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L. C. Gentile

Researcher at Air Force Research Laboratory

Publications -  23
Citations -  649

L. C. Gentile is an academic researcher from Air Force Research Laboratory. The author has contributed to research in topics: Ionosphere & Earth's magnetic field. The author has an hindex of 11, co-authored 23 publications receiving 567 citations.

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DMSP observations of equatorial plasma bubbles in the topside ionosphere near solar maximum

TL;DR: In this paper, the authors examined a large database of postsunset plasma density measurements acquired during ∼ 15,000 equatorial crossings made by DMSP F9 and F10 in 1989 and 1991, respectively.
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C/NOFS observations of deep plasma depletions at dawn

TL;DR: In this article, the authors discuss the roles of dynamo electric fields, over-shielding, and tidal effects as sources for the reported depletions in C/NOFS and ground-based measurements.
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Ionospheric disturbances observed by DMSP at middle to low latitudes during the magnetic storm of June 4–6, 1991

TL;DR: In this article, the authors extend a recent study of electric field penetration into the inner magnetosphere observed by the Combined Release and Radiation Effects (CRRES) satellite and the Defense Meteorological Satellite Program (DMSP) satellite F8 during the magnetic storm of June 4-6, 1991, to consider its ionospheric consequences.
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C/NOFS observations of plasma density and electric field irregularities at post-midnight local times

TL;DR: In this paper, the authors report on plasma densities and electric fields measured by the C/NOFS satellite between 10 and 20 June 2008, and discuss relative contributions of gravity-driven currents, overshielding electric fields and disturbance dynamos as drivers of post-midnight depletions.
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Climatology of plasma density depletions observed by DMSP in the dawn sector

TL;DR: In this paper, the authors take advantage of the long history of plasma density measurements by a similar sensor on Defense Meteorological Satellite Program (DMSP) spacecraft to determine whether this change is typical of solar minima in general or unique to the present extended quiet time.