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    Rights statement: This is the author’s version of a work that was accepted for publication in Advances in Space Research. Changes resulting from the publishing process, such as peer review, editing, corrections, structural formatting, and other quality control mechanisms may not be reflected in this document. Changes may have been made to this work since it was submitted for publication. A definitive version was subsequently published in Advances in Space Research, 63, 1, 2018 DOI: 10.1016/j.asr.2018.08.042

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Multi-instrument observations of large-scale atmospheric gravity waves/traveling ionospheric disturbances associated with enhanced auroral activity over Svalbard

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Multi-instrument observations of large-scale atmospheric gravity waves/traveling ionospheric disturbances associated with enhanced auroral activity over Svalbard. / Katamzi-Joseph, Zama T.; Aruliah, Anasuya L.; Oksavik, Kjellmar et al.
In: Advances in Space Research, Vol. 63, No. 1, 01.01.2019, p. 270-281.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

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Katamzi-Joseph ZT, Aruliah AL, Oksavik K, Habarulema JB, Kauristie K, Kosch MJ. Multi-instrument observations of large-scale atmospheric gravity waves/traveling ionospheric disturbances associated with enhanced auroral activity over Svalbard. Advances in Space Research. 2019 Jan 1;63(1):270-281. Epub 2018 Sept 3. doi: 10.1016/j.asr.2018.08.042

Author

Katamzi-Joseph, Zama T. ; Aruliah, Anasuya L. ; Oksavik, Kjellmar et al. / Multi-instrument observations of large-scale atmospheric gravity waves/traveling ionospheric disturbances associated with enhanced auroral activity over Svalbard. In: Advances in Space Research. 2019 ; Vol. 63, No. 1. pp. 270-281.

Bibtex

@article{136028e132eb4a488b35e2eb711e69e8,
title = "Multi-instrument observations of large-scale atmospheric gravity waves/traveling ionospheric disturbances associated with enhanced auroral activity over Svalbard",
abstract = "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{\textquoteright}s (FPI{\textquoteright}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 minutes 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 minutes. 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 minutes and ∼823 m/s) and the IMAGE magnetometers (∼32–53 minutes 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.",
keywords = "ANGWIN, Arctic polar cap, Atmospheric gravity waves, Aurora, Substorm, Traveling ionospheric disturbances",
author = "Katamzi-Joseph, {Zama T.} and Aruliah, {Anasuya L.} and Kjellmar Oksavik and Habarulema, {John Bosco} and Kirsti Kauristie and Kosch, {Michael J.}",
note = "This is the author{\textquoteright}s version of a work that was accepted for publication in Advances in Space Research. Changes resulting from the publishing process, such as peer review, editing, corrections, structural formatting, and other quality control mechanisms may not be reflected in this document. Changes may have been made to this work since it was submitted for publication. A definitive version was subsequently published in Advances in Space Research, 63, 1, 2018 DOI: 10.1016/j.asr.2018.08.042",
year = "2019",
month = jan,
day = "1",
doi = "10.1016/j.asr.2018.08.042",
language = "English",
volume = "63",
pages = "270--281",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier Ltd",
number = "1",

}

RIS

TY - JOUR

T1 - Multi-instrument observations of large-scale atmospheric gravity waves/traveling ionospheric disturbances associated with enhanced auroral activity over Svalbard

AU - Katamzi-Joseph, Zama T.

AU - Aruliah, Anasuya L.

AU - Oksavik, Kjellmar

AU - Habarulema, John Bosco

AU - Kauristie, Kirsti

AU - Kosch, Michael J.

N1 - This is the author’s version of a work that was accepted for publication in Advances in Space Research. Changes resulting from the publishing process, such as peer review, editing, corrections, structural formatting, and other quality control mechanisms may not be reflected in this document. Changes may have been made to this work since it was submitted for publication. A definitive version was subsequently published in Advances in Space Research, 63, 1, 2018 DOI: 10.1016/j.asr.2018.08.042

PY - 2019/1/1

Y1 - 2019/1/1

N2 - 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 minutes 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 minutes. 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 minutes and ∼823 m/s) and the IMAGE magnetometers (∼32–53 minutes 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.

AB - 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 minutes 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 minutes. 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 minutes and ∼823 m/s) and the IMAGE magnetometers (∼32–53 minutes 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.

KW - ANGWIN

KW - Arctic polar cap

KW - Atmospheric gravity waves

KW - Aurora

KW - Substorm

KW - Traveling ionospheric disturbances

U2 - 10.1016/j.asr.2018.08.042

DO - 10.1016/j.asr.2018.08.042

M3 - Journal article

VL - 63

SP - 270

EP - 281

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 1

ER -