Add to ORKGThe theoretical power spectrum of velocity fields, calculated at the solar photosphere using the superposition of unstable linear convective eigenmodes in the convection zone, displays the mesogranular peak besides the peaks corresponding to granulation and supergranulation. The length-scale associated with the three distinct peaks are in reasonable accord with observations
Context. Regions of quiet Sun generally exhibit a complex distribution of small-scale magnetic field...
The Sun provides us with the only spatially well-resolved astrophysical example of turbulent thermal...
Supergranular motions in the solar photosphere are implicated in phemomena as diverse as the global ...
This work confirms the existence of the mesogranulation as an intermediate scale of convection in th...
[[abstract]]The properties of convective motions on the sun are studied using Kitt Peak Doppler imag...
The theoretical power spectrum of solar velocity field and flux variation is obtained with amplitude...
Aims. We analyse mesogranular flow patterns in a three-dimensional hydrodynamical simulation of sola...
We study whether mesogranulation flow patterns at the solar surface can arise solely from the statis...
The relation of the solar surface magnetic field with mesogranular cells is studied using high spati...
The stability of linear convective modes in the solar convection zone is investigated by incorporati...
Using a 45.5-h time series of photospheric flow fields generated from a set of high-resolution conti...
[[abstract]]The properties of convective motion on the sun for the scales smaller than supergranules...
The origin of solar supergranulation remains a mystery. Unlike granulation, the size of which is com...
Context. Supergranulation is a pattern of the velocity field at the surface of the Sun, which has be...
The characteristics of the most unstable fundamental mode and the first harmonic excited in the conv...
Context. Regions of quiet Sun generally exhibit a complex distribution of small-scale magnetic field...
The Sun provides us with the only spatially well-resolved astrophysical example of turbulent thermal...
Supergranular motions in the solar photosphere are implicated in phemomena as diverse as the global ...
This work confirms the existence of the mesogranulation as an intermediate scale of convection in th...
[[abstract]]The properties of convective motions on the sun are studied using Kitt Peak Doppler imag...
The theoretical power spectrum of solar velocity field and flux variation is obtained with amplitude...
Aims. We analyse mesogranular flow patterns in a three-dimensional hydrodynamical simulation of sola...
We study whether mesogranulation flow patterns at the solar surface can arise solely from the statis...
The relation of the solar surface magnetic field with mesogranular cells is studied using high spati...
The stability of linear convective modes in the solar convection zone is investigated by incorporati...
Using a 45.5-h time series of photospheric flow fields generated from a set of high-resolution conti...
[[abstract]]The properties of convective motion on the sun for the scales smaller than supergranules...
The origin of solar supergranulation remains a mystery. Unlike granulation, the size of which is com...
Context. Supergranulation is a pattern of the velocity field at the surface of the Sun, which has be...
The characteristics of the most unstable fundamental mode and the first harmonic excited in the conv...
Context. Regions of quiet Sun generally exhibit a complex distribution of small-scale magnetic field...
The Sun provides us with the only spatially well-resolved astrophysical example of turbulent thermal...
Supergranular motions in the solar photosphere are implicated in phemomena as diverse as the global ...