CHROMOSPHERIC OSCILLATIONS IN K-2V BRIGHT POINTS

The 3 minute waves observed in K-2v emission from bright points in the quiet solar chromosphere are shown to be oscillations of the atmosphe re at the cutoff period of acoustic waves, implying impulsive excitati on. Other interpretations of the period are shown not to be viable sin ce they fail the dual requirement of spatial intermittence, in which m ost of the supergranulation cell interior is inert over the course of an hour, and temporal intermittence, in which the active locations in the cell interior are active at most half the time. It is speculated t hat the episodic excitation of the K-2v oscillations is due to collisi ons of granules with magnetic elements of mixed polarity with a field strength of at least 0.5 kG.