Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Mélissa D. Menu"'
Publikováno v:
Physics of the Earth and Planetary Interiors
Physics of the Earth and Planetary Interiors, Elsevier, 2020, 307, pp.106542. ⟨10.1016/j.pepi.2020.106542⟩
Physics of the Earth and Planetary Interiors, Elsevier, 2020, 307, pp.106542. ⟨10.1016/j.pepi.2020.106542⟩
The dynamo effect is the most popular candidate to explain the non-primordial magnetic fields of astrophysical objects. Although many systematic studies of parameters have already been made to determine the different dynamical regimes explored by dir
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d0c26728adab3487fe57ad7f49c62e3
http://arxiv.org/abs/2007.05530
http://arxiv.org/abs/2007.05530
Autor:
Regis Terrier, V. H. M. Phan, Julian Krause, Mélissa D. Menu, Stefano Gabici, Giovanni Morlino, Jacco Vink
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A40. ⟨10.1051/0004-6361/201936927⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A40. ⟨10.1051/0004-6361/201936927⟩
Astronomy & Astrophysics, 635:A40. EDP Sciences
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2020, 635, pp.A40. ⟨10.1051/0004-6361/201936927⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A40. ⟨10.1051/0004-6361/201936927⟩
Astronomy & Astrophysics, 635:A40. EDP Sciences
Astronomy & Astrophysics
Supernova remnants interacting with molecular clouds are ideal laboratories to study the acceleration of particles at shock waves and their transport and interactions in the surrounding interstellar medium. In this paper, we focus on the supernova re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da3ea086579367e90a04c8a03e5c8e0a
https://hal-cea.archives-ouvertes.fr/cea-02499011/file/aa36927-19.pdf
https://hal-cea.archives-ouvertes.fr/cea-02499011/file/aa36927-19.pdf
We investigate the impact of a solid-body rotation $\Omega_0$ on the large-scale dynamics of an incompressible magnetohydrodynamic turbulent flow in presence of a background magnetic field $\bf B_0$ and at low Rossby number. Three-dimensional direct
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ce5c808d62fe2edac8d92a242a723d2b
http://arxiv.org/abs/1905.10250
http://arxiv.org/abs/1905.10250