云南师范大学学报（自然科学版）2017，Vol.37Issue(3)：1-4,4.DOI:10.7699/j.ynnu.ns-2017-029
抚仙湖观测站对太阳黑子的观测
Observations of Sunspots by Fuxian Solar Observatory
摘要
Abstract
Oscillations and waves are a type of fundamental phenomena occurring in sunspots.It is important to measure the oscillation period for understanding the evolution of sunspots.A high temporal resolution observation images of the sunspot within the active region AR 11692 was carried out by NVST(The 1m New Vacuum Solar Telescope) at FSO(Fuxian Solar Observatory) in March 13,2013 at the Hα(6 562.80(A)) line.The high quality observations give us a good chance to measure the oscillation period.By using Fast Fourier Transformation(FFT),we derive the umbra oscillation period of the sunspot is 165 s,which means the umbra oscillation in the Hα(6 562.80(A)) line formation region is a typical 3 min oscillation,and existing a typical 5min oscillations at penumbra area,the oscillation period is 283 s.关键词
太阳黑子/本影振荡/半影行波/周期Key words
Sunspots/Umbra oscillation/Penumbra wave/Period分类
天文与地球科学引用本文复制引用
张文佳,周新平,梁红飞,李秋幻..抚仙湖观测站对太阳黑子的观测[J].云南师范大学学报（自然科学版）,2017,37(3):1-4,4.基金项目
国家自然科学基金资助项目(11363007,11063005). （11363007,11063005）
