Microscopic observations of pulsating aurora associated with chorus element structures : coordinated arase satellite‐PWING observations |
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Author: | Ozaki, M.1; Shiokawa, K.2; Miyoshi, Y.2; |
Organizations: |
1Kanazawa Univ, Grad Sch Nat Sci & Technol, Kanazawa, Ishikawa, Japan 2Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi, Japan 3Univ Electrocommun, Grad Sch Informat & Engn, Chofu, Tokyo, Japan
4Univ Oulu, Ionosphere Res Unit, Oulu, Finland
5Natl Inst Polar Res, Tachikawa, Tokyo, Japan 6Tohoku Univ, Grad Sch Sci, Sendai, Miyagi, Japan 7Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Tokyo, Japan 8Grad Univ Adv Studies SOKENDAI, Dept Polar Sci, Tachikawa, Tokyo, Japan 9Kyoto Univ, Res Inst Sustainable Elumanosphere, Kyoto, Japan 10Univ Florida, Dept Elect & Comp Engn, Gainesville, FL USA 11Res Org Informat & Syst, Joint Support Ctr Data Sci Res, Tokyo, Japan 12Natl Inst Informat & Commun Technol, Tokyo, Japan 13Athabasca Univ, Ctr Sci, Athabasca, AB, Canada |
Format: | article |
Version: | published version |
Access: | open |
Online Access: | PDF Full Text (PDF, 4.5 MB) |
Persistent link: | http://urn.fi/urn:nbn:fi-fe201902226069 |
Language: | English |
Published: |
American Geophysical Union,
2018
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Publish Date: | 2019-05-26 |
Description: |
AbstractRapid (<1 s) intensity modulation of pulsating auroras is caused by successive chorus elements as a response to wave‐particle interactions in the magnetosphere. Here we found that a pulsating auroral patch responds to the time spacing for successive chorus elements and possibly to chorus subpacket structures with a time scale of tens of milliseconds. These responses were identified from coordinated Arase satellite and ground (Gakona, Alaska) observations with a high‐speed auroral imager (100 Hz). The temporal variations of auroral intensity in a few‐hertz frequency range exhibited a spatial concentration at the lower‐latitude edge of the auroral patch. The spatial evolution of the auroral patch showed repeated expansion/contraction with tens of kilometer scales in the ionosphere, which could be spatial behaviors in the wave‐particle interactions. These observations indicate that chorus elements evolve coherently within the auroral patch, which is approximately 900 km in the radial and longitudinal directions at the magnetic equator. see all
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Series: |
Geophysical research letters |
ISSN: | 0094-8276 |
ISSN-E: | 1944-8007 |
ISSN-L: | 0094-8276 |
Volume: | 45 |
Issue: | 22 |
Pages: | 12,125 - 12,134 |
DOI: | 10.1029/2018GL079812 |
OADOI: | https://oadoi.org/10.1029/2018GL079812 |
Type of Publication: |
A1 Journal article – refereed |
Field of Science: |
115 Astronomy and space science |
Subjects: | |
Funding: |
MEXT | Japan Society for the Promotion of Science (JSPS), International Space Science Institute‐Beijing (ISSI‐BJ) International team program, IUGONET (Inter‐university Upper atmosphere Global Observation NETwork) project, JSPS Bilateral Open Partnership Joint Research Projects, Kanazawa University SAKIGAKE project, JSPS KAKENHI. Grant Numbers: JP17K06456, JP17H06140, JP16H04056, JP16H06286, JP15H05815, JP15H05747, JP14J02108, JP17K05668, JP18H03727. |
Copyright information: |
© 2018. American Geophysical Union. All Rights Reserved. |