Polar Coronal Structures and the Global Magnetic Field Evolution Through the Cycle

Details Polar Coronal Structures and the Global Magnetic Field Evolution Through the Cycle Polar Coronal Structures and the Global Magnetic Field Evolution Through the Cycle

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004soph..224..277f&link_type=abstract

Solar Physics, Volume 224, Issue 1-2, pp. 277-284

Physics

3

Scientific paper

We compare the shape and position of some plasma formations visible in the polar corona with the cyclic evolution of the global magnetic field. The first type of object is polar crown prominences. A two-fold decrease of the height of polar crown prominences was found during their poleward migration from the middle latitudes to the poles before a polar magnetic field reversal. The effect could be assigned to a decrease of the magnetic field scale. The second type of object is the polar plumes, ray like structures that follow magnetic field lines. Tangents to polar ray structures are usually crossed near some point, “a magnetic focus,” below the surface. The distance q between the focus and the center of the solar disk changes from the maximum value about 0.65 R &sun; at solar minimum activity to the minimum value about 0.45 R &sun; at solar maximum. At first glance this behaviour seems to be contrary to the dynamics of spherical harmonics of the global magnetic field throughout a cycle. We believe that the problem could be resolved if one takes into account not only scale changes in the global magnetic field but also the phase difference in the cyclic variations of large-scale and small-scale components of the global field.

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