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| Paper: |
Jet Phenomena in the Solar Atmosphere caused by Interaction between Emerging Flux and Coronal Fields |
| Volume: |
325, The Solar-B Mission and the Forefront of Solar Physics |
| Page: |
69 |
| Authors: |
Miyagoshi, T.; Yokoyama, T.; Isobe, H.; Shibata, K. |
| Abstract: |
We have studied jet phenomena in the solar atmosphere with MHD numerical simulations. Emerging flux could interact coronal magnetic fields through magnetic reconnection. Then, magnetic energy is released and magnetic topology drastically changes. Our numerical simulation results show that coronal jets are produced through this process. |
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