Observational Study of Solar Magnetic Active Phenomena

Details Observational Study of Solar Magnetic Active Phenomena Observational Study of Solar Magnetic Active Phenomena

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006japa...27..305z&link_type=abstract

Journal of Astrophysics and Astronomy, vol. 27, no.2 & 3 P. 305-314

Astronomy and Astrophysics

Astrophysics

Sun: Activity, Flares, Magnetic Fields.

Scientific paper

The electric current separated into two parts reflected the quantative properties of heterogeneity and chirality of magnetic field, and defined them as the shear and twist components of current. We analyze the basic configuration and evolution of superactive region NOAA 6580- 6619-6659. It is found that the contribution of the twist component of current cannot be reflected in the normal analysis of the magnetic shear and gradient of the active regions. The observational evidence of kink magnetic ropes generated from the subatmosphere cannot be found completely in some super delta active regions.

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