The uncombed penumbra

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dc.creatorBorrero, J. M.
dc.creatorRempel, M.
dc.creatorSolanki, S. K.
dc.date2006-02-06
dc.date.accessioned2026-07-07T06:57:13Z
dc.date.available2026-07-07T06:57:13Z
dc.descriptionThe uncombed penumbral model explains the structure of the sunspot penumbra in terms of thick magnetic fibrils embedded in a magnetic surrounding atmosphere. This model has been successfully applied to explain the polarization signals emerging from the sunspot penumbra. Thick penumbral fibrils face some physical problems, however. In this contribution we will offer possible solutions to these shortcomings.
dc.description6 pages, 2 figures. to appear in the proceedings of the Solar Polarization Workshop IV
dc.identifierhttps://arxiv.org/abs/astro-ph/0602129
dc.identifierhttp://arxiv.org/abs/astro-ph/0602129
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/106886
dc.subjectAstrophysics
dc.titleThe uncombed penumbra
dc.typetext

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