{"_buckets": {"deposit": "27e52704-ed44-46f1-9f5d-00101dc77f94"}, "_deposit": {"id": "19535", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "19535"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00019535"}, "item_9_biblio_info_6": {"attribute_name": "\u66f8\u8a8c\u60c5\u5831", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "1956-01-30", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "109", "bibliographicPageStart": "102", "bibliographicVolumeNumber": "3", "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": "An 8-element interferometer with quarter-wavelength plates was completed in June, 1954. Each aerial has a paraboloidal reflector, 1.5 metre in diameter which can automatically follow the sun. Aerials are placed in E-W direction at 6.45 metres (86\u03bb) intervals. The main lobes are spaced 40\u0027 apart and have half-power widths of 4.5\u0027 around the local noon. Observations can be made for about five hours a day. Two dimensional location of radio spots is partially possible because the scanning direction gradually changes in a day except for the periods around the equinoxes. Quarter-wavelength plates are mounted over the paraboloidal reflectors and they can be driven simultaneously. They are so designed as to minimize the reflection. To improve the accuracy of measurement, a square-law detector is used and a hot load is prepared for daily calibrations.", "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/2237/21571"}]}, "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": "TANAKA, HARUO"}], "nameIdentifiers": [{"nameIdentifier": "57088", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "KAKINUMA, TAKAKIYO"}], "nameIdentifiers": [{"nameIdentifier": "57089", "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": "Vol3-11.pdf", "filesize": [{"value": "1.5 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 1500000.0, "url": {"label": "Vol3-11.pdf", "url": "https://nagoya.repo.nii.ac.jp/record/19535/files/Vol3-11.pdf"}, "version_id": "1cc7acc5-e61f-4b3e-9fce-7beeb33376d7"}]}, "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": "MULTIPLE ELEMENT INTERFEROMETER FOR LOCATING SOURCES OF SOLAR NOISE AT 4,000 MEGACYCLES (2)", "item_titles": {"attribute_name": "\u30bf\u30a4\u30c8\u30eb", "attribute_value_mlt": [{"subitem_title": "MULTIPLE ELEMENT INTERFEROMETER FOR LOCATING SOURCES OF SOLAR NOISE AT 4,000 MEGACYCLES (2)"}]}, "item_type_id": "9", "owner": "1", "path": ["879/1183/1640/1698"], "permalink_uri": "http://hdl.handle.net/2237/21571", "pubdate": {"attribute_name": "\u516c\u958b\u65e5", "attribute_name_i18n": "\u516c\u958b\u65e5", "attribute_value": "2015-04-16"}, "publish_date": "2015-04-16", "publish_status": "0", "recid": "19535", "relation": {}, "relation_version_is_last": true, "title": ["MULTIPLE ELEMENT INTERFEROMETER FOR LOCATING SOURCES OF SOLAR NOISE AT 4,000 MEGACYCLES (2)"], "weko_shared_id": null}