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Features of observing for weak MSTIDs by GNSS satellites

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dc.contributor.author Sherstyukov R.
dc.contributor.author Akchurin A.
dc.contributor.author Sherstyukov O.
dc.date.accessioned 2020-01-15T22:11:25Z
dc.date.available 2020-01-15T22:11:25Z
dc.date.issued 2019
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/156950
dc.description.abstract © 2019 URSI. All rights reserved. To analyze the weak midlatitude medium-scale travelling ionospheric disturbances we use the sufficiently dense network of GNSS receivers (more than 150 ground-based stations). We show the reason that the monitoring for MSTIDs by GNSS satellites is fragmented. Comparing of satellites R18 and G18 data (at 9:40 UT on September 21, 2016) revealed that the LOS directed to ongoing MSTIDs front is preferred for MSTIDs observing. The characteristics of extremely weak MSTIDs with TECp values ~0.2 TECU, wavelength~ 100 km and western direction of phase front moving are presented. We estimate these characteristics as a threshold for monitoring the MSTIDs by GNSS network we used.
dc.title Features of observing for weak MSTIDs by GNSS satellites
dc.type Conference Paper
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS-2019-SID85068593463


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  • Публикации сотрудников КФУ Scopus [22633]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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