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    Test of the Principle of Operation of a Wideband Magnetic Direction Finder for Lightning Return Strokes

    Source: Journal of Applied Meteorology:;1976:;volume( 015 ):;issue: 004::page 402
    Author:
    Herrman, B. D.
    ,
    Uman, M. A.
    ,
    Brantley, R. D.
    ,
    Krider, E. P.
    DOI: 10.1175/1520-0450(1976)015<0402:TOTPOO>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The 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.
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      Test of the Principle of Operation of a Wideband Magnetic Direction Finder for Lightning Return Strokes

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4232508
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    • Journal of Applied Meteorology

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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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    DSpace software copyright © 2002-2015  DuraSpace
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