Formation of Opposite-Sign Magnetic Helicity by an Erupting Filament in a Coronal Mass Ejection
スポンサーリンク
概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 2004-06-25
著者
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Kurokawa Hiroki
Kwasan And Hida Observatories Kyoto University
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LIU Yu
Kwasan and Hida Observatories, Kyoto University
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Liu Yu
Kwasan And Hida Observatories Kyoto University
関連論文
- Energetic Relations between the Disappearing Solar Filaments and the Associated Flare Arcades
- Horizontal and Vertical Flow Structure in Emerging Flux Regions
- X-Ray Expanding Features Associated with a Moreton Wave
- Eruptive and Quasi-Eruptive Disappearing Solar Filaments and Their Relationship with Coronal Activities
- Relation between a Moreton Wave and an EIT Wave Observed on 1997 November 4
- Emergence of Twisted Magnetic-Flux Bundles and Flare Activity in a Large Active Region, NOAA 4201
- Contribution and Properties of the Green-and Red-Line Coronal Loops in the K-Corona
- Close Correlation among Hα Surges, Magnetic Flux Cancellations, and UV Brightenings Found at the Edge of an Emerging Flux Region
- A Method for the Determination of 3-D Velocity Fields of Disappearing Solar Filaments
- Formation of Opposite-Sign Magnetic Helicity by an Erupting Filament in a Coronal Mass Ejection
- A Study on Red Asymmetry of Hα Flare Ribbons Using a Narrowband Filtergram in the 2001 April 10 Solar Flare