| Form of presentation | Articles in international journals and collections |
| Year of publication | 2019 |
| Язык | английский |
|
Akchurin Adel Dzhavidovich, author
Sherstyukov Oleg Nikolaevich, author
|
| Bibliographic description in the original language |
Sherstyukov R.O, Akchurin A.D, Sherstyukov O.N., Features of observing for weak MSTIDs by GNSS satellites//2019 URSI Asia-Pacific Radio Science Conference, AP-RASC 2019. - 2019. - Vol., Is.. - Art. № 8738525. |
| Annotation |
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. ? 2019 URSI. All rights reserved. |
| Keywords |
weak MSTIDs , GNSS satellites |
| The name of the journal |
2019 URSI Asia-Pacific Radio Science Conference, AP-RASC 2019
|
| URL |
https://www.scopus.com/inward/record.uri?eid=2-s2.0-85068593463&doi=10.23919%2fURSIAP-RASC.2019.8738525&partnerID=40&md5=7ebde5abc3d4d66c1e57696c8013d432 |
| Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=205993&p_lang=2 |
Full metadata record  |
| Field DC |
Value |
Language |
| dc.contributor.author |
Akchurin Adel Dzhavidovich |
ru_RU |
| dc.contributor.author |
Sherstyukov Oleg Nikolaevich |
ru_RU |
| dc.date.accessioned |
2019-01-01T00:00:00Z |
ru_RU |
| dc.date.available |
2019-01-01T00:00:00Z |
ru_RU |
| dc.date.issued |
2019 |
ru_RU |
| dc.identifier.citation |
Sherstyukov R.O, Akchurin A.D, Sherstyukov O.N., Features of observing for weak MSTIDs by GNSS satellites//2019 URSI Asia-Pacific Radio Science Conference, AP-RASC 2019. - 2019. - Vol., Is.. - Art. № 8738525. |
ru_RU |
| dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=205993&p_lang=2 |
ru_RU |
| dc.description.abstract |
2019 URSI Asia-Pacific Radio Science Conference, AP-RASC 2019 |
ru_RU |
| dc.description.abstract |
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. ? 2019 URSI. All rights reserved. |
ru_RU |
| dc.language.iso |
ru |
ru_RU |
| dc.subject |
weak MSTIDs |
ru_RU |
| dc.subject |
GNSS satellites |
ru_RU |
| dc.title |
Features of observing for weak MSTIDs by GNSS satellites |
ru_RU |
| dc.type |
Articles in international journals and collections |
ru_RU |
|
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