An Ephemeral Red Arc Appeared at 68° MLat at a Pseudo Breakup During Geomagnetically Quiet Conditions-Reference-Cited by-同舟云学术

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An Ephemeral Red Arc Appeared at 68° MLat at a Pseudo Breakup During Geomagnetically Quiet Conditions

Published:2020-10 Issue:10 Volume:125 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Oyama S.¹²³^ORCID,Shinbori A.¹^ORCID,Ogawa Y.³^ORCID,Kellinsalmi M.⁴,Raita T.⁵,Aikio A.²^ORCID,Vanhamäki H.²^ORCID,Shiokawa K.¹^ORCID,Virtanen I.²^ORCID,Cai L.⁶^ORCID,Workayehu A. B.²^ORCID,Pedersen M.²,Kauristie K.⁴^ORCID,Tsuda T. T.⁷^ORCID,Kozelov B.⁸^ORCID,Demekhov A.⁸^ORCID,Yahnin A.⁸^ORCID,Tsuchiya F.⁹^ORCID,Kumamoto A.⁹^ORCID,Kasahara Y.¹⁰^ORCID,Matsuoka A.¹¹,Shoji M.¹^ORCID,Teramoto M.¹²^ORCID,Lester M.¹³^ORCID

Affiliation:

1. Institute for Space‐Earth Environmental Research Nagoya University Nagoya Japan

2. Space Physics and Astronomy Research Unit University of Oulu Oulu Finland

3. National Institute of Polar Research Tachikawa Japan

4. Finnish Meteorological Institute Helsinki Finland

5. Sodankylä Geophysical Observatory University of Oulu Oulu Finland

6. Space and Plasma Physics, School of Electrical Engineering and Computer Science KTH Royal Institute of Technology Stockholm Sweden

7. Department of Computer and Network Engineering The University of Electro‐Communications Chofu Japan

8. Polar Geophysical Institute Apatity Russia

9. Graduate School of Science Tohoku University Sendai Japan

10. Graduate School of Natural Science and Technology Kanazawa University Kanazawa Japan

11. Kyoto University Kyoto Japan

12. Department of Space Systems Engineering Kyushu Institute of Technology Kitakyushu Japan

13. Department of Physics and Astronomy University of Leicester Leicester UK

Funder

Academy of Finland

Japan Society for the Promotion of Science London

Science and Technology Facilities Council

Russian Foundation for Basic Research

Canadian Space Agency

Energy Consumers Australia

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JA028468

Reference48 articles.

1. Accuracy of using 6300 Å auroral emission to identify the magnetic separatrix on the nightside of Earth

2. Interplanetary magnetic field control of afternoon-sector detached proton auroral arcs

3. Thermally excited 630.0 nm O( 1 D ) emission in the cusp: A frequent high‐altitude transient signature

4. An ISEE/whistler model of equatorial electron density in the magnetosphere

5. Identifying STEVE's Magnetospheric Driver Using Conjugate Observations in the Magnetosphere and on the Ground

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1. Post-midnight purple arc and patches appeared on the high latitude part of the auroral oval: Dawnside counterpart of STEVE?;Earth, Planets and Space;2024-04-09

2. Thermospheric wind response to a sudden ionospheric variation in the trough: event at a pseudo-breakup during geomagnetically quiet conditions;Earth, Planets and Space;2022-10-18

3. Interaction Between Proton Aurora and Stable Auroral Red Arcs Unveiled by Citizen Scientist Photographs;Journal of Geophysical Research: Space Physics;2022-07

4. Study of an Equatorward Detachment of Auroral Arc From the Oval Using Ground‐Space Observations and the BATS‐R‐US–CIMI Model;Journal of Geophysical Research: Space Physics;2021-12

5. Determination of the Enhancement in Electron Temperature in the Subauroral Ionosphere during Magnetic Storms on a Global Scale;Geomagnetism and Aeronomy;2021-12

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