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Convective plasma around solar pores S. Vargas DomÃnguez Abstract Magnetic structures are commonly observed in the solar photosphere at many different spatial scales, being sunspots and pores the most conspicuous ones.
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Document Date: 2010-04-20 07:47:25
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File Size: 2,75 MB
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Organization
National Oceanic and Atmospheric Administration /
/
Person
Martinez Pillet /
V /
/
SocialTag
Physics
Space plasmas
Plasma physics
Stellar astronomy
Sun
Corona
Hinode
Velocity
Proper motion
Astronomy
Convective plasma around solar pores S. Vargas DomÃnguez Abstract Magnetic structures are commonly observed in the solar photosphere at many different spatial scales, being sunspots and pores the most conspicuous ones.