ログイン
言語:

WEKO3

  • トップ
  • ランキング
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": "d791bb18-c3c4-41cb-8657-491dba46b22e"}, "_deposit": {"id": "20189", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "20189"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00020189", "sets": []}, "author_link": ["58983", "58984"], "item_1615768549627": {"attribute_name": "出版タイプ", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_970fb48d4fbd8a85", "subitem_version_type": "VoR"}]}, "item_9_biblio_info_6": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "1986-03-25", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "18", "bibliographicPageStart": "1", "bibliographicVolumeNumber": "33", "bibliographic_titles": [{"bibliographic_title": "Proceedings of the Research Institute of Atmospherics, Nagoya University", "bibliographic_titleLang": "en"}]}]}, "item_9_description_4": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "Long-term evolution of the solar wind structure in the heliographic longitude and latitude was studied on the basis of observations of interplanetary scintillation. The evolution from 1983 to 1985 was studied using two-dimensional solar wind maps. These were made with a new mapping method developed to investigate the structure of solar wind in detail. In this period of low solar activity, the lowspeed regions are distributed along the wavy neutral sheet made by the magnetic dipole and quadrupole field. The higher-speed regions were more fully developed in the northern hemisphere than in the southern hemisphere. Large latitudinal gradients of speed were developed at the latitude where the high speed region extended. Breadth of the low speed region decreased with subsiding solar activity. Two localized minimum-speed regions appeared on the neutral sheet and their locations coincide with those of the two giant bipolar magnetic regions. These two minimum-speed regions are longitudinally separated almost by 180°.", "subitem_description_language": "en", "subitem_description_type": "Abstract"}]}, "item_9_identifier_60": {"attribute_name": "URI", "attribute_value_mlt": [{"subitem_identifier_type": "HDL", "subitem_identifier_uri": "http://hdl.handle.net/2237/22103"}]}, "item_9_publisher_32": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "The Research Institute of Atmospherics, Nagoya University", "subitem_publisher_language": "en"}]}, "item_9_select_15": {"attribute_name": "著者版フラグ", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "item_9_source_id_7": {"attribute_name": "ISSN(print)", "attribute_value_mlt": [{"subitem_source_identifier": "0077-264X", "subitem_source_identifier_type": "PISSN"}]}, "item_access_right": {"attribute_name": "アクセス権", "attribute_value_mlt": [{"subitem_access_right": "open access", "subitem_access_right_uri": "http://purl.org/coar/access_right/c_abf2"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Kojima, Masayoshi", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "58983", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Kakinuma, Takakiyo", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "58984", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2017-05-10"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "proria_33_1.pdf", "filesize": [{"value": "3.2 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 3200000.0, "url": {"label": "proria_33_1.pdf", "objectType": "fulltext", "url": "https://nagoya.repo.nii.ac.jp/record/20189/files/proria_33_1.pdf"}, "version_id": "7cc456a7-185a-445e-a6f4-bc5584788ed8"}]}, "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": "departmental bulletin paper", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "THREE-STATION OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 327 MHz-II : EVOLUTION OF TWO-DIMENSIONAL SOLAR WIND SPEED STRUCTURE DURING 1983 TO 1985", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "THREE-STATION OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 327 MHz-II : EVOLUTION OF TWO-DIMENSIONAL SOLAR WIND SPEED STRUCTURE DURING 1983 TO 1985", "subitem_title_language": "en"}]}, "item_type_id": "9", "owner": "1", "path": ["1744"], "permalink_uri": "http://hdl.handle.net/2237/22103", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2015-05-29"}, "publish_date": "2015-05-29", "publish_status": "0", "recid": "20189", "relation": {}, "relation_version_is_last": true, "title": ["THREE-STATION OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 327 MHz-II : EVOLUTION OF TWO-DIMENSIONAL SOLAR WIND SPEED STRUCTURE DURING 1983 TO 1985"], "weko_shared_id": -1}
  1. F300 宇宙地球環境研究所
  2. F300b 紀要
  3. Proceedings of the Research Institute of Atmospherics, Nagoya University
  4. 33

THREE-STATION OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 327 MHz-II : EVOLUTION OF TWO-DIMENSIONAL SOLAR WIND SPEED STRUCTURE DURING 1983 TO 1985

http://hdl.handle.net/2237/22103
http://hdl.handle.net/2237/22103
7f740234-e8f3-45d8-a9a9-032502a93b5e
名前 / ファイル ライセンス アクション
proria_33_1.pdf proria_33_1.pdf (3.2 MB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2015-05-29
タイトル
タイトル THREE-STATION OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 327 MHz-II : EVOLUTION OF TWO-DIMENSIONAL SOLAR WIND SPEED STRUCTURE DURING 1983 TO 1985
言語 en
著者 Kojima, Masayoshi

× Kojima, Masayoshi

WEKO 58983

en Kojima, Masayoshi

Search repository
Kakinuma, Takakiyo

× Kakinuma, Takakiyo

WEKO 58984

en Kakinuma, Takakiyo

Search repository
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
抄録
内容記述 Long-term evolution of the solar wind structure in the heliographic longitude and latitude was studied on the basis of observations of interplanetary scintillation. The evolution from 1983 to 1985 was studied using two-dimensional solar wind maps. These were made with a new mapping method developed to investigate the structure of solar wind in detail. In this period of low solar activity, the lowspeed regions are distributed along the wavy neutral sheet made by the magnetic dipole and quadrupole field. The higher-speed regions were more fully developed in the northern hemisphere than in the southern hemisphere. Large latitudinal gradients of speed were developed at the latitude where the high speed region extended. Breadth of the low speed region decreased with subsiding solar activity. Two localized minimum-speed regions appeared on the neutral sheet and their locations coincide with those of the two giant bipolar magnetic regions. These two minimum-speed regions are longitudinally separated almost by 180°.
言語 en
内容記述タイプ Abstract
出版者
言語 en
出版者 The Research Institute of Atmospherics, Nagoya University
言語
言語 eng
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ departmental bulletin paper
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
ISSN(print)
収録物識別子タイプ PISSN
収録物識別子 0077-264X
書誌情報 en : Proceedings of the Research Institute of Atmospherics, Nagoya University

巻 33, p. 1-18, 発行日 1986-03-25
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/22103
識別子タイプ HDL
戻る
0
views
See details
Views

Versions

Ver.1 2021-03-01 15:54:58.385217
Show All versions

Share

Mendeley Twitter Facebook Print Addthis

Cite as

エクスポート

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

Confirm


Powered by WEKO3


Powered by WEKO3