| Item type |
itemtype_ver1(1) |
| 公開日 |
2021-10-15 |
| タイトル |
|
|
タイトル |
The Extreme Space Weather Event in 1941 February/March |
|
言語 |
en |
| 著者 |
Hayakawa, Hisashi
Blake, Sean P.
Bhaskar, Ankush
Hattori, Kentaro
Oliveira, Denny M.
Ebihara, Yusuke
|
| アクセス権 |
|
|
アクセス権 |
open access |
|
アクセス権URI |
http://purl.org/coar/access_right/c_abf2 |
| 権利 |
|
|
言語 |
en |
|
権利情報 |
© 2021. The American Astronomical Society |
| キーワード |
|
|
主題Scheme |
Other |
|
主題 |
Solar-terrestrial interactions |
| キーワード |
|
|
主題Scheme |
Other |
|
主題 |
Sunspots |
| キーワード |
|
|
主題Scheme |
Other |
|
主題 |
Solar flares |
| キーワード |
|
|
主題Scheme |
Other |
|
主題 |
Solar coronal mass ejections |
| キーワード |
|
|
主題Scheme |
Other |
|
主題 |
Geomagnetic fields |
| キーワード |
|
|
主題Scheme |
Other |
|
主題 |
Solar active regions |
| 内容記述 |
|
|
内容記述タイプ |
Abstract |
|
内容記述 |
Given the infrequency of extreme geomagnetic storms, it is significant to note the concentration of three extreme geomagnetic storms in 1941, whose intensities ranked fourth, twelfth, and fifth within the aa index between 1868–2010. Among them, the geomagnetic storm on 1941 March 1 was so intense that three of the four Dst station magnetograms went off scale. Herein, we reconstruct its time series and measure the storm intensity with an alternative Dst estimate (Dst*). The source solar eruption at 09:29–09:38 GMT on February 28 was located at RGO AR 13814 and its significant intensity is confirmed by large magnetic crochets of ∣35∣ nT measured at Abinger. This solar eruption most likely released a fast interplanetary coronal mass ejection with estimated speed 2260 km s^−1. After its impact at 03:57–03:59 GMT on March 1, an extreme magnetic storm was recorded worldwide. Comparative analyses on the contemporary magnetograms show the storm peak intensity of minimum Dst* ≤ −464 nT at 16 GMT, comparable to the most and the second most extreme magnetic storms within the standard Dst index since 1957. This storm triggered significant low-latitude aurorae in the East Asian sector and their equatorward boundary has been reconstructed as 38fdg5 in invariant latitude. This result agrees with British magnetograms, which indicate an auroral oval moving above Abinger at 53fdg0 in magnetic latitude. The storm amplitude was even more enhanced in equatorial stations and consequently casts caveats on their usage for measurements of the storm intensity in Dst estimates. |
|
言語 |
en |
| 出版者 |
|
|
出版者 |
IOP publishing |
|
言語 |
en |
| 言語 |
|
|
言語 |
eng |
| 資源タイプ |
|
|
資源タイプ識別子 |
http://purl.org/coar/resource_type/c_6501 |
|
資源タイプ |
journal article |
| 出版タイプ |
|
|
出版タイプ |
VoR |
|
出版タイプResource |
http://purl.org/coar/version/c_970fb48d4fbd8a85 |
| 関連情報 |
|
|
関連タイプ |
isVersionOf |
|
|
識別子タイプ |
DOI |
|
|
関連識別子 |
https://doi.org/10.3847/1538-4357/abb772 |
| 収録物識別子 |
|
|
収録物識別子タイプ |
EISSN |
|
収録物識別子 |
1538-4357 |
| 書誌情報 |
en : The Astrophysical Journal
巻 908,
号 2,
p. 209,
発行日 2021-02-20
|
Hayakawa_2021_ApJ_908_209.pdf (942 KB)
