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Solar Photospheric Magnetic Reconnection by Olmnop is a document available to read on EtoBox.

What is Solar Photospheric Magnetic Reconnection about?

1. The document investigates photospheric magnetic reconnection through 2.5-dimensional MHD simulations of oppositely directed vertical magnetic flux sheets encountering each other. 2. A resistivity model with a maximum at the temperature-minimum region is used, allowing Sweet-Parker type reconnection to occur around this height. 3. The reconnection generates upward propagating MHD slow mode waves, with an energy flux of 1010 erg/cm2/s that could help power solar spicules. When the initial field is incli

Author

Olmnop

Language

EN