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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

Radial Speed Evolution of Interplanetary Coronal Mass Ejections During Solar Cycle 23

http://hdl.handle.net/2237/19929
http://hdl.handle.net/2237/19929
9a03aa9a-4037-47ed-8a47-ccf6e507f384
名前 / ファイル ライセンス アクション
Iju_manuscript_solarphysics.pdf Iju_manuscript_solarphysics.pdf (894.1 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2014-05-07
タイトル
タイトル Radial Speed Evolution of Interplanetary Coronal Mass Ejections During Solar Cycle 23
言語 en
著者 Iju, T.

× Iju, T.

WEKO 52241

en Iju, T.

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Tokumaru, M.

× Tokumaru, M.

WEKO 52242

en Tokumaru, M.

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Fujiki, K.

× Fujiki, K.

WEKO 52243

en Fujiki, K.

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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
言語 en
権利情報 The final publication is available at Springer via http://dx.doi.org/10.1007/s11207-013-0297-5
キーワード
主題Scheme Other
主題 Coronal mass ejections
キーワード
主題Scheme Other
主題 Initiation and propagation
キーワード
主題Scheme Other
主題 Coronal mass ejections
キーワード
主題Scheme Other
主題 Interplanetary
キーワード
主題Scheme Other
主題 Plasma physics
キーワード
主題Scheme Other
主題 Radio scintillation
抄録
内容記述タイプ Abstract
内容記述 We report radial-speed evolution of interplanetary coronal mass ejections (ICMEs) detected by the Large Angle and Spectrometric Coronagraph onboard the Solar and Heliospheric Observatory (SOHO/LASCO), interplanetary scintillation (IPS) at 327 MHz, and in-situ observations. We analyze solar-wind disturbance factor (g-value) data derived from IPS observations during 1997 – 2009 covering nearly the whole period of Solar Cycle 23. By comparing observations from SOHO/LASCO, IPS, and in situ, we identify 39 ICMEs that could be analyzed carefully. Here, we define two speeds [V SOHO and V bg], which are the initial speed of the ICME and the speed of the background solar wind, respectively. Examinations of these speeds yield the following results: i) Fast ICMEs (with V SOHO−V bg>500 km s−1) rapidly decelerate, moderate ICMEs (with 0 km s−1≤V SOHO−V bg≤500 km s−1) show either gradually decelerating or uniform motion, and slow ICMEs (with V SOHO−V bg<0 km s−1) accelerate. The radial speeds converge on the speed of the background solar wind during their outward propagation. We subsequently find; ii) both the acceleration and the deceleration are nearly complete by 0.79±0.04 AU, and those are ended when the ICMEs reach a 480±21 km s−1. iii) For ICMEs with (V SOHO−V bg)≥0 km s−1, i.e. fast and moderate ICMEs, a linear equation a=−γ 1(V−V bg) with γ 1=6.58±0.23×10−6 s−1 is more appropriate than a quadratic equation a=−γ 2(V−V bg)|V−V bg| to describe their kinematics, where γ 1 and γ 2 are coefficients, and a and V are the acceleration and speed of ICMEs, respectively, because the χ 2 for the linear equation satisfies the statistical significance level of 0.05, while the quadratic one does not. These results support the assumption that the radial motion of ICMEs is governed by a drag force due to interaction with the background solar wind. These findings also suggest that ICMEs propagating faster than the background solar wind are controlled mainly by the hydrodynamic Stokes drag.
言語 en
内容記述
内容記述タイプ Other
内容記述 Published online: 26 April 2013
言語 en
出版者
出版者 Springer
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 AM
出版タイプResource http://purl.org/coar/version/c_ab4af688f83e57aa
DOI
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.1007/s11207-013-0297-5
ISSN
収録物識別子タイプ PISSN
収録物識別子 0038-0938
書誌情報 en : Solar Physics

巻 288, 号 1, p. 331-353, 発行日 2013-11
著者版フラグ
値 author
URI
識別子 http://dx.doi.org/10.1007/s11207-013-0297-5
識別子タイプ DOI
URI
識別子 http://hdl.handle.net/2237/19929
識別子タイプ HDL
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