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Propagating disturbances along fan-like coronal loops in an active region
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作者 sudip mandal Tanmoy Samanta +2 位作者 Dipankar Banerjee S.Krishna Prasad Luca Teriaca 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2015年第11期1832-1842,共11页
Propagating disturbances are often observed in active region fan-like coronal loops. They were thought to be due to slow mode magnetohydrodynamic waves based on some of the observed properties. However, recent studies... Propagating disturbances are often observed in active region fan-like coronal loops. They were thought to be due to slow mode magnetohydrodynamic waves based on some of the observed properties. However, recent studies involving spectroscopy indicate that they could be due to high speed quasi-periodic upflows which are difficult to distinguish from upward propagating slow waves. In this context, we have studied a fan loop structure in the active region AR 11465 using simultaneous spectroscopic and imaging observations from the Extreme Ultraviolet Imaging Spectrometer onboard Hinode and Atmospheric Imaging Assembly onboard Solar Dynamics Observatory. Analysis of the data shows significant oscillations at different locations. We explore the variations in different line parameters to determine whether the waves or flows could cause these oscillations to improve the current understanding of the nature of these disturbances. 展开更多
关键词 wavelet simultaneous distinguish Extreme propagating Solar fitting pixel spectroscopic Roberts
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