The Solar Internetwork. III. Unipolar versus Bipolar Flux Appearance

This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.

Detalhes bibliográficos
Autores: Gosic, Milan, Bellot Rubio, Luis R., Cheung, M. C. M., Orozco Suárez, David, Katsukawa, Y., Toro, José Carlos del
Tipo de documento: artigo
Estado:Versão publicada
Data de publicação:2022
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositório:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/282015
Acesso em linha:http://hdl.handle.net/10261/282015
Access Level:Acceso aberto
Palavra-chave:Solar photosphere
Solar magnetic flux emergence
Solar magnetic fields
Descrição
Resumo:This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.

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