Chromospheric Running Wave from a Solar Cyclone Produced through the Emergence of a Twisted Magnetic Flux Tube | Zendy

Tetsuya Magara | Zendy; Jun-Mo An | Zendy; Hwanhee Lee | Zendy; Jihye Kang | Zendy; Satoshi Inoue | Zendy; G. S. Choe | Zendy

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Chromospheric Running Wave from a Solar Cyclone Produced through the Emergence of a Twisted Magnetic Flux Tube

Author(s) -

Tetsuya Magara,

Jun-Mo An,

Hwanhee Lee,

Jihye Kang,

Satoshi Inoue,

G. S. Choe

Publication year - 2012

Publication title -

publications of the astronomical society of japan

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.99

H-Index - 110

eISSN - 2053-051X

pISSN - 0004-6264

DOI - 10.1093/pasj/64.5.l4

Subject(s) - physics , flux tube , flux (metallurgy) , cyclone (programming language) , tube (container) , magnetic flux , astrophysics , astronomy , mechanics , meteorology , magnetic field , mechanical engineering , materials science , quantum mechanics , field programmable gate array , computer science , computer hardware , metallurgy , engineering

An innovative solar observing satellite, Hinode, has successfully observed the detailed evolution of an emerging magnetic field, starting from its appearance at the solar surface, to forming a developed bipolar region. The high spatial and temporal resolutions provided by the satellite has enabled us to capture prominent dynamic phenomena caused by the emerging magnetic field, such as a running wa...

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