Geomagnetic storms of cycle 24 and their solar sources
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DOI[10.1186/s40623-017-0653-z]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Shinichi Watari
- Publication, Distribution, etc.
- Publication Date
- 2017-05-19
- Publication Date (W3CDTF)
- 2017-05-19
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 69(70)
- Volume
- 69(70)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-017-0653-z
- Persistent ID (NDL)
- info:ndljp/pid/10369097
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2017-06-22T22:40:19+09:00
- Date Captured (W3CDTF)
- 2017-06-22
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/10319651
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- コレクション : 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- DOI
- 10.1186/s40623-017-0653-z
- Access Restrictions
- インターネット公開
- Related Material (URI)
- Is Referenced By
- The Solar and Geomagnetic Storms in 2024 May: A Flash Data ReportRelationship between the low-latitude coronal hole area, solar wind velocity, and geomagnetic activity during solar cycles 23 and 24
- References
- Geomagnetic activity during the rising phase of solar cycle 24Solar wind drivers of geomagnetic storms during more than four solar cyclesSolar connections of geoeffective magnetic structuresNo Major Solar Flares but the Largest Geomagnetic Storm in the Present Solar CycleOn the relationship between magnetic cloud field polarity and geoeffectivenessAn empirical relationship between interplanetary conditions and<i>Dst</i>ASYMMETRIC SOLAR POLAR FIELD REVERSALSInterplanetary conditions causing intense geomagnetic storms (Dst ≤ −100 nT) during solar cycle 23 (1996–2006)WEAKEST SOLAR WIND OF THE SPACE AGE AND THE CURRENT “MINI” SOLAR MAXIMUMSolar and interplanetary sources of major geomagnetic storms (<i>Dst</i> ≤ −100 nT) during 1996–2005How unprecedented a solar minimum?Major geomagnetic storms (<i>Dst</i> ≤ −100 nT) generated by corotating interaction regionsDual-peak solar cycle distribution of intense geomagnetic stormsMajor solar eruptions and high-energy particle events during solar cycle 24
- References (URI)
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 雑誌記事索引データベースCrossref科学研究費助成事業データベースCrossrefCrossref
- Bibliographic ID (NDL)
- 10369097