Convective plasma around solar pores S. Vargas Domínguez 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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Date: 2010-04-20 07:47:25 Physics Space plasmas Plasma physics Stellar astronomy Sun Corona Hinode Velocity Proper motion Astronomy Light sources Space		Convective plasma around solar pores S. Vargas Domínguez Abstract Magnetic structures are commonly observed in the solar photosphere at many different spatial scales, being sunspots and pores the most conspicuous ones. Add to Reading List Source URL: www.mssl.ucl.ac.uk Download Document from Source Website File Size: 2,75 MB Share Document on Facebook

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