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": "007a0b47-dfd0-4341-9336-e88fc3d8c5b2"}, "_deposit": {"created_by": 17, "id": "2002051", "owner": "17", "owners": [17], "owners_ext": {"displayname": "図書情報係", "username": "repository"}, "pid": {"revision_id": 0, "type": "depid", "value": "2002051"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:02002051", "sets": ["2028"]}, "author_link": [], "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_1629683748249": {"attribute_name": "日付", "attribute_value_mlt": [{"subitem_date_issued_datetime": "2022-02-08", "subitem_date_issued_type": "Available"}]}, "item_9_biblio_info_6": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2021-09-20", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "1", "bibliographicPageStart": "1", "bibliographicVolumeNumber": "919", "bibliographic_titles": [{"bibliographic_title": "The Astrophysical Journal", "bibliographic_titleLang": "en"}]}]}, "item_9_description_4": {"attribute_name": "内容記述", "attribute_value_mlt": [{"subitem_description": "In addition to regular Schwabe cycles (≈11 yr), solar variability also shows longer periods of enhanced or reduced activity. Of these, reconstructions of the Dalton Minimum provide controversial sunspot group numbers and limited sunspot positions, partially due to limited source record accessibility. In this context, we analyzed Stephan Prantner\u0027s sunspot observations spanning from 1804 to 1844, the values of which had only been known through estimates despite their notable chronological coverage during the Dalton Minimum. We identified his original manuscript in Stiftsarchiv Wilten, near Innsbruck (Austria). We reviewed his biography (1782–1873) and located his observational sites at Wilten and Waidring, which housed the principal telescopes for his early and late observations: a 3.5 inch astronomical telescope and a Reichenbach 4 foot achromatic erecting telescope, respectively. We identified 215 days of datable sunspot observations, which is almost twice as much data as his estimated data in the existing databases (=115 days). In Prantner\u0027s records, we counted up to seven to nine sunspot groups per day and measured sunspot positions, which show their distributions in both solar hemispheres. These results strikingly emphasize the difference between the Dalton Minimum and the Maunder Minimum as well as the similarity between the Dalton Minimum and the weak solar cycles in the modern observations.", "subitem_description_language": "en", "subitem_description_type": "Abstract"}]}, "item_9_publisher_32": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "IOP publishing", "subitem_publisher_language": "en"}]}, "item_9_relation_43": {"attribute_name": "関連情報", "attribute_value_mlt": [{"subitem_relation_type": "isVersionOf", "subitem_relation_type_id": {"subitem_relation_type_id_text": "https://doi.org/10.3847/1538-4357/abee1b", "subitem_relation_type_select": "DOI"}}]}, "item_9_rights_12": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "© 2021. The American Astronomical Society", "subitem_rights_language": "en"}]}, "item_9_source_id_7": {"attribute_name": "収録物識別子", "attribute_value_mlt": [{"subitem_source_identifier": "0004-637X", "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": "Hayakawa, Hisashi", "creatorNameLang": "en"}]}, {"creatorNames": [{"creatorName": "Uneme, Shoma", "creatorNameLang": "en"}]}, {"creatorNames": [{"creatorName": "Besser, Bruno P.", "creatorNameLang": "en"}]}, {"creatorNames": [{"creatorName": "Iju, Tomoya", "creatorNameLang": "en"}]}, {"creatorNames": [{"creatorName": "Imada, Shinsuke", "creatorNameLang": "en"}]}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_access", "date": [{"dateType": "Available", "dateValue": "2022-02-08"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "Hayakawa_2021_ApJ_919_1.pdf", "filesize": [{"value": "1.2 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "mimetype": "application/pdf", "size": 1200000.0, "url": {"objectType": "fulltext", "url": "https://nagoya.repo.nii.ac.jp/record/2002051/files/Hayakawa_2021_ApJ_919_1.pdf"}, "version_id": "4a44e6a3-3869-4fd5-bb13-676345aec88c"}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "Sunspots", "subitem_subject_scheme": "Other"}, {"subitem_subject": "Sunspot cycle", "subitem_subject_scheme": "Other"}, {"subitem_subject": "Sunspot groups", "subitem_subject_scheme": "Other"}, {"subitem_subject": "Solar-terrestrial interactions", "subitem_subject_scheme": "Other"}, {"subitem_subject": "Maunder minimum", "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": "journal article", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "Stephan Prantner’s Sunspot Observations during the Dalton Minimum", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Stephan Prantner’s Sunspot Observations during the Dalton Minimum", "subitem_title_language": "en"}]}, "item_type_id": "40001", "owner": "17", "path": ["2028"], "permalink_uri": "http://hdl.handle.net/2237/0002002051", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2022-02-08"}, "publish_date": "2022-02-08", "publish_status": "0", "recid": "2002051", "relation": {}, "relation_version_is_last": true, "title": ["Stephan Prantner’s Sunspot Observations during the Dalton Minimum"], "weko_shared_id": -1}
  1. I200 高等研究院
  2. I200a 雑誌掲載論文
  3. 学術雑誌

Stephan Prantner’s Sunspot Observations during the Dalton Minimum

http://hdl.handle.net/2237/0002002051
http://hdl.handle.net/2237/0002002051
46b7be07-c47a-4859-9a71-88017e6dbcb6
名前 / ファイル ライセンス アクション
Hayakawa_2021_ApJ_919_1.pdf Hayakawa_2021_ApJ_919_1.pdf (1.2 MB)
Item type itemtype_ver1(1)
公開日 2022-02-08
タイトル
タイトル Stephan Prantner’s Sunspot Observations during the Dalton Minimum
言語 en
著者 Hayakawa, Hisashi

× Hayakawa, Hisashi

en Hayakawa, Hisashi

Search repository
Uneme, Shoma

× Uneme, Shoma

en Uneme, Shoma

Search repository
Besser, Bruno P.

× Besser, Bruno P.

en Besser, Bruno P.

Search repository
Iju, Tomoya

× Iju, Tomoya

en Iju, Tomoya

Search repository
Imada, Shinsuke

× Imada, Shinsuke

en Imada, Shinsuke

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
権利
言語 en
権利情報 © 2021. The American Astronomical Society
キーワード
主題Scheme Other
主題 Sunspots
キーワード
主題Scheme Other
主題 Sunspot cycle
キーワード
主題Scheme Other
主題 Sunspot groups
キーワード
主題Scheme Other
主題 Solar-terrestrial interactions
キーワード
主題Scheme Other
主題 Maunder minimum
内容記述
内容記述 In addition to regular Schwabe cycles (≈11 yr), solar variability also shows longer periods of enhanced or reduced activity. Of these, reconstructions of the Dalton Minimum provide controversial sunspot group numbers and limited sunspot positions, partially due to limited source record accessibility. In this context, we analyzed Stephan Prantner's sunspot observations spanning from 1804 to 1844, the values of which had only been known through estimates despite their notable chronological coverage during the Dalton Minimum. We identified his original manuscript in Stiftsarchiv Wilten, near Innsbruck (Austria). We reviewed his biography (1782–1873) and located his observational sites at Wilten and Waidring, which housed the principal telescopes for his early and late observations: a 3.5 inch astronomical telescope and a Reichenbach 4 foot achromatic erecting telescope, respectively. We identified 215 days of datable sunspot observations, which is almost twice as much data as his estimated data in the existing databases (=115 days). In Prantner's records, we counted up to seven to nine sunspot groups per day and measured sunspot positions, which show their distributions in both solar hemispheres. These results strikingly emphasize the difference between the Dalton Minimum and the Maunder Minimum as well as the similarity between the Dalton Minimum and the weak solar cycles in the modern observations.
言語 en
内容記述タイプ Abstract
出版者
言語 en
出版者 IOP publishing
言語
言語 eng
資源タイプ
資源タイプresource http://purl.org/coar/resource_type/c_6501
タイプ journal article
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
関連情報
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.3847/1538-4357/abee1b
収録物識別子
収録物識別子タイプ PISSN
収録物識別子 0004-637X
書誌情報 en : The Astrophysical Journal

巻 919, 号 1, p. 1, 発行日 2021-09-20
ファイル公開日
日付 2022-02-08
日付タイプ Available
戻る
0
views
See details
Views

Versions

Ver.1 2022-02-08 05:40:29.071319
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