Results 21 to 30 of about 1,036,703 (213)
Dynamics of the solar granulation [PDF]
Temporal series of quiet region images near the center of the Sun are analysed. The images, monochromatic and in white light, have been acquired at the French-Italian solar telescope THEMIS (Tenerife, Canarie, Spain) by the Italian panoramic monochromator IPM.
Berrilli, F. +3 more
openaire +4 more sources
Modelling of solar granulation [PDF]
AbstractWe present the essential features of the ANTARES code. ANTARES has been developed to perform the simulation of astrophysical flows in one, two, or three dimensions. Using, in particular, the option of grid refinement, we present results for solar granulation achieved at very high spatial resolution.
Muthsam, H. +5 more
openaire +3 more sources
The Evolution of an Average Solar Granule [PDF]
AbstractHigh-resolution photographic spectra of the center of the solar disk have been obtained with the Vacuum Tower Telescope at Sacramento Peak Observatory. Two weak iron lines and the neighboring continuum were recorded with 40 sec time resolutions and better than 1” spatial resolution over a period of 40 min.
openaire +1 more source
Effect of operating conditions and physico–chemical properties on the wet granulation kinetics in high shear mixer [PDF]
The wet granulation process is sensitive to changes in product properties and process variables. The optimal process and formulation are based on the knowledge of the granule growth mechanisms and of the effects of product properties and process ...
Hemati, Mehrdji +2 more
core +1 more source
Context. These studies were carried out in the context of solar-chromosphere heating and solar-wind generation. Aims. We aim to explore granulation-generated, two-fluid waves and flows in the solar atmosphere permeated by a solar magnetic carpet. Methods.
Niedziela R. +2 more
doaj +1 more source
Spectral Deconvolution With Deep Learning: Removing the Effects of Spectral PSF Broadening
We explore novel methods of recovering the original spectral line profiles from data obtained by instruments that sample those profiles with an extended or multipeaked spectral transmission profile.
Momchil Molnar +6 more
doaj +1 more source
The scale of solar granulation
We derive the observed scale of granulation as a consequence of a physical model. At scales smaller than granulation, horizontal radiative transport reduces temperature fluctuations and the resultant buoyancy forces in the surface layers. At scales only slightly larger than granulation, the dynamical pressure required to drive horizontal motions ...
G. D. Nelson, S. Musman
openaire +1 more source
Observations of a bright plume in solar granulation
Aims.The aim of this paper is to analyze the thermal properties, oscillatory, and flow motions of a bright, long-lasting feature observed in solar granulation, which we call the plume.
R. I. Kostik, E. V. Khomenko
core +1 more source
SSI: The Stellar Seismic Indices Data Base *
The Stellar Seismic Indices database (hereafter SSI) has been developed within the SPACEInn project funded under the UE Seventh Framework Programme (FP7). This data base aims at providing stellar seismic indices of solar-like oscillating stars as well as
Samadi Reza +5 more
doaj +1 more source
STEAM GRANULATION VERSUS WET GRANULATION: IMPACT ON GRANULE AND TABLETS PROPERTIES
Steam granulation (SG) involves the use of steam as the granulating medium instead of traditional liquid water [1]. Steam provides a higher diffusion rate into the powder bed and a more favourable thermal balance during the drying step.
Giulia De Santi +5 more
core +2 more sources

