Zobrazeno 1 - 1
of 1
pro vyhledávání: '"Accretion disks – Dynamo – Instabilities – Magnetohydrodynamics (MHD) – Turbulence"'
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2015, 575, pp.A14. ⟨10.1051/0004-6361/201424324⟩
Astronomy and Astrophysics-A&A, 2015, 575, pp.A14. ⟨10.1051/0004-6361/201424324⟩
The magnetorotational (MRI) dynamo has long been considered one of the possible drivers of turbulent angular momentum transport in astrophysical accretion disks. However, various numerical results suggest that this dynamo may be difficult to excite i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::98f19a11573a5f0d3d0195ac1cf02f3f
http://arxiv.org/abs/1410.3406
http://arxiv.org/abs/1410.3406
