In a 3D radiative hydrodynamic solar simulation, convective patterns increase in size down to about 7 Mm, then become more homogeneous while the velocity spectra continue to show scale growth with depth.
Kitiashvili, Alan A
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling
In a 3D radiative hydrodynamic solar simulation, convective patterns increase in size down to about 7 Mm, then become more homogeneous while the velocity spectra continue to show scale growth with depth.