High-frequency oscillations in a solar active region coronal loop
High-frequency oscillations in a solar active region coronal loop
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DOI：
10.1046/j.1365-8711.2001.04491.x
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发表时间：
2001-09
影响因子：
4.8
通讯作者：
David R. Williams;K. Phillips;P. Rudawy;M. Mathioudakis;P. Gallagher;E. O'Shea;F. Keenan;P. Read-P
中科院分区：
文献类型：
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作者：
David R. Williams;K. Phillips;P. Rudawy;M. Mathioudakis;P. Gallagher;E. O'Shea;F. Keenan;P. Read-P
日食日冕成像系统 (SECIS) 用于记录 1999 年 8 月 11 日日全食期间的日冕高频率观测。在 2 分 23.5 秒的全食期间，两个通道同时记录了 6364 张图像：白光通道和 Fe XIV (5303 A°)“绿线”通道 (cid:133) T , 2 MK （用户ID：134）。在这里，我们报告 SECIS 实验的初步结果，包括在活动区域日冕环中发现 6 秒强度振荡。
The Solar Eclipse Corona Imaging System (SECIS) was used to record high-cadence observations of the solar corona during the total solar eclipse of 1999 August 11. During the 2 min 23.5 s of totality, 6364 images were recorded simultaneously in each of the two channels: a white light channel, and the Fe XIV (5303 A ˚ ) ‘green line’ channel (cid:133) T , 2 MK (cid:134) . Here we report initial results from the SECIS experiment, including the discovery of a 6-s intensity oscillation in an active region coronal loop.