Sunspot transition region oscillations in NOAA 8156

被引:45
作者
Brynildsen, N
Leifsen, T
Kjeldseth-Moe, O
Maltby, P
Wilhelm, K
机构
[1] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway
[2] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany
基金
美国国家航空航天局;
关键词
Sun : magnetic fields; Sun : oscillations; Sun : transition region; Sun : UV radiation sunspots;
D O I
10.1086/311854
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Based on observations obtained with the Solar and Heliospheric Observatory joint observing program for velocity fields in sunspot regions, we have detected 3 minute transition region umbral oscillations in NOAA 8156. Simultaneous recordings of O v lambda 629 and N v lambda 1238, lambda 1242 with the SUMER instrument give the spatial distribution of power in the 3 minute oscillations, both in intensity and in line-of-sight velocity. Comparing loci with the same phase, we find that the entire umbral transition region oscillates. The observed maxima in peak line intensity are nearly in phase with the maxima in velocity directed toward the observer. We discuss the suggestion that the waves are upward-propagating acoustic waves.
引用
收藏
页码:L121 / L124
页数:4
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