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  1. H300 宇宙地球環境研究所
  2. H300a 雑誌掲載論文
  3. 学術雑誌

Possible generation mechanisms for Pc1 pearl structures in the ionosphere based on 6 years of ground observations in Canada, Russia, and Japan

http://hdl.handle.net/2237/25071
http://hdl.handle.net/2237/25071
79618b45-15c7-44fd-962d-d067ed95be9e
名前 / ファイル ライセンス アクション
Jun_et_al-2016-Journal_of_Geophysical_Research_Space_Physics.pdf Jun_et_al-2016-Journal_of_Geophysical_Research_Space_Physics.pdf (2.9 MB)
アイテムタイプ 学術雑誌論文 / Journal Article(1)
公開日 2016-11-21
タイトル
タイトル Possible generation mechanisms for Pc1 pearl structures in the ionosphere based on 6 years of ground observations in Canada, Russia, and Japan
言語 en
著者 Chae-Woo, Jun

× Chae-Woo, Jun

WEKO 67337

en Chae-Woo, Jun

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Shiokawa, Kazuo

× Shiokawa, Kazuo

WEKO 67338

en Shiokawa, Kazuo

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Connors, Martin

× Connors, Martin

WEKO 67339

en Connors, Martin

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Schofield, Ian

× Schofield, Ian

WEKO 67340

en Schofield, Ian

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Poddelsky, Igor

× Poddelsky, Igor

WEKO 67341

en Poddelsky, Igor

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Shevtsov, Boris

× Shevtsov, Boris

WEKO 67342

en Shevtsov, Boris

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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
権利情報 © 2016 American Geophysical Union
言語 en
抄録
内容記述タイプ Abstract
内容記述 We investigate pearl structures (amplitude modulations) of Pc1 pulsations simultaneously observed at Athabasca (ATH, 54.7°N, 246.7°E, L = 4.3) in Canada, Magadan (MGD, 60.1°N, 150.7°E, L = 2.6) in Russia, and Moshiri (MOS, 44.4°N, 142.3°E, L = 1.5) in Japan. From 6 years of ground observations, from 2008 to 2013, we selected 84 Pc1 events observed simultaneously at the longitudinally separated stations (ATH and MGD) and 370 events observed at the latitudinally separated stations (MGD and MOS), all with high coherence (>0.7) of Pc1 waveforms. We calculated the cross-correlation coefficient (similarity: r) for the Pc1 pearl structures and found that more than half of the events in both pairs had low similarity (r < 0.7), indicating that most Pc1 waves exhibit different pearl structures at different stations. We found that high-similarity Pc1 pearl structures (r > 0.7) at the longitudinally separated stations are concentrated from 6 to 15 UT when both stations are in the nighttime. The similarity of Pc1 pearl structures tends to show a negative correlation with the standard deviation of the polarization angle in both pairs. The observed repetition period of Pc1 pearl structures has a clear positive correlation with the repetition period estimated from Pc1 bandwidth by assuming beating of different frequencies. From these results, we suggest that ionospheric beating effect could be a dominant process for the generation of Pc1 pearl structures. Beating processes in the ionosphere with a spatially distributed ionospheric source can cause the different shapes of Pc1 pearl structures at different observation points during ionospheric duct propagation.
言語 en
出版者
出版者 Wiley
言語 en
言語
言語 eng
資源タイプ
資源タイプresource http://purl.org/coar/resource_type/c_6501
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
DOI
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.1002/2015JA022123
ISSN
収録物識別子タイプ EISSN
収録物識別子 2169-9402
書誌情報 en : JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS

巻 121, 号 5, p. 4409-4424, 発行日 2016-05-21
著者版フラグ
値 publisher
URI
識別子 http://doi.org/10.1002/2015JA022123
識別子タイプ DOI
URI
識別子 http://hdl.handle.net/2237/25071
識別子タイプ HDL
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