WEKO3
アイテム
{"_buckets": {"deposit": "28d4f4a0-1e6b-4196-8e0c-a2df71518ef0"}, "_deposit": {"created_by": 3, "id": "10477", "owners": [3], "pid": {"revision_id": 0, "type": "depid", "value": "10477"}, "status": "published"}, "_oai": {"id": "oai:nifs-repository.repo.nii.ac.jp:00010477", "sets": ["32"]}, "author_link": ["66181", "66179", "66182", "66180"], "item_5_biblio_info_7": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2003-12-01", "bibliographicIssueDateType": "Issued"}, "bibliographic_titles": [{}, {"bibliographic_title": "Research Report NIFS-Series", "bibliographic_titleLang": "en"}]}]}, "item_5_description_5": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "\"Characteristics of electrically-conducting media are reviewed from the macroscopic viewpoint based on the mean-field magnetohydrodynamics, while being compared with the methodology and knowledge in fluid mechanics. The themes covered in this review range from the generation mechanism of stellar magnetic fields (dynamo) to transport properties in fusion. The primary concern here is to see the characteristics common to these apparently different phenomena, within the framework of the mean-field theory. Owing to the intrinsic limitation of the approach, the present discussions are limited more or less to specific aspects of phenomena. They are supplemented with the reference to theoretical, numerical, and observational approaches intrinsic to each theme. In the description of dynamo phenomena, an emphasis is put on the cross-helicity dynamo. Features common to the stellar magnetic-field generation and the rotational-motion drive in toroidal plasmas are illustrated on this basis.\"", "subitem_description_type": "Abstract"}]}, "item_5_source_id_10": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0915-633X", "subitem_source_identifier_type": "ISSN"}]}, "item_5_text_25": {"attribute_name": "登録情報", "attribute_value_mlt": [{"subitem_text_value": "Made available in DSpace on 2010-02-05T10:16:37Z (GMT). No. of bitstreams: 0\n Previous issue date: 2003-12"}]}, "item_5_text_8": {"attribute_name": "報告書番号", "attribute_value_mlt": [{"subitem_text_value": "NIFS-788"}]}, "item_access_right": {"attribute_name": "アクセス権", "attribute_value_mlt": [{"subitem_access_right": "metadata only access", "subitem_access_right_uri": "http://purl.org/coar/access_right/c_14cb"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "\"Yoshizawa, A.", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "66179", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Itoh, S.-I.", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "66180", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Itoh, K.", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "66181", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Yokoi, N.\"", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "66182", "nameIdentifierScheme": "WEKO"}]}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "Dynamo", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "stellar magnetic field", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "stellar jet", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "accretion disk", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "turbulence suppression", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "mean-field MHD", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "turbulence", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "renormalization", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "structure formation", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "helicity", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "cross-helicity", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}]}, "item_language": {"attribute_name": "言語", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "資源タイプ", "attribute_value_mlt": [{"resourcetype": "research report", "resourceuri": "http://purl.org/coar/resource_type/c_18ws"}]}, "item_title": "Dynamos and MHD Theory of Turbulence Suppression", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Dynamos and MHD Theory of Turbulence Suppression", "subitem_title_language": "en"}]}, "item_type_id": "5", "owner": "3", "path": ["32"], "permalink_uri": "http://hdl.handle.net/10655/2453", "pubdate": {"attribute_name": "公開日", "attribute_value": "2010-02-05"}, "publish_date": "2010-02-05", "publish_status": "0", "recid": "10477", "relation": {}, "relation_version_is_last": true, "title": ["Dynamos and MHD Theory of Turbulence Suppression"], "weko_shared_id": -1}
Dynamos and MHD Theory of Turbulence Suppression
http://hdl.handle.net/10655/2453
http://hdl.handle.net/10655/24536122d966-30e1-4c2e-b8ab-191ddf3ecbb1
Item type | 研究報告書 / Research Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2010-02-05 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Dynamos and MHD Theory of Turbulence Suppression | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Dynamo | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | stellar magnetic field | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | stellar jet | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | accretion disk | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | turbulence suppression | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | mean-field MHD | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | turbulence | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | renormalization | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | structure formation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | helicity | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | cross-helicity | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_18ws | |||||
資源タイプ | research report | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
"Yoshizawa, A.
× "Yoshizawa, A.× Itoh, S.-I.× Itoh, K.× Yokoi, N." |
|||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | "Characteristics of electrically-conducting media are reviewed from the macroscopic viewpoint based on the mean-field magnetohydrodynamics, while being compared with the methodology and knowledge in fluid mechanics. The themes covered in this review range from the generation mechanism of stellar magnetic fields (dynamo) to transport properties in fusion. The primary concern here is to see the characteristics common to these apparently different phenomena, within the framework of the mean-field theory. Owing to the intrinsic limitation of the approach, the present discussions are limited more or less to specific aspects of phenomena. They are supplemented with the reference to theoretical, numerical, and observational approaches intrinsic to each theme. In the description of dynamo phenomena, an emphasis is put on the cross-helicity dynamo. Features common to the stellar magnetic-field generation and the rotational-motion drive in toroidal plasmas are illustrated on this basis." | |||||
書誌情報 |
en : Research Report NIFS-Series 発行日 2003-12-01 |
|||||
報告書番号 | ||||||
NIFS-788 | ||||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0915-633X |