Does the solar magnetic flux depends on boundary conditions?

Details Does the solar magnetic flux depends on boundary conditions? Does the solar magnetic flux depends on boundary conditions?

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh11a1490c&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SH11A-1490

Astronomy and Astrophysics

Astrophysics

[7509] Solar Physics, Astrophysics, And Astronomy / Corona, [7526] Solar Physics, Astrophysics, And Astronomy / Magnetic Reconnection

Scientific paper

The open flux of the heliosphere is thought to have a floor value during solar minimum. It has been suggested that CMEs increase the total amount of observed flux during solar maximum. This increase is temporary however, presumably due to the fact that CMEs undergo interchange reconnection with the ambient open flux, so that the total open flux of the Sun might be a conserved quantity. We argue that the view on the amount of open flux highly depends on both the inner and outer boundary conditions of the heliospheric system. We demonstrate this argument using a numerical simulation of a real CME event.

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