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David R. Smith

Researcher at Duke University

Publications -  891
Citations -  102589

David R. Smith is an academic researcher from Duke University. The author has contributed to research in topics: Metamaterial & Antenna (radio). The author has an hindex of 110, co-authored 881 publications receiving 91683 citations. Previous affiliations of David R. Smith include Brunel University London & Princeton University.

Papers
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Proceedings ArticleDOI

The effects of radiation damage on the spectral resolution of the Chandrayaan-1 x-ray spectrometer

TL;DR: The Chandrayaan-1 X-ray Spectrometer (C1XS) was launched onboard the Indian Space Research Organisation (ISROI) spacecraft for the Chandrayaa-1 lunar mission in October 2008 as discussed by the authors.
Journal ArticleDOI

Relationship between edge localized mode severity and electron transport in the National Spherical Torus Experiment

TL;DR: Menard et al. as mentioned in this paper showed that the electron thermal transport during the cold pulses showed a large enhancement over the underlying cross-field thermal diffusivity, χe, of up to several tens of m2∕s.
Book ChapterDOI

Experiment on Cloaking Devices

TL;DR: This chapter discusses the approach of utilizing transformation optic approach and metamaterial technology to construct various cloaking devices in experiment and takes the advantage of rapid design approach to demonstrate the reduced cloaking device in free space.

X-Ray Fluorescence Particle Size and Scattering Angle Considerations - Preparatory Experiments for the Calibration and Interpretation of C1XS Data

TL;DR: In this article, a plan of testing the accuracy and robustness of the C1XS XRF code using XRF spectral data from well characterised geological samples is presented, in order to quantify how XRF intensity varies with changing particle size and phase angle.
Proceedings ArticleDOI

Sun avoidance strategies at the Large Millimeter Telescope

TL;DR: In this article, a sun avoidance strategy was implemented in the control system in real-time to avoid excessive heating and damage to the secondary mirror and the prime focus of the Large Millimeter Telescope observatory.