[HTML][HTML] Solar surface convection
Å Nordlund, RF Stein, M Asplund - Living Reviews in Solar Physics, 2009 - Springer
Solar Surface Convection | Living Reviews in Solar Physics Skip to main content
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Dynamics of large-scale solar flows
The Sun's axisymmetric large-scale flows, differential rotation and meridional circulation, are
thought to be maintained by the influence of rotation on the thermal-convective motions in …
thought to be maintained by the influence of rotation on the thermal-convective motions in …
[图书][B] The sun: an introduction
M Stix - 2012 - books.google.com
A wealth of new experimental and theoretical results has been obtained in solar physics
since the first edition of this textbook appeared in 1989. Thus all nine chapters have been …
since the first edition of this textbook appeared in 1989. Thus all nine chapters have been …
Interactive desktop analysis of high resolution simulations: application to turbulent plume dynamics and current sheet formation
The ever increasing processing capabilities of the supercomputers available to
computational scientists today, combined with the need for higher and higher resolution …
computational scientists today, combined with the need for higher and higher resolution …
Structure and evolution of giant cells in global models of solar convection
The global scales of solar convection are studied through three-dimensional simulations of
compressible convection carried out in spherical shells of rotating fluid that extend from the …
compressible convection carried out in spherical shells of rotating fluid that extend from the …
A grid of three-dimensional stellar atmosphere models of solar metallicity. I. General properties, granulation, and atmospheric expansion
Present grids of stellar atmosphere models are the workhorses in interpreting stellar
observations and determining their fundamental parameters. These models rely on greatly …
observations and determining their fundamental parameters. These models rely on greatly …
The scales of granulation, mesogranulation, and supergranulation
MP Rast - The Astrophysical Journal, 2003 - iopscience.iop.org
Solar granulation is described as an advection-fragmentation process in the upper layers of
the convection zone. The fundamental hydrodynamic unit is the downflow plume, and from …
the convection zone. The fundamental hydrodynamic unit is the downflow plume, and from …
Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
MP Rast, N Bello González, L Bellot Rubio, W Cao… - Solar Physics, 2021 - Springer
Abstract The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will
revolutionize our ability to measure, understand, and model the basic physical processes …
revolutionize our ability to measure, understand, and model the basic physical processes …
Time series of solar granulation images. I. Differences between small and large granules in quiet regions
J Hirzberger, M Vázquez, JA Bonet… - The Astrophysical …, 1997 - iopscience.iop.org
A 90 minute time series of high spatial resolution white-light images of solar granulation,
obtained at the Swedish Vacuum Solar Tower (Observatorio del Roque de los Muchachos …
obtained at the Swedish Vacuum Solar Tower (Observatorio del Roque de los Muchachos …
Development of structure in pores and sunspots: flows around axisymmetric magnetic flux tubes
NE Hurlburt, AM Rucklidge - Monthly Notices of the Royal …, 2000 - academic.oup.com
Flux elements, pores and sunspots form a family of magnetic features observed at the solar
surface. As a first step towards developing a fully non-linear model of the structure of these …
surface. As a first step towards developing a fully non-linear model of the structure of these …