Results 31 to 40 of about 3,875 (223)
Latitudinal Variation of the Solar Photospheric Intensity [PDF]
24 pages, 8 figs, accepted in ...
Rast, Mark P. +2 more
openaire +2 more sources
Simulations of magneto-convection in the solar photosphere
We have developed a 3D magnetohydrodynamics simulation code for applications in the solar convection zone and photosphere. The code includes a non-local and non-grey radiative transfer module and takes into account the effects of partial ionization.
Shelyag, S. +17 more
core +1 more source
STOCHASTIC COUPLING OF SOLAR PHOTOSPHERE AND CORONA [PDF]
36 pageS, 11 figures, 3 ...
Uritsky, Vadim M. +3 more
openaire +2 more sources
Turbulence in the Solar Photosphere [PDF]
16 pages, 1 ...
openaire +2 more sources
MAGNETOHYDRODYNAMICS OF THE WEAKLY IONIZED SOLAR PHOTOSPHERE [PDF]
We investigate the importance of ambipolar diffusion and Hall currents for high-resolution comprehensive ('realistic') photospheric simulations. To do so we extended the radiative magnetohydrodynamics code \emph{MURaM} to use the generalized Ohm's law under the assumption of local thermodynamic equilibrium.
Cheung, M., Cameron, R.
openaire +3 more sources
We report and discuss the phase shift and phase travel time of low-frequency ( ν < 5.0 mHz) acoustic waves estimated within the photosphere and photosphere–chromosphere interface regions, utilizing multiheight velocities in the quiet Sun.
Hirdesh Kumar +4 more
doaj +1 more source
Solar and stellar photospheric abundances
The determination of photospheric abundances in late-type stars from spectroscopic observations is a well-established field, built on solid theoretical foundations. Improving those foundations to refine the accuracy of the inferred abundances has proven challenging, but progress has been made.
openaire +3 more sources
Simulated magnetic flows in the solar photosphere [PDF]
Recent Sunrise/IMaX observations have revealed the existence of supersonic magnetic flows. Our aim is to determine the origin of such flows by using realistic MHD simulations. We simulate cancellation and emergence of magnetic flux through the solar photosphere. Our first numerical experiment starts with magnetic field of both polarities.
Danilovic, S., Cameron, R., Solanki, S.
openaire +3 more sources
Noble gases and nitrogen in material from asteroid Bennu
Abstract We report the elemental and isotopic abundances of all stable noble gases (helium, neon, argon, krypton, and xenon) in eight particles from asteroid Bennu returned by NASA's OSIRIS‐REx mission. We also report nitrogen abundances and isotopic ratios that were analyzed alongside neon and argon in four additional Bennu particles.
B. Marty +7 more
wiley +1 more source
A High-resolution, Inversion-based Synoptic Study of Solar Granulation
The convectively driven, weakly magnetized regions of the solar photosphere dominate the Sun’s surface at any given time, but the temporal variations of these quiet regions of the photosphere throughout the solar cycle are still not well known.
James W. Crowley +3 more
doaj +1 more source

