SOLAR P-MODE LINEWIDTHS FROM RECENT BISON-ASTERISK HELIOSEISMOLOGICALDATA

We present low-degree solar p-mode linewidths from the analysis of sev eral high-resolution frequency spectra generated from high-quality Dop pler velocity data collected - in integrated sunlight - by the Birming ham Solar-Oscillations Network (BiSON) between 1991 July and 1995 July . We have used linewidths, Delta nu, measured in a 32-month frequency spectrum, to test the power-law dependence of the widths at low freque ncies. Over the range 1473 less than or equal to nu less than or equal to 1822 mu Hz, we find Delta nu proportional to nu(7.0+/-1.5). If an effort is made to correct for finite observing time systematics, the f itted index increases to 7.3 (and even higher, to 7.8, if a naive, sin gle-bin-width correction is applied). This is somewhat steeper than re ported in previous observations of intermediate-degree modes, and is m ore in line with theoretical calculations which predict Delta nu propo rtional to nu(8) over this frequency range. If one assumes that the st eep dependence reported here persists down to lower frequencies, low-d egree-mode coherence (e-folding) times at 800 mu Hz of > 14 yr, and at 300 mu Hz (i.e. near the frequency expected for the fundamental) of > 13 000 yr are implied.