ログイン
言語:

WEKO3

  • トップ
  • コミュニティ
  • ランキング
AND
To
lat lon distance
To

Field does not validate



インデックスリンク

インデックスツリー

メールアドレスを入力してください。

WEKO

One fine body…

WEKO

One fine body…

アイテム

{"_buckets": {"deposit": "ca2574d7-13fc-462e-83b8-5b7a81453125"}, "_deposit": {"id": "10209", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "10209"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00010209"}, "item_10_biblio_info_6": {"attribute_name": "\u66f8\u8a8c\u60c5\u5831", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2008-09-16", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "9", "bibliographicPageEnd": "092305", "bibliographicPageStart": "092305", "bibliographicVolumeNumber": "15", "bibliographic_titles": [{"bibliographic_title": "PHYSICS OF PLASMAS"}]}]}, "item_10_description_4": {"attribute_name": "\u6284\u9332", "attribute_value_mlt": [{"subitem_description": "The study of heavy-ion acceleration by magnetosonic shock waves in multi-ion-species plasmas [M. Toida and Y. Ohsawa, Solar Physics 171, 161 (1997)] is extended to the case in which the ion masses are of the same order of magnitude; specifically, the effect of mass and density ratios is examined for H-T and D-T plasmas with three-dimensional, electromagnetic, particle simulations. The frequency difference \u0394_\u03c9, where \u0394_\u03c9=(\u03c9_+0\u2212\u03c9_\u2212r)/\u03c9_+0 with \u03c9_+0 the cut-off frequency of the high-frequency magnetosonic mode and \u03c9_\u2212r the resonance frequency of the low-frequency mode, is \na key parameter in the generation of shock waves from a disturbance. In H-T plasmas with\n n_H\u003c\u003cn_T and with n_H\u003e\u003en_T and in D-T plasmas with any density ratio, \u0394_\u03c9 is small, and the\n high-frequency-mode shock wave is mainly generated and plays a central role in ion energization processes. In H-T plasmas with n_H=n_T, for which \u0394\u03c9\u3000is much greater, both the high- and low-frequency-mode shock waves are generated and contribute to the acceleration.", "subitem_description_type": "Abstract"}]}, "item_10_identifier_60": {"attribute_name": "URI", "attribute_value_mlt": [{"subitem_identifier_type": "DOI", "subitem_identifier_uri": "http://dx.doi.org/10.1063/1.2977481"}, {"subitem_identifier_type": "HDL", "subitem_identifier_uri": "http://hdl.handle.net/2237/12029"}]}, "item_10_publisher_32": {"attribute_name": "\u51fa\u7248\u8005", "attribute_value_mlt": [{"subitem_publisher": "American Institite of Physics"}]}, "item_10_rights_12": {"attribute_name": "\u6a29\u5229", "attribute_value_mlt": [{"subitem_rights": "Copyright (2008) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics."}]}, "item_10_select_15": {"attribute_name": "\u8457\u8005\u7248\u30d5\u30e9\u30b0", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "item_10_source_id_7": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "1070-664X", "subitem_source_identifier_type": "ISSN"}]}, "item_10_text_14": {"attribute_name": "\u30d5\u30a9\u30fc\u30de\u30c3\u30c8", "attribute_value_mlt": [{"subitem_text_value": "application/pdf"}]}, "item_creator": {"attribute_name": "\u8457\u8005", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Toida, Mieko"}], "nameIdentifiers": [{"nameIdentifier": "30896", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Higashino, Hiroyuki"}], "nameIdentifiers": [{"nameIdentifier": "30897", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Ohsawa, Yukiharu"}], "nameIdentifiers": [{"nameIdentifier": "30898", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "\u30d5\u30a1\u30a4\u30eb\u60c5\u5831", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2018-02-20"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "PhysPlasmas_15_092305.pdf", "filesize": [{"value": "8.7 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 8700000.0, "url": {"label": "PhysPlasmas_15_092305.pdf", "url": "https://nagoya.repo.nii.ac.jp/record/10209/files/PhysPlasmas_15_092305.pdf"}, "version_id": "c5d2226a-2306-4154-bc27-d68f4a4db656"}]}, "item_language": {"attribute_name": "\u8a00\u8a9e", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "\u8cc7\u6e90\u30bf\u30a4\u30d7", "attribute_value_mlt": [{"resourcetype": "journal article", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "Effect of ion composition on ion acceleration by magnetosonic shock waves", "item_titles": {"attribute_name": "\u30bf\u30a4\u30c8\u30eb", "attribute_value_mlt": [{"subitem_title": "Effect of ion composition on ion acceleration by magnetosonic shock waves"}]}, "item_type_id": "10", "owner": "1", "path": ["336/695/696"], "permalink_uri": "http://hdl.handle.net/2237/12029", "pubdate": {"attribute_name": "\u516c\u958b\u65e5", "attribute_value": "2009-08-07"}, "publish_date": "2009-08-07", "publish_status": "0", "recid": "10209", "relation": {}, "relation_version_is_last": true, "title": ["Effect of ion composition on ion acceleration by magnetosonic shock waves"], "weko_shared_id": null}
  1. B100 理学部/理学研究科
  2. B100a 雑誌掲載論文
  3. 学術雑誌

Effect of ion composition on ion acceleration by magnetosonic shock waves

http://hdl.handle.net/2237/12029
856e9dba-bf87-4313-93ed-cd4cc08157bf
名前 / ファイル ライセンス アクション
PhysPlasmas_15_092305.pdf PhysPlasmas_15_092305.pdf (8.7 MB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2009-08-07
タイトル
タイトル Effect of ion composition on ion acceleration by magnetosonic shock waves
著者 Toida, Mieko

× Toida, Mieko

WEKO 30896

Toida, Mieko

Search repository
Higashino, Hiroyuki

× Higashino, Hiroyuki

WEKO 30897

Higashino, Hiroyuki

Search repository
Ohsawa, Yukiharu

× Ohsawa, Yukiharu

WEKO 30898

Ohsawa, Yukiharu

Search repository
権利
権利情報 Copyright (2008) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.
抄録
内容記述 The study of heavy-ion acceleration by magnetosonic shock waves in multi-ion-species plasmas [M. Toida and Y. Ohsawa, Solar Physics 171, 161 (1997)] is extended to the case in which the ion masses are of the same order of magnitude; specifically, the effect of mass and density ratios is examined for H-T and D-T plasmas with three-dimensional, electromagnetic, particle simulations. The frequency difference Δ_ω, where Δ_ω=(ω_+0−ω_−r)/ω_+0 with ω_+0 the cut-off frequency of the high-frequency magnetosonic mode and ω_−r the resonance frequency of the low-frequency mode, is
a key parameter in the generation of shock waves from a disturbance. In H-T plasmas with
n_H<<n_T and with n_H>>n_T and in D-T plasmas with any density ratio, Δ_ω is small, and the
high-frequency-mode shock wave is mainly generated and plays a central role in ion energization processes. In H-T plasmas with n_H=n_T, for which Δω is much greater, both the high- and low-frequency-mode shock waves are generated and contribute to the acceleration.
内容記述タイプ Abstract
出版者
出版者 American Institite of Physics
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
ISSN
収録物識別子タイプ ISSN
収録物識別子 1070-664X
書誌情報 PHYSICS OF PLASMAS

巻 15, 号 9, p. 092305-092305, 発行日 2008-09-16
フォーマット
application/pdf
著者版フラグ
値 publisher
URI
識別子 http://dx.doi.org/10.1063/1.2977481
識別子タイプ DOI
URI
識別子 http://hdl.handle.net/2237/12029
識別子タイプ HDL
戻る
0
views
See details
Views

Versions

Ver.1 2021-03-01 19:34:12.557622
Show All versions

Share

Mendeley CiteULike Twitter Facebook Print Addthis

Cite as

Export

OAI-PMH
  • OAI-PMH JPCOAR
  • OAI-PMH DublinCore
  • OAI-PMH DDI
Other Formats
  • JSON
  • BIBTEX

Confirm


Powered by CERN Data Centre & Invenio


Powered by CERN Data Centre & Invenio