Features of observing for weak MSTIDs by GNSS satellites

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

Files in this item

Size: 49.03Kb

Format: PDF

Публикации сотрудников КФУ Scopus [24551]
Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.