Incoherent scatter radar study of the impact of the meteoric influx on nocturnal E-region ionization

Q. H. Zhou, John David Mathews, Q. N. Zhou

    Research output: Contribution to journalArticle

    17 Citations (Scopus)

    Abstract

    We use the Arecibo incoherent scatter radar data collected from 1987 to 1995 to study meteoric impact on the nocturnal E-region electron/ion content. The nighttime ionization is observed to increase after midnight, which we interpret to be due to increase in background meteoric input. The column incremental rate due to meteoric ionization between 0100 to 0600 LT is estimated to be 109/cm2/hr. Direct meteoric deposition is responsible for 60% of the total ionization in the morning hours in the altitude range of 97 to 114 km. Although there appears to be an increase in electron content during shower periods, there is not an one-to-one relation between meteor showers and E-region ionization enhancement.

    Original languageEnglish (US)
    Article number1999GL900369
    Pages (from-to)1833-1836
    Number of pages4
    JournalGeophysical Research Letters
    Volume26
    Issue number13
    DOIs
    StatePublished - Jul 1 1999

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    incoherent scatter radar
    E region
    ionization
    radar
    showers
    electron
    morning
    radar data
    meteoroids
    meteor
    electrons
    ion
    augmentation
    ions

    All Science Journal Classification (ASJC) codes

    • Geophysics
    • Earth and Planetary Sciences(all)

    Cite this

    Zhou, Q. H. ; Mathews, John David ; Zhou, Q. N. / Incoherent scatter radar study of the impact of the meteoric influx on nocturnal E-region ionization. In: Geophysical Research Letters. 1999 ; Vol. 26, No. 13. pp. 1833-1836.
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    abstract = "We use the Arecibo incoherent scatter radar data collected from 1987 to 1995 to study meteoric impact on the nocturnal E-region electron/ion content. The nighttime ionization is observed to increase after midnight, which we interpret to be due to increase in background meteoric input. The column incremental rate due to meteoric ionization between 0100 to 0600 LT is estimated to be 109/cm2/hr. Direct meteoric deposition is responsible for 60{\%} of the total ionization in the morning hours in the altitude range of 97 to 114 km. Although there appears to be an increase in electron content during shower periods, there is not an one-to-one relation between meteor showers and E-region ionization enhancement.",
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    Incoherent scatter radar study of the impact of the meteoric influx on nocturnal E-region ionization. / Zhou, Q. H.; Mathews, John David; Zhou, Q. N.

    In: Geophysical Research Letters, Vol. 26, No. 13, 1999GL900369, 01.07.1999, p. 1833-1836.

    Research output: Contribution to journalArticle

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