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Bob Abel

Researcher at Olympic College

Publications -  10
Citations -  4460

Bob Abel is an academic researcher from Olympic College. The author has contributed to research in topics: Electron precipitation & Scattering. The author has an hindex of 9, co-authored 10 publications receiving 3599 citations. Previous affiliations of Bob Abel include University of California, Los Angeles.

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LSST: from Science Drivers to Reference Design and Anticipated Data Products

Željko Ivezić, +312 more
- 15 May 2008 - 
TL;DR: The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the solar system, exploring the transient optical sky, and mapping the Milky Way.
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LSST: From Science Drivers to Reference Design and Anticipated Data Products

Željko Ivezić, +335 more
TL;DR: The Large Synoptic Survey Telescope (LSST) as discussed by the authors is a large, wide-field ground-based system designed to obtain repeated images covering the sky visible from Cerro Pachon in northern Chile.
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Electron scattering loss in Earth's inner magnetosphere: 1. Dominant physical processes

TL;DR: Pitch angle diffusion rates due to Coulomb collisions and resonant interactions with plasmaspheric hiss, lightning-induced whistlers and anthropogenic VLF transmissions are computed for inner magnetospheric electrons as discussed by the authors.
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Electron scattering loss in Earth's inner magnetosphere: 2. Sensitivity to model parameters

TL;DR: In this paper, the sensitivity of the rate of energetic electron pitch angle scattering and precipitation loss in the Earth's magnetosphere due to Coulomb interactions with thermal plasma and resonant wave-particle interactions with plasmaspheric hiss, lightning-generated whistlers and VLF transmitter signals is computed for a realistic range of plasma and wave parameters.
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Solar cyclic behavior of trapped energetic electrons in Earth's inner radiation belt

TL;DR: In this article, a comparison of the observed energy spectra at L equal to or greater than 1.35 for different phases of the solar cycle reveals a clear trend toward enhanced fluxes during periods of solar maximum for energies below a few hundred keV; this is caused by an increase in the rate of inward radial diffusion from a source at higher L.