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pro vyhledávání: '"dynamo / stars: activity / stars: chromospheres / stars: magnetic field / stars: solar-type"'
Autor:
C. P. Folsom, Jeffrey C. Hall, Robert H. Cameron, Ansgar Reiners, Sandra V. Jeffers, Stephen C. Marsden, Aline A. Vidotto, Julien Morin, Pascal Petit, J.-F. Donati, S. Boro Saikia, V. Perdelwitz
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 594, pp.A29. ⟨10.1051/0004-6361/201628262⟩
NASA Astrophysics Data System
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 594, pp.A29. ⟨10.1051/0004-6361/201628262⟩
NASA Astrophysics Data System
International audience; The long-term monitoring of magnetic cycles in cool stars is a key diagnostic in understanding how dynamo generation and amplification of magnetic fields occur in stars similar in structure to the Sun. We investigate the tempo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::db503b19c75b2dd155c53a01bf1bedb2
https://hal.archives-ouvertes.fr/hal-01529718
https://hal.archives-ouvertes.fr/hal-01529718