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Lightning Contribution to Overall Whistler Mode Wave Intensities in the Plasmasphere

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    0507729 - ÚFA 2020 RIV US eng J - Journal Article
    Záhlava, Jan - Němec, F. - Santolík, Ondřej - Kolmašová, Ivana - Hospodarsky, G. B. - Parrot, M. - Kurth, W. S. - Kletzing, C. A.
    Lightning Contribution to Overall Whistler Mode Wave Intensities in the Plasmasphere.
    Geophysical Research Letters. Roč. 46, č. 15 (2019), s. 8607-8616. ISSN 0094-8276. E-ISSN 1944-8007
    R&D Projects: GA ČR(CZ) GA17-07027S
    Grant - others:AV ČR(CZ) AP1401
    Program: Akademická prémie - Praemium Academiae
    Institutional support: RVO:68378289
    Keywords : VLF line radiation * field experiment * Demeter * frequency * magnetosphere * association * propagation * emissions * electron * system
    OECD category: Fluids and plasma physics (including surface physics)
    Impact factor: 4.497, year: 2019
    Method of publishing: Open access
    https://hal-insu.archives-ouvertes.fr/insu-02263541/file/Z-hlava_et_al-2019-Geophysical_Research_Letters.pdf

    Electromagnetic waves generated by lightning propagate into the plasmasphere as dispersed whistlers. They can therefore influence the overall wave intensity in space, which, in turn, is important for dynamics of the Van Allen radiation belts. We analyze spacecraft measurements in low‐Earth orbit as well as in high‐altitude equatorial region, together with a ground‐based estimate of lightning activity. We accumulate wave intensities when the spacecraft are magnetically connected to thunderstorms and compare them with measurements obtained when thunderstorms are absent. We show that strong lightning activity substantially affects the wave intensity in a wide range of L‐shells and altitudes. The effect is observed mainly between 500 Hz and 4 kHz, but its frequency range strongly varies with L‐shell, extending up to 12 kHz for L lower than 3. The effect is stronger in the afternoon, evening, and night sectors, consistent with more lightning and easier wave propagation through the ionosphere.
    Permanent Link: http://hdl.handle.net/11104/0298706

     
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