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contributor authorHerrman, B. D.
contributor authorUman, M. A.
contributor authorBrantley, R. D.
contributor authorKrider, E. P.
date accessioned2017-06-09T17:38:34Z
date available2017-06-09T17:38:34Z
date copyright1976/04/01
date issued1976
identifier issn0021-8952
identifier otherams-9061.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4232508
description abstractThe principle of operation of a wideband crossed-loop magnetic-field direction finder is studied by comparing the bearing determined from the NS and EW magnetic fields at various times up to 155 ?s after return stroke initiation with the TV-determined lightning channel base direction. For 40 lightning strokes in the 3 to 12 km range, the difference between the bearings found from magnetic fields sampled at times between 1 and 10 ?s and the TV channel-base data has a standard deviation of 3°?4°. Included in this standard deviation is a 2°?3° measurement error. For fields sampled at progressively later times, both the mean and the standard deviation of the difference between the direction-finder bearing and the TV bearing increase. Near 150 ?s, means are about 35° and standard deviations about 60°. The physical reasons for the late-time inaccuracies in the wideband direction finder and the occurrence of these effects in narrow-band VLF direction finders are considered.
publisherAmerican Meteorological Society
titleTest of the Principle of Operation of a Wideband Magnetic Direction Finder for Lightning Return Strokes
typeJournal Paper
journal volume15
journal issue4
journal titleJournal of Applied Meteorology
identifier doi10.1175/1520-0450(1976)015<0402:TOTPOO>2.0.CO;2
journal fristpage402
journal lastpage405
treeJournal of Applied Meteorology:;1976:;volume( 015 ):;issue: 004
contenttypeFulltext


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