D
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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Journal ArticleDOI
Understanding the Physical Nature of Coronal "EIT Waves"
David Long,D. Shaun Bloomfield,Peng-Fei Chen,Cooper Downs,Peter T. Gallagher,Ryun-Young Kwon,Kamalam Vanninathan,Astrid Veronig,Angelos Vourlidas,Bojan Vršnak,Alexander Warmuth,T. Zic +11 more
TL;DR: In this paper, the authors reexamine the theories proposed to explain "EIT waves" to identify measurable properties and behaviours that can be compared to current and future observations, and conclude that EIT waves are best described as fastmode large-amplitude waves/shocks that are initially driven by the impulsive expansion of an erupting coronal mass ejection in the low corona.
Journal ArticleDOI
Silicone Rubber: A New Diffusion Property Useful for General Anesthesia
TL;DR: Silicone rubber tubing for general anesthesia can be produced in dogs by passing the vapors of any of these anesthetic agents through a coil of silicone rubber tubing, each end of which is placed in an artery and vein.
Journal ArticleDOI
Gas migration pathways, controlling mechanisms and changes in sediment acoustic properties observed in a controlled sub-seabed CO2 release experiment
TL;DR: In this article, the impacts of a CO2 release were investigated by a controlled release experiment that injected CO2 at a known flux into shallow, under-consolidated marine sediments for 37 days.
Book
The Geology of the Moray Firth
TL;DR: The geology of the Moray Firth is described in detail in this paper, where the authors present a series of ten Offshore Regional Reports produced by the British Geological Survey.
Journal ArticleDOI
The wave properties of coronal bright fronts observed using SDO/AIA
TL;DR: In this article, the authors used high cadence, multi-thermal observations of the solar corona from the Solar Dynamic Observatory (SDO) and Solar TErrestrial RElations Observatory (STEREO) spacecraft to determine the kinematics and expansion rate of a CBF wavefront observed on 2010 August 14.