Multiscale analysis of active region evolution
Flows in the photosphere of solar active regions are turbulent in nature. Because magnetic fields are frozen into the plasma on the solar surface, magnetograms can be used to investigate the processes responsible for structuring active regions. Here, a continuous wavelet technique is developed, anal...
| Main Authors: | , , , , , , |
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| 格式: | Conference item |
| 出版: |
2008
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