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Slow reconnection - PowerPoint PPT Presentation

Magnetic reconnection in stars: fast and slow

Magnetic reconnection in stars: fast and slow. D. J. Mullan University of Delaware, Newark DE USA. Flares in stars. Flare: a transient increase in brightness In the Sun, flares occur in magnetic regions. Flare stars are known to have strong surface fields.

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414 views • 29 slides

Solar Eruption Onset: Where Does the Action Begin?

Solar Eruption Onset: Where Does the Action Begin?. Alphonse C. Sterling UAT/NASA/MSFC/NSSTC/ISAS. Eruptions on the Sun involve the sudden release of large amounts of energy. Where does the main energy release occur, and where are the key regions that are involved? Two possibilities:

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259 views • 18 slides

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Slow reconnection - PowerPoint PPT Presentation

Magnetic reconnection in stars: fast and slow

Solar Eruption Onset: Where Does the Action Begin?