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David Long
Researcher at University College London
Publications - 338
Citations - 10139
David Long is an academic researcher from University College London. The author has contributed to research in topics: Coronal mass ejection & Solar flare. The author has an hindex of 49, co-authored 286 publications receiving 9270 citations. Previous affiliations of David Long include Wayne State University & Penn State Milton S. Hershey Medical Center.
Papers
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Physiologically Personalized Color Management for Motion Picture Workflows
TL;DR: In this paper , color matching functions (CMFs) are used to predict the average spectral integration behavior of observers, which can result in impactful color rendering errors, as there exists significant variation in the spectral absorption characteristics of the eye within populations of color-normal observers.
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‘Laramide’ events: Mid North Sea High (UK Quadrants 38 & 39)
TL;DR: In this paper, seismic reflection profiles were used to map isopach patterns of the Chalk Group (Upper Cretaceous and lowermost Paleocene), of the combined Montrose and Moray groups (Paleocene and lower most Eocene), and of the lower Stronsay Group (lower Eocene) in UK Quadrants 38 and 39, on the eastern Mid North Sea High.
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Plasma Upflows Induced by Magnetic Reconnection Above an Eruptive Flux Rope
Deborah Baker,Teodora Mihailescu,Pascal Démoulin,Lucie M. Green,Lidia van Driel-Gesztelyi,Lidia van Driel-Gesztelyi,Lidia van Driel-Gesztelyi,Gherardo Valori,Gherardo Valori,David H. Brooks,David Long,Miho Janvier +11 more
TL;DR: In this article, the authors examined the driving mechanism(s) of the very strong upflows with velocities in excess of 70 km/s−1, known as blue-wing asymmetries, observed during the eruption of a flux rope in AR 10977 (eruptive flare SOL2007-12-07T04:50).
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Localised acceleration of energetic particles by a weak shock in the solar corona
TL;DR: In this paper, it was shown that a reconfiguration of the coronal magnetic field driven by the erupting CME enabled the weak shock to accelerate particles along field lines initially contained within the fan and subsequently opened into the heliosphere, producing the observed type III emission.
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The source of unusual coronal upflows with photospheric abundance in a solar active region
Louise K. Harra,Cristina H. Mandrini,David H. Brooks,Krzysztof Barczynski,Cecilia Mac Cormack,G. D. Cristiani,Suman Mandal,A. C. Sterling,V. Martínez Pillet,Nils Janitzek,Udo Schühle,David Berghmans,F. Auchère,R. Aznar Cuadrado,Eric Buchlin,E. Kraaikamp,David Long +16 more
TL;DR: The upflows in the corona are of importance, as they may contribute to the solar wind as mentioned in this paper , and there has been considerable interest in up�ows from active regions (ARs).