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dc.contributor.author Ruzmaikin, A. en_US
dc.date.accessioned 2004-09-23T17:54:09Z
dc.date.available 2004-09-23T17:54:09Z
dc.date.issued 2000 en_US
dc.identifier.citation Space science reviews, Vol. 95, No. 1/2, 2000, pp. 43-53 en_US
dc.identifier.citation Pasadena, CA, USA en_US
dc.identifier.clearanceno 00-0576 en_US
dc.identifier.uri http://hdl.handle.net/2014/14171
dc.description.abstract Sunspots, seen as cool regions on the surface of the Sun, are a thermal phenomenon. Sunspots are always associated with bipolar magnetic loops that break through the solar surface. en_US
dc.format.extent 84702 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Solar convection bipolar active regionsmagnetoconvection en_US
dc.title Origin of sunspots en_US


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