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": "d747f40b-964f-4935-ad97-72d052844f26"}, "_deposit": {"id": "20405", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "20405"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00020405", "sets": []}, "author_link": ["59414"], "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": "1979-03", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "52", "bibliographicPageStart": "35", "bibliographicVolumeNumber": "26", "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": "A search for 5-min oscillation was performed using the data of solar total flux at four different microwave frequencies taken in the period August, 1977 through July, 1978 on the full automatic polarimeters at Toyokawa. Spectral analysis of about 600 hours of data showed that there are no periodic components with statistical significance (\u003e 95% confidence) in the fluctuation of the flux. Upper limits of the oscillating amplitude at the period of 300 sec are 2.7, 5.1, 13, and 53 K at 9.4, 3.75, 2.0, and 1.0 GHz respectively. Correlations between the parameters of fluctuating power of total flux and solar activity were also investigated. When solar activity is very high, spectral power increases particularly at lower frequency range (1 - 5 mHz).", "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/2237/22280"}]}, "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": "MORITA, Koh-ichiro", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "59414", "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": "2018-02-21"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "proria_26_35.pdf", "filesize": [{"value": "2.5 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 2500000.0, "url": {"label": "proria_26_35.pdf", "objectType": "fulltext", "url": "https://nagoya.repo.nii.ac.jp/record/20405/files/proria_26_35.pdf"}, "version_id": "1c747a51-72ec-4688-9bbd-e59386e9b30d"}]}, "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": "A SEARCH FOR 5-MIN OSCILLATION IN TOTAL MICROWAVE FLUX OF THE SUN OBSERVED AT TOYOKAWA", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "A SEARCH FOR 5-MIN OSCILLATION IN TOTAL MICROWAVE FLUX OF THE SUN OBSERVED AT TOYOKAWA", "subitem_title_language": "en"}]}, "item_type_id": "9", "owner": "1", "path": ["1757"], "permalink_uri": "http://hdl.handle.net/2237/22280", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2015-06-04"}, "publish_date": "2015-06-04", "publish_status": "0", "recid": "20405", "relation": {}, "relation_version_is_last": true, "title": ["A SEARCH FOR 5-MIN OSCILLATION IN TOTAL MICROWAVE FLUX OF THE SUN OBSERVED AT TOYOKAWA"], "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. 26

A SEARCH FOR 5-MIN OSCILLATION IN TOTAL MICROWAVE FLUX OF THE SUN OBSERVED AT TOYOKAWA

http://hdl.handle.net/2237/22280
http://hdl.handle.net/2237/22280
ce03aaf2-4324-4871-b95b-1a997ba7d755
名前 / ファイル ライセンス アクション
proria_26_35.pdf proria_26_35.pdf (2.5 MB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2015-06-04
タイトル
タイトル A SEARCH FOR 5-MIN OSCILLATION IN TOTAL MICROWAVE FLUX OF THE SUN OBSERVED AT TOYOKAWA
言語 en
著者 MORITA, Koh-ichiro

× MORITA, Koh-ichiro

WEKO 59414

en MORITA, Koh-ichiro

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 A search for 5-min oscillation was performed using the data of solar total flux at four different microwave frequencies taken in the period August, 1977 through July, 1978 on the full automatic polarimeters at Toyokawa. Spectral analysis of about 600 hours of data showed that there are no periodic components with statistical significance (> 95% confidence) in the fluctuation of the flux. Upper limits of the oscillating amplitude at the period of 300 sec are 2.7, 5.1, 13, and 53 K at 9.4, 3.75, 2.0, and 1.0 GHz respectively. Correlations between the parameters of fluctuating power of total flux and solar activity were also investigated. When solar activity is very high, spectral power increases particularly at lower frequency range (1 - 5 mHz).
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 26, p. 35-52, 発行日 1979-03
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/22280
識別子タイプ HDL
戻る
0
views
See details
Views

Versions

Ver.1 2021-03-01 15:49:46.896615
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