WEKO3
AND
アイテム
{"_buckets": {"deposit": "08e6b74a-01d9-4cdd-aad9-590294e9d640"}, "_deposit": {"id": "19605", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "19605"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00019605"}, "item_9_biblio_info_6": {"attribute_name": "\u66f8\u8a8c\u60c5\u5831", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "1958-03-25", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "80", "bibliographicPageStart": "71", "bibliographicVolumeNumber": "5", "bibliographic_titles": [{"bibliographic_title": "Proceedings of the Research Institute of Atmospherics, Nagoya University"}]}]}, "item_9_description_4": {"attribute_name": "\u6284\u9332", "attribute_value_mlt": [{"subitem_description": "The intensity and polarization of solar radio bursts have been observed at 9400, 3750, 2000 and 1000 Mc/s since July, 1957. In this paper the results of observations during 6 months are described. In most bursts at microwave frequencies, the difference in the intensity of two circularly polarized components is observed. At 3750 Mc/s, the bursts of small degree of polarization (less than 10%) are predominant, compared with other frequencies. At 2000 and 1000 Mc/s the circularly polarized bursts were occasionally observed, but not at 9400 and 3750 Mc/s and at 3750 Mc/s the linearly polarized components were not observed. In most bursts observed at four frequencies, the sense of polarization reverses near 3750 or 2000 Mc/s and the degree of polarization is generally small at 3750 Mc/s. At 9400 Mc/s, it seems that the sense of polarization correlates with the position of the source on the solar disk. Further observations will be continued to investigate the relation between them.", "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/2237/21652"}]}, "item_9_publisher_32": {"attribute_name": "\u51fa\u7248\u8005", "attribute_value_mlt": [{"subitem_publisher": "The Research Institute of Atmospherics, Nagoya University"}]}, "item_9_select_15": {"attribute_name": "\u8457\u8005\u7248\u30d5\u30e9\u30b0", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "item_9_source_id_7": {"attribute_name": "ISSN\uff08print\uff09", "attribute_value_mlt": [{"subitem_source_identifier": "0077-264X", "subitem_source_identifier_type": "ISSN"}]}, "item_creator": {"attribute_name": "\u8457\u8005", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "KAKINUMA, T."}], "nameIdentifiers": [{"nameIdentifier": "57258", "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": "2018-02-21"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "Vol5-8.pdf", "filesize": [{"value": "1.6 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 1600000.0, "url": {"label": "Vol5-8.pdf", "url": "https://nagoya.repo.nii.ac.jp/record/19605/files/Vol5-8.pdf"}, "version_id": "a892a810-96d9-494a-9368-ce1ecdd44a3a"}]}, "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": "departmental bulletin paper", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "POLARIZATION OF SOLAR RADIO BURSTS AT MICROWAVE FREQUENCIES I", "item_titles": {"attribute_name": "\u30bf\u30a4\u30c8\u30eb", "attribute_value_mlt": [{"subitem_title": "POLARIZATION OF SOLAR RADIO BURSTS AT MICROWAVE FREQUENCIES I"}]}, "item_type_id": "9", "owner": "1", "path": ["879/1183/1640/1703"], "permalink_uri": "http://hdl.handle.net/2237/21652", "pubdate": {"attribute_name": "\u516c\u958b\u65e5", "attribute_value": "2015-04-21"}, "publish_date": "2015-04-21", "publish_status": "0", "recid": "19605", "relation": {}, "relation_version_is_last": true, "title": ["POLARIZATION OF SOLAR RADIO BURSTS AT MICROWAVE FREQUENCIES I"], "weko_shared_id": null}
POLARIZATION OF SOLAR RADIO BURSTS AT MICROWAVE FREQUENCIES I
http://hdl.handle.net/2237/21652
a43d2d14-1b2b-4b25-be83-f1d090916f97
名前 / ファイル | ライセンス | アクション | |
---|---|---|---|
![]() |
|
Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-04-21 | |||||
タイトル | ||||||
タイトル | POLARIZATION OF SOLAR RADIO BURSTS AT MICROWAVE FREQUENCIES I | |||||
著者 |
KAKINUMA, T.
× KAKINUMA, T. |
|||||
抄録 | ||||||
内容記述 | The intensity and polarization of solar radio bursts have been observed at 9400, 3750, 2000 and 1000 Mc/s since July, 1957. In this paper the results of observations during 6 months are described. In most bursts at microwave frequencies, the difference in the intensity of two circularly polarized components is observed. At 3750 Mc/s, the bursts of small degree of polarization (less than 10%) are predominant, compared with other frequencies. At 2000 and 1000 Mc/s the circularly polarized bursts were occasionally observed, but not at 9400 and 3750 Mc/s and at 3750 Mc/s the linearly polarized components were not observed. In most bursts observed at four frequencies, the sense of polarization reverses near 3750 or 2000 Mc/s and the degree of polarization is generally small at 3750 Mc/s. At 9400 Mc/s, it seems that the sense of polarization correlates with the position of the source on the solar disk. Further observations will be continued to investigate the relation between them. | |||||
内容記述タイプ | Abstract | |||||
出版者 | ||||||
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 | |||||
ISSN(print) | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0077-264X | |||||
書誌情報 |
Proceedings of the Research Institute of Atmospherics, Nagoya University 巻 5, p. 71-80, 発行日 1958-03-25 |
|||||
著者版フラグ | ||||||
値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/21652 | |||||
識別子タイプ | HDL |