Mapping solar magnetic fields from the photosphere to the base of the corona

Routine ultraviolet imaging of the Sun’s upper atmosphere shows the spectacular manifestation of solar activity; yet, we remain blind to its main driver, the magnetic field. Here, we report unprecedented spectropolarimetric observations of an active region plage and its surrounding enhanced network,...

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Detalles Bibliográficos
Autores principales: Ishikawa, Ryohko, Bueno, Javier Trujillo, del Pino Alemán, Tanausú, Okamoto, Takenori J., McKenzie, David E., Auchère, Frédéric, Kano, Ryouhei, Song, Donguk, Yoshida, Masaki, Rachmeler, Laurel A., Kobayashi, Ken, Hara, Hirohisa, Kubo, Masahito, Narukage, Noriyuki, Sakao, Taro, Shimizu, Toshifumi, Suematsu, Yoshinori, Bethge, Christian, De Pontieu, Bart, Dalda, Alberto Sainz, Vigil, Genevieve D., Winebarger, Amy, Ballester, Ernest Alsina, Belluzzi, Luca, Štěpán, Jiří, Ramos, Andrés Asensio, Carlsson, Mats, Leenaarts, Jorrit
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2021
Materias:
Research Articles
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7895431/
https://www.ncbi.nlm.nih.gov/pubmed/33608278
http://dx.doi.org/10.1126/sciadv.abe8406

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7895431/
https://www.ncbi.nlm.nih.gov/pubmed/33608278
http://dx.doi.org/10.1126/sciadv.abe8406

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