Multi-instrument observations of large-scale atmospheric gravity waves/traveling ionospheric disturbances associated with enhanced auroral activity over Svalbard
Autor: | Kirsti Kauristie, Kjellmar Oksavik, Zama T. Katamzi-Joseph, Michael Kosch, Anasuya Aruliah, John Bosco Habarulema |
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Rok vydání: | 2019 |
Předmět: |
Physics
Atmospheric Science 010504 meteorology & atmospheric sciences Total electron content Magnetometer TEC Aerospace Engineering Astronomy and Astrophysics Geodesy 01 natural sciences law.invention Azimuth Geophysics Space and Planetary Science law 0103 physical sciences Substorm General Earth and Planetary Sciences Ionosphere Joule heating 010303 astronomy & astrophysics 0105 earth and related environmental sciences Line (formation) |
Zdroj: | Advances in Space Research. 63:270-281 |
ISSN: | 0273-1177 |
DOI: | 10.1016/j.asr.2018.08.042 |
Popis: | This study reports on observations of large-scale atmospheric gravity waves/traveling ionospheric disturbances (AGWs/TIDs) using Global Positioning System (GPS) total electron content (TEC) and Fabry–Perot Interferometer’s (FPI’s) intensity of oxygen red line emission at 630 nm measurements over Svalbard on the night of 6 January 2014. TEC large-scale TIDs have primary periods ranging between 29 and 65 min and propagate at a mean horizontal velocity of ∼ 749–761 m/s with azimuth of ∼ 345–347 ° (which corresponds to poleward propagation direction). On the other hand, FPI large-scale AGWs have larger periods of ∼ 42–142 min. These large-scale AGWs/TIDs were linked to enhanced auroral activity identified from co-located all-sky camera and IMAGE magnetometers. Similar periods, speed and poleward propagation were found for the all-sky camera ( ∼ 60–97 min and ∼ 823 m/s) and the IMAGE magnetometers ( ∼ 32–53 min and ∼ 708 m/s) observations. Joule heating or/and particle precipitation as a result of auroral energy injection were identified as likely generation mechanisms for these disturbances. |
Databáze: | OpenAIRE |
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