Swarm Satellite and EISCAT Radar Observations of a Plasma Flow Channel in the Auroral Oval Near Magnetic Midnight-Reference-Cited by-同舟云学术

Swarm Satellite and EISCAT Radar Observations of a Plasma Flow Channel in the Auroral Oval Near Magnetic Midnight

Published:2018-06 Issue:6 Volume:123 Page:5140-5158
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Aikio A. T.¹^ORCID,Vanhamäki H.¹²^ORCID,Workayehu A. B.¹^ORCID,Virtanen I. I.¹^ORCID,Kauristie K.³^ORCID,Juusola L.³^ORCID,Buchert S.⁴^ORCID,Knudsen D.⁵^ORCID

Affiliation:

1. Ionospheric Physics Unit; University of Oulu; Oulu Finland

2. International Center for Space Weather Science and Education; Kyushu University; Fukuoka Japan

3. Finnish Meteorological Institute; Helsinki Finland

4. Swedish Institute of Space Physics; Uppsala Sweden

5. Department of Physics and Astronomy; University of Calgary; Calgary Alberta Canada

Funder

China

Varsinais-Suomen Sairaanhoitopiiri

Japan

Norway

Sweden

United Kingdom

Canadian Space Agency

Academy of Finland

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2018JA025409/fullpdf

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5. Method to locate the polar cap boundary in the nightside ionosphere and application to a substorm event;Aikio;Annales Geophysicae,2006

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