Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Anamaria Navarro"'
Existen observaciones que indican que el campo magnético en la atmósfera solar tiene twist, esto cumple un papel muy importante en diferentes fenómenos solares como la reconexión magnética, las fulguraciones solares, entre otros. Sin embargo, su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::adf4a600db9a3935eb5a032c06dfc6c0
https://repositorio.accefyn.org.co/handle/001/1274
https://repositorio.accefyn.org.co/handle/001/1274
We measure the effects of non-isotropic thermal conduction on generation of solar chromospheric jets through numerical simulations carried out with the use of one fluid MHD code MAGNUS. Following the work of Srivastava et al. (2018), we consider the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::df34e56613dede3103b2cefd56e48389
We numerically simulate emergence of a magnetic plasma blob into a solar coronal hole. This blob may be associated with granulation and therefore it has a weak magnetic field. Two-dimensional simulations are performed using the MAGNUS code which solv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7109778eacfc64c62bf1643d4ddc3a8
http://arxiv.org/abs/1910.11814
http://arxiv.org/abs/1910.11814
Publikováno v:
Canadian Journal of Physics. 95:1089-1095
We explore the influence of density fluctuations on isotropic and anisotropic configurations, extending the concept of cracking for isotropic general relativistic fluid spheres. This concept, conceived to describe the behaviour of anisotropic matter
An infinite family of exact solutions of the electrovacuum Einstein-Maxwell equations is presented. The family is static, axially symmetric and describe thin disks composed by electrically polarized material in a conformastatic spacetime. The form of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::763a99b74b02028544924b01ad34df2b
http://arxiv.org/abs/1704.06630
http://arxiv.org/abs/1704.06630
We present a new magnetohydrodynamic (MHD) code for the simulation of wave propagation in the solar atmosphere, under the effects of electrical resistivity, but not dominant, and heat transference in a uniform 3D grid. The code is based on the finite
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c57d2ea2fc3cfb617e5c05c1d5f21f0d
Publikováno v:
Journal of Physics: Conference Series. 600:012014
We have studied the stability in some anisotropic and isotropic matter configurations, by using the concept of cracking in General Relativity, which was conceived as an alternative and different approach to detect instabilities. It is based in the an