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R. C. Noggle

Researcher at University of Arizona

Publications -  7
Citations -  397

R. C. Noggle is an academic researcher from University of Arizona. The author has contributed to research in topics: Lightning & Lightning detection. The author has an hindex of 6, co-authored 6 publications receiving 386 citations.

Papers
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Journal ArticleDOI

A Gated, Wideband Magnetic Direction Finder for Lightning Return Strokes

TL;DR: In this article, a magnetic direction finder was developed which utilizes only the initial few microseconds of wideband return stroke waveforms to provide accurate directions to the channel bases of lightning discharges to ground.
Journal ArticleDOI

Broadband antenna systems for lightning magnetic fields

TL;DR: In this article, the authors describe two types of magnetic antenna systems suitable for recording sub-microsecond field changes from distant lightning, one with a high-impedance antenna loop connected to the integrator by a twisted pair of coaxial cables, and another with the antenna loop and twisted signal loops formed from a single piece of cable.
Patent

Gated lightning detection system

TL;DR: In this article, a gated magnetic direction finder was used for determining the range and direction of lightning discharges to ground. But the magnetic direction detector was not gated.
Patent

Detection system for lightning

TL;DR: In this article, a gated magnetic direction finder is used to determine the range and direction of lightning discharges to ground, and logic circuitry is provided for controlling gating circuits within the directed finder so that the direction measurement is made during the initial few microseconds of the return stroke waveform, thereby minimizing errors caused by nonvertical lightning channels to ground.
Journal ArticleDOI

Lightning and the Apollo 17/Saturn V Exhaust Plume

TL;DR: In this paper, a survey of the Apollo 17/Saturn V exhaust plume during launch was obtained in the ultraviolet, visible, and near infrared, showing that the plume resembles a blackbody source for about 40 m from the exit plane, and beyond this point the characteristic radiation is the sodium D-lines.