Small-scale topology of solar atmosphere dynamics. IV. On the relation of photospheric oscillations to meso-scale flows

Astronomy and Astrophysics – Astrophysics

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Sun: Granulation, Sun: Oscillations, Sun: Photosphere

Scientific paper

We use a high quality five-hour sequence of images of the solar photosphere taken at the Swedish Solar Vacuum Telescope, La Palma, to study the relation of meso-scale divergence with the amplitudes of photospheric intensity oscillations. Meso-scale flows are determined by local correlation tracking of the granulation. Statistical evaluation of the co-location probability of regions with more than twice the average oscillation amplitude and regions with high or low meso-scale divergence shows that high amplitude regions are preferentially located in regions of negative divergence (convergence) and avoid meso-divergent regions. Additionally we confirm the increase of granule brightness in regions of positive divergence with the opposite effect in regions of convergence.

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