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Multi-channel observations of plasma outflows and the associated small-scale magnetic field cancellations on the edges of an active region

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Abstract

With the SDO/AIA instrument, continuous and intermittent plasma outflows are observed on the boundaries of an active region along two distinct open coronal loops. By investigating the temporal sequence magnetograms obtained from HMI/SDO, it is found that a small-scale magnetic reconnection probably plays an important role in the generation of the plasma outflows in the coronal loops. It is found that the origin of the plasma outflows coincides with the locations of the small-scale magnetic fields with mixed polarities, which suggests that the plasma outflows along coronal loops probably results from the magnetic reconnection between the small-scale closed emerging loops and the large-scale open active region coronal loops.

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Acknowledgements

This work is supported by the National Basic Research Program of China under grant 2011CB8114001, the Natural Science Foundation of China (Grant Nos. 11373040, 11203036, 11125314, 11173033, 11103037, 11103038, 11221063 and 11178016) and Important Directional Projects of Chinese Academy of Sciences (Grant No. KLCX2-YW-T04).

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Liu, S., Su, J.T. Multi-channel observations of plasma outflows and the associated small-scale magnetic field cancellations on the edges of an active region. Astrophys Space Sci 351, 417–425 (2014). https://doi.org/10.1007/s10509-014-1853-7

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  • DOI: https://doi.org/10.1007/s10509-014-1853-7

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