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Whistler intensities above thunderstorms
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SYSNO ASEP 0340437 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Whistler intensities above thunderstorms Tvůrce(i) Fišer, Jiří (UFA-U) RID, ORCID
Chum, Jaroslav (UFA-U) RID, ORCID
Diendorfer, G. (AT)
Parrot, M. (FR)
Santolík, Ondřej (UFA-U) RID, ORCIDZdroj.dok. Annales Geophysicae. - : Copernicus - ISSN 0992-7689
Roč. 28, č. 1 (2010), s. 37-46Poč.str. 10 s. Forma vydání web - web Jazyk dok. eng - angličtina Země vyd. US - Spojené státy americké Klíč. slova Ionosphere (Wave propagation) ; Meteorology and atmospheric dynamics (Lightning) ; Radio science (Waves in plasma) Vědní obor RIV BL - Fyzika plazmatu a výboje v plynech CEP GA205/09/1253 GA ČR - Grantová agentura ČR CEZ AV0Z30420517 - UFA-U, BC-A (2005-2011) UT WOS 000274136900005 DOI 10.5194/angeo-28-37-2010 Anotace We report a study of penetration of the VLF electromagnetic waves induced by lightning to the ionosphere. We compare the fractional hop whistlers recorded onboard the DEMETER satellite with lightning detected by the EUCLID network. We have developed software for automatic detection of the fractional hop whistlers in the VLF spectrograms. We obtain a map of mean amplitudes of whistler electric field as a function of latitudinal and longitudinal difference between the location of the causative lightning and satellite magnetic footprint. The mean whistler amplitude monotonically decreases with horizontal distance up to ~1000 km from the lightning. The maximum of whistler intensities is shifted from the satellite magnetic footprint ~1° owing to the oblique propagation. The average amplitude of whistlers increases with the lightning current. At nighttime, the average amplitude of whistlers is about three times higher than during the daytime. Pracoviště Ústav fyziky atmosféry Kontakt Kateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019 Rok sběru 2010
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