LONG-PERIOD NETWORK OSCILLATIONS IN THE SOLAR CHROMOSPHERE

被引:22
|
作者
LOU, YQ
机构
关键词
MHD; SUN; CHROMOSPHERE; MAGNETIC FIELDS; OSCILLATIONS; TRANSITION REGION;
D O I
10.1093/mnras/274.1.L1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent observations of solar chromospheric oscillations have revealed two different types: 3-min intranetwork oscillations above the supergranule cells; and long-period (similar to 5 to 20 min) oscillations associated with the bright chromospheric network. It has been speculated previously that the long-period network oscillations could be somehow related to low-frequency magneto-gravity waves in magnetized boundary lanes surrounding supergranules. We explore this scenario and examine its feasibility, as well as constraints based on a magnetohydrodynamic (MHD) model for the long-period solar network oscillations.
引用
收藏
页码:L1 / L4
页数:4
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