Possible Cause of Extremely Bright Aurora Witnessed in East Asia on 17 September 1770-Reference-Cited by-同舟云学术

Possible Cause of Extremely Bright Aurora Witnessed in East Asia on 17 September 1770

Published:2017-10 Issue:10 Volume:15 Page:1373-1382
ISSN:1542-7390
Container-title:Space Weather
language:en
Short-container-title:Space Weather

Author:

Ebihara Yusuke¹²^ORCID,Hayakawa Hisashi³⁴^ORCID,Iwahashi Kiyomi⁵,Tamazawa Harufumi⁶,Kawamura Akito Davis⁶,Isobe Hiroaki²⁷

Affiliation:

1. Research Institute for Sustainable Humanosphere; Kyoto University; Kyoto Japan

2. Unit of Synergetic Studies for Space; Kyoto University; Kyoto Japan

3. Graduate School of Letters; Osaka University; Toyonaka Japan

4. JSPS Research Fellow; Tokyo Japan

5. National Institute of Japanese Literature; Tachikawa Japan

6. Kwasan Observatory; Kyoto University; Kyoto Japan

7. Graduate School of Advanced Integrated Studies in Human Survivability; Kyoto University; Kyoto Japan

Funder

Japan Society for the Promotion of Science London

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2017SW001693/fullpdf

Reference46 articles.

1. Chamberlain , J. W. 1961 Physics of the aurora and Airglow, pp. 124-125 https://doi.org/10.1029/SP041

2. The CIE 1931 V(λ) data were modified by D. B. Judd and J. J. Vos in 1978. The Judd−Vos-modified eye sensitivity function is frequently referred to as VM(λ); see J. J. Vos “Colorimetric and photometric properties of a 2-deg fundamental observer”;CIE data of 1931 Retrieved from http://cvision.ucsd.edu and http://www.cvrl.org;Color Research and Application,1978

3. The 1859 space weather event revisited: Limits of extreme activity;Cliver;Journal of Space Weather and Space Climate,2013

4. The 1859 solar-terrestrial disturbance And the current limits of extreme space weather activity;Cliver;Solar Physics,2004

5. Bulk plasma properties at geosynchronous orbit;Denton;Journal of Geophysical Research,2005

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