Horizontal and Vertical Flow Structure in Emerging Flux Regions
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
- 2006-04-25
著者
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Berger Thomas
Lockheed Martin Solar And Astrophysics Lab
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Brooks David
Naval Res. Lab. Washington D.c. Usa
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KUROKAWA Hiroki
Kwasan and Hida Observatories, Kyoto University
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KOZU Hiromichi
Hida Observatory, Kyoto University
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KITAI Reizaburo
Hida Observatory, Kyoto University
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BROOKS David
E.O. Hulburt Center for Space Research, Code 7670 Naval Research Laboratory
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YOSHIMURA Keiji
Montana State University, Physics Department
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Kozu Hiromichi
Hida Observatory Kyoto University
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Kurokawa Hiroki
Kwasan And Hida Observatories Kyoto University
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Kitai Reizaburo
Kyoto Univ. Gifu
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Kitai Reizaburo
Hida Observatory Kyoto University
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Yoshimura Keiji
Montana State University Physics Department
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KUROKAWA Hiroki
Kwasan Observatory, Kyoto University
関連論文
- Evidence from the Extreme-Ultraviolet Imaging Spectrometer for Axial Filament Rotation before a Large Flare
- Spicule Dynamics over a Plage Region
- Hinode Observations of Horizontal Quiet Sun Magnetic Flux and the "Hidden Turbulent Magnetic Flux"
- Flare Ribbons Observed with G-band and Fe I 6302A Filters of the Solar Optical Telescope on Board Hinode
- Initial Helioseismic Observations by Hinode/SOT
- Formation Process of a Light Bridge Revealed with the Hinode Solar Optical Telescope
- Hinode EUV Study of Jets in the Sun's South Polar Corona
- Internal Fine Structure of Ellerman Bombs
- Energetic Relations between the Disappearing Solar Filaments and the Associated Flare Arcades
- Hinode Observations of the Onset Stage of a Solar Filament Eruption
- Hinode EUV Imaging Spectrometer Observations of Solar Active Region Dynamics
- Hinode EUV Imaging Spectrometer Observations of Active Region Loop Morphology : Implications for Static Heating Models of Coronal Emission
- Observations of Transient Active Region Heating with Hinode
- 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
- Evolutional Characteristics of Multiple Spectral Lines during the Impulsive Phase of Solar Flares
- 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
- Development of Real-Time Frame Selector 2 and the Characteristic Convective Structure in the Emerging Flux Region
- Development of Real-Time Frame Selector 2 and the Characteristic Convective Structure in the 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
- 3D Velocity-Field Observation of Solar Convection I. Characteristics of Mesogranulation
- A Study on Red Asymmetry of Hα Flare Ribbons Using a Narrowband Filtergram in the 2001 April 10 Solar Flare