Observations of P-Mode Oscillations in the Sun and Solar-Like Stars

大熊星大量日震数据集的再分析 太阳观测站将负责提取所有信息 它所包含的。 还将搜索 太阳振荡与太阳周期，因为数据涵盖了 从太阳活动极小期到极大期的整个时间间隔。 新型精密径向 将获得明亮的太阳型恒星的速度数据， 尝试检测与那些类似的单独p模式振荡 在阳光下。

A reanalysis of the extensive helioseismic data set from Big Bear Solar Observatory will be undertaken to extract all the information which it contains. A search will also be made for variation of the solar oscillations with the solar cycle since the data covers the entire interval from solar minimum to maximum. New precise radial velocity data will be obtained for bright solar type stars to attempt to detect individual p-mode oscillations analogous to those in the sun.