Latitudinal variations of diurnal meteor rates

Csilla Szasz, Johan Kero, Asta Pellinen-Wannberg, John D. Mathews, Nick J. Mitchell, Werner Singer

    Research output: Contribution to journalArticlepeer-review

    17 Scopus citations


    The presence of a diurnal variation in meteor activity is well established. The sporadic meteor count rates are higher on the local dawn side and lower on the local dusk side. This phenomenon is caused by the Earth's orbital motion and rotation. Meteor radar measurements have been compared from Esrange, Kiruna, Sweden, at 68° N, from Juliusruh, Germany, at 55° N, and from Ascension Island, at 8° S, to investigate how the diurnal variation depends on season at different latitudes. Data have been used from vernal and autumnal equinoxes and summer and winter solstices to locate the largest seasonal differences.

    Original languageEnglish (US)
    Pages (from-to)101-107
    Number of pages7
    JournalEarth, Moon and Planets
    Issue number1-4
    StatePublished - Dec 2004

    All Science Journal Classification (ASJC) codes

    • Astronomy and Astrophysics
    • Earth and Planetary Sciences (miscellaneous)
    • Space and Planetary Science


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