Zobrazeno 1 - 10
of 106
pro vyhledávání: '"Robert F. Stein"'
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 1, p 24 (2024)
We describe the Stagger code for simulations of magnetohydrodynamic (MHD) systems. This is a modular code with a variety of physics modules that will let the user run simulations of deep stellar atmospheres, sunspot formation, stellar chromospheres a
Externí odkaz:
https://doaj.org/article/1ab0dedd271e4bb2bbca5b4f65d3facf
Autor:
Robert F. Stein
Publikováno v:
Living Reviews in Solar Physics, Vol 9, p 4 (2012)
We review the properties of solar magneto-convection in the top half of the convection zones scale heights (from 20 Mm below the visible surface to the surface, and then through the photosphere to the temperature minimum). Convection is a highly non-
Externí odkaz:
https://doaj.org/article/a446c090cf524fd7aa8030de1bb2db7c
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 622, pp.A112. ⟨10.1051/0004-6361/201834283⟩
Astronomy and Astrophysics-A&A, 2019, 622, pp.A112. ⟨10.1051/0004-6361/201834283⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 622, pp.A112. ⟨10.1051/0004-6361/201834283⟩
Astronomy and Astrophysics-A&A, 2019, 622, pp.A112. ⟨10.1051/0004-6361/201834283⟩
Trees of fragmenting granules (TFG) and associated flows are suspected to playa major role in the formation of the network in the quiet Sun. We investigate the counterparts, in terms of dynamics, of surface structures detectable by high resolution ob
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::67ba185e3370c67f107265c549b7024a
https://hal.archives-ouvertes.fr/hal-02178031
https://hal.archives-ouvertes.fr/hal-02178031
Autor:
John Leibacher, Robert F. Stein
Publikováno v:
Solar Neutrinos ISBN: 9780429502811
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c539f2066bb32cc54e12029642f845a0
https://doi.org/10.1201/9780429502811-109
https://doi.org/10.1201/9780429502811-109
Publikováno v:
Solar Physics
Solar Physics, Springer Verlag, 2018, 293 (1), ⟨10.1007/s11207-017-1225-x⟩
Solar Physics, Springer Verlag, 2018, 293 (1), ⟨10.1007/s11207-017-1225-x⟩
We compare horizontal velocities, vertical magnetic fields and evolution of trees of fragmenting granules (TFG, also named families of granules) derived in the quiet Sun at disk center from observations at solar minimum and maximum of the Solar Optic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fdc113927a0f252b92383e7e593fd60d
https://hal.archives-ouvertes.fr/hal-02178056
https://hal.archives-ouvertes.fr/hal-02178056
Autor:
Robert F. Stein, Sebastien Couvidat, Aaron C. Birch, Bernhard Fleck, Sanja Danilovic, Laurent Gizon, Robert H. Cameron, Björn Löptien, Kaori Nagashima
Publikováno v:
Solar Physics. 289:3457-3481
The Solar Dynamics Observatory/Helioseismic and Magnetic Imager (SDO/HMI) filtergrams, taken at six wavelengths around the Fe I 6173.3 {\AA} line, contain information about the line-of-sight velocity over a range of heights in the solar atmosphere. M
Publikováno v:
EPJ Web of Conferences, Vol 101, p 06064 (2015)
We have constructed a grid of 3D hydrodynamic simulations of deep convective and line-blanketed atmospheres. We have developed a new consistent method for computing and employing T(τ ) relations from these simulations, as surface boundary conditions
Publikováno v:
Proceedings of the International Astronomical Union. 2:331-342
Excitation of f- and p- modes by Reynolds stresses and entropy fluctuations is reviewed. Approximations made to allow semi-analytic analysis are discussed. The spectrum of solar convection is presented and shown to NOT be separable into independent s
Autor:
M. van Noort, Åke Nordlund, Mats G. Löfdahl, Göran B. Scharmer, Robert F. Stein, Mats Carlsson, L. Rouppe van der Voort, B. De Pontieu
Publikováno v:
The Astrophysical Journal. 646:1405-1420
We present high-resolution G-band observations (obtained with the Swedish 1 m Solar Telescope) of the rapid temporal variability of faculae, which occurs on granular timescales. By combining these observations with magnetoconvection simulations of a
Autor:
Robert F. Stein, Åke Nordlund
Publikováno v:
The Astrophysical Journal. 642:1246-1255
Magnetoconvection simulations on mesogranule and granule scales near the solar surface are used to study the effect of convective motions on magnetic fields: the sweeping of magnetic flux into downflow lanes, the twisting of magnetic field lines, and