere interactions; ionospheric irregularities; space weather

Is space weather different over Africa, and if so, why? An agu chapman conference report

Yizengaw, Endawoke; Doherty, Patricia; Fuller-Rowell, Tim;

Published by: Published on:

YEAR: 2013 DOI:

2012

Extreme Ultraviolet Variability Experiment (EVE) on~the~Solar Dynamics Observatory (SDO): Overview~of~Science Objectives, Instrument Design, Data~Products, and Model Developments

The highly variable solar extreme ultraviolet (EUV) radiation is the major energy input to the Earth\textquoterights upper atmosphere, strongly impacting the geospace environment, affecting satellite operations, communications, and navigation. The Extreme ultraviolet Variability Experiment (EVE) onboard the NASA Solar Dynamics Observatory (S ...

Woods, T.; Eparvier, F.; Hock, R.; Jones, A.; Woodraska, D.; Judge, D.; Didkovsky, L.; Lean, J.; Mariska, J.; Warren, H.; McMullin, D.; Chamberlin, P.; Berthiaume, G.; Bailey, S.; Fuller-Rowell, T.; Sojka, J.; Tobiska, W.; Viereck, R.;

Published by: Solar Physics Published on: 01/2012

YEAR: 2012 DOI: 10.1007/s11207-009-9487-6

EVE; SDO; Solar EUV irradiance; Space weather research

Quantitative comparison of CTIPe model results with ground and space-based observations

Fedrizzi, M; , Olsen; Fuller-Rowell, TJ; Codrescu, M;

Published by: Published on:

YEAR: 2012 DOI:

2011

Storm-Time Response of the Thermosphere\textendashIonosphere System

During a geomagnetic storm, the magnetospheric energy injected into the upper atmosphere increases by at least an order of magnitude, and during these times far exceeds the solar EUV and UV energy input. The energy is initially deposited towards higher latitudes where it heats and expands the thermosphere, increasing temperature and neutral density. Ionospheric plasma at high latitudes accelerates in response to the magnetospheric forcing, and through collisions can drive neutral winds in excess of 1\ km/s. Large sca ...

Fuller-Rowell, Timothy;

Published by: Published on:

YEAR: 2011 DOI: 10.1007/978-94-007-0326-1_32

2010

Equatorial-PRIMO (Problems Related to Ionospheric Models and Observations)

Fang, T; Anderson, DN; Fuller-Rowell, TJ; Akmaev, RA; Codrescu, M; Millward, GH; Sojka, JJ; Scherliess, L; Eccles, JV; Retterer, JM; , others;