LOCALIZED SOURCES OF PROPAGATING ACOUSTIC-WAVES IN THE SOLAR PHOTOSPHERE

We describe a time series of Doppler measurements of the solar photosphere with moderate spatial resolution, covering a portion of the solar disk surrounding a small sunspot group. At temporal frequencies above 5.5 mHz, the Doppler field probes the spatial and temporal distribution of regions that emit acoustic energy. We find that in the frequency range 5.5 less-than-or-equal-to v less-than-or-equal-to 7.5 mHz, a small fraction of the surface area emits a disproportionate amount of acoustic energy. The regions with excess emission are characterized by a patchy structure at spatial scales of a few arcseconds and by association (but not exact co-location) with regions having substantial magnetic field strength. These observations bear on the conjecture (see work by Brown) that most of the acoustic energy driving solar p-modes is created in localized regions occupying a small fraction of the solar surface area.