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Coronal quasi-periodic fast-propagating magnetosonic waves observed by SDO/AIA

Published online by Cambridge University Press:  09 September 2016

Yuandeng Shen*
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China email: [email protected]
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Abstract

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Coronal quasi-periodic fast-propagating (QFP) magnetosonic waves are scare in previous studies due to the relative low temporal and spatial resolution of past telescopes. Recently, they are detected by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO). Here, two cases of QFP waves are presented. The analysis results indicate that QFP waves are tightly associated with the associated flares. It is indicate that QFP waves and the associated flares are possibly driven by the same physic process such as quasi-periodic magnetic reconnection process in producing flares.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

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