Synoptic Solar Velocity and Magnetic Field Observations Using the 150-Foot Solar Tower on Mount Wilson Observatory

这个项目继续研究太阳能量学和动力学，基于威尔逊山太阳塔观测设施及其数字数据库（可追溯到1967年）。研究人员的目的是增加对太阳周期变化及其对地球环境影响的了解。此外，他还通过网站向社区提供他的数据。具体来说，这个持续的项目：(1)在四条不同的谱线上对至少6对线翼样品进行磁图观测，包括磁图、多普勒图和强度图；(2)对1986年至今的数据集应用改进的太阳半径定义；(3)使用钠D线研究声和磁振荡的垂直传播。

This program continues studies of solar energetics and dynamics, based on the Mount Wilson solar tower observing facility and its digital database (dating back to 1967). The investigator's intent is increasing understanding of the solar cycle of variability and its influence on Earth's environment. In addition, he makes his data available to the community via the website. Specifically, this continuing program: (1) makes magnetogram observations consisting of magnetograms, dopplergrams and intensitygrams for at least 6 pairs of line wing samples in four different spectral lines, (2) applies an improved solar radius definition to the 1986-present data set, and (3) studies the vertical propagation of acoustic and magnetic oscillations using the sodium D line.