Spectroscopic Studies of Stellar Activity

对表面活动类似于 太阳色球层将继续使用仪器 宾夕法尼亚州立大学开发的。 恒星的类型 研究包括BY Dra星，RS CVn星，弱线T Tau星 和经典的T型Tau星 一个大约两千人的档案 光谱已经建立了一段时间，并将 沿着，在本研究中利用新的数据来获取。 新 还计划使用仪器进行红外观测， 测量恒星磁场的目标。

Research on stars which show surface activity analogous to the solar chromosphere will be continued using instrumentation developed at Pennsylvania State University. Types of stars to be studied include BY Dra stars, RS CVn stars, weak-lined T Tau stars and classical T Tau stars. An archive of about two thousand spectra has been built up over a period of years and will be exploited in this research along with new data to be acquired. New instrumentation is also planned for infrared observations with the goal of measuring magnetic fields in stars.