Zobrazeno 1 - 10
of 46
pro vyhledávání: '"Matthew K. Browning"'
Autor:
Allan Sacha Brun, Matthew K. Browning
Publikováno v:
Living Reviews in Solar Physics, Vol 14, Iss 1, Pp 1-133 (2017)
Abstract The Sun and other stars are magnetic: magnetism pervades their interiors and affects their evolution in a variety of ways. In the Sun, both the fields themselves and their influence on other phenomena can be uncovered in exquisite detail, bu
Externí odkaz:
https://doaj.org/article/a59b6b92c22b4364af59ca3e8f7a2f2e
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 456:1708-1722
We discuss here a purely hydrodynamical mechanism to invert the sign of the kinetic helicity, which plays a key role in determining the direction of propagation of cyclical magnetism in most models of dynamo action by rotating convection. Such propag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::404a05786b3969e7718812a5204dde8b
https://doi.org/10.1093/mnras/stv2726
https://doi.org/10.1093/mnras/stv2726
Autor:
Edward Townsend, Suzannah Boardman, Joshua Clarke, Maria A. Weber, Samuel Pugsley, Matthew K. Browning
Evidence of surface magnetism is now observed on an increasing number of cool stars. The detailed manner by which dynamo-generated magnetic fields giving rise to starspots traverse the convection zone still remains unclear. Some insight into this flu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ed6f73d61e1a61e531b187c4cbd0b98
http://arxiv.org/abs/1703.04982
http://arxiv.org/abs/1703.04982
Autor:
Laura K. Currie, Matthew K. Browning
Convection in astrophysical systems must be maintained against dissipation. Although the effects of dissipation are often assumed to be negligible, theory suggests that in strongly stratified convecting fluids, the dissipative heating rate can exceed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c74b013dcbc2523e873b68109f162ba1
Autor:
Nathan J. Mayne, Isabelle Baraffe, John Thuburn, David M. Acreman, Chris Smith, F. Debras, James Manners, Matthew K. Browning, David S. Amundsen, Nigel Wood
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2017, 604, ⟨10.1051/0004-6361/201730465⟩
Astronomy and Astrophysics-A&A, 2017, 604, ⟨10.1051/0004-6361/201730465⟩
We present highlights from a large set of simulations of a hot Jupiter atmosphere, nominally based on HD 209458b, aimed at exploring both the evolution of the deep atmosphere, and the acceleration of the zonal flow or jet. We find the occurrence of a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::608bef354b76276250b7d6321b4cb8ba
https://hal-insu.archives-ouvertes.fr/insu-03710617
https://hal-insu.archives-ouvertes.fr/insu-03710617
Autor:
Matthew K. Browning, Allan Sacha Brun
Publikováno v:
Living Reviews in Solar Physics
Living Reviews in Solar Physics, Vol 14, Iss 1, Pp 1-133 (2017)
Living Reviews in Solar Physics, Vol 14, Iss 1, Pp 1-133 (2017)
The Sun and other stars are magnetic: magnetism pervades their interiors and affects their evolution in a variety of ways. In the Sun, both the fields themselves and their influence on other phenomena can be uncovered in exquisite detail, but these o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e3cab765455fa0d88f687cdf09acd8a
https://pubmed.ncbi.nlm.nih.gov/31997984
https://pubmed.ncbi.nlm.nih.gov/31997984
Autor:
Matthew K. Browning
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 108:736-738
It is by now a truism to note that magnetic fields are ubiquitous in astrophysics: from the formation of stars to their eventual death, from the grandest galaxy to the rockiest planet, few astrophy...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eb608214f254baf42bd1817bf060fe4e
https://doi.org/10.1080/03091929.2014.964919
https://doi.org/10.1080/03091929.2014.964919
Autor:
Matthew K. Browning, Mark S. Miesch, Nicholas J. Nelson, Benjamin P. Brown, Juri Toomre, Allan Sacha Brun
Publikováno v:
Proceedings of the International Astronomical Union. 6:272-275
Observations of sun-like stars rotating faster than our current sun tend to exhibit increased magnetic activity as well as magnetic cycles spanning multiple years. Using global simulations in spherical shells to study the coupling of large-scale conv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4797e6c0270b51a5f0c1b54d0d1fbdef
https://doi.org/10.1017/s1743921311015365
https://doi.org/10.1017/s1743921311015365
Publikováno v:
Proceedings of the International Astronomical Union. 6:111-115
A-type stars have both a near-surface layer of fast convection that can excite acoustic modes and a deep zone of core convection whose properties may be probed with asteroseismology. Many A-type stars also exhibit large magnetic spots that are often
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a01dfb8e124230a6313ed26f7e00f86b
https://doi.org/10.1017/s1743921311015092
https://doi.org/10.1017/s1743921311015092