OBSERVATIONS OF SOLAR OSCILLATIONS WITH PERIODS OF 160 MINUTES
OBSERVATIONS OF SOLAR OSCILLATIONS WITH PERIODS OF 160 MINUTES
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DOI：
10.1038/277635a0
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发表时间：
1979-01-01
期刊：
影响因子：
64.8
通讯作者：
TSAP, TT
中科院分区：
文献类型：
--
作者：
SCHERRER, PH;WILCOX, JM;TSAP, TT
Severnyet等人[1]曾报道过太阳周期接近160分钟的振荡，Kotovet等人[2]对此作了进一步的描述。这种振荡的存在将导致我们对太阳物理学知识的显着增加。报告的振幅约为1 ms− 1，接近观测技术的极限。这里描述的观测在斯坦福大学太阳天文台从1975年到现在似乎支持克里米亚天体物理观测站的报告。
OSCILLATIONS of the Sun with a period near 160 min have been reported by Severnyet al.1and further described by Kotovet al.2. The presence of such oscillations would lead to a significant increase in our knowledge of solar physics. The reported amplitude is of the order of 1 ms−1which is near the limit of observing technology. Observations described here at the Stanford Solar Observatory from 1975 to the present seem to support the reports from the Crimean Astrophysical Observatory1,2.