Response of the Coronal N-S Asymmetry to its Manifestations in the Photosphere

Details Response of the Coronal N-S Asymmetry to its Manifestations in the Photosphere Response of the Coronal N-S Asymmetry to its Manifestations in the Photosphere

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...8e..22r&link_type=abstract

Solar and Stellar Activity Cycles, 26th meeting of the IAU, Joint Discussion 8, 17-18 August 2006, Prague, Czech Republic, JD08,

Computer Science

Scientific paper

The North-South (N-S) asymmetries of three solar activity indices are mutually compared over the period of more than five solar cycles (1945 - 2001). Our own catalogue of the hemispheric sunspot numbers, the database of the uniform coronal green line brightness and the magnetic field strength, as derived from the NSO/KP data (1975-2001), are treated within the discrete latitudinal zones (5° - 30° and 35° - 60°). The calculated paired correlations and regressions reveal much better expressed mutual relations between the N-S asymmetries than those are manifested if using the indices alone. A distinctly different behaviour of the N-S asymmetries found at different solar cycle phases separately for the low- and mid-latitude zones is picked out. The revealed differences could be considered when any dynamo theories of solar activity are developed.

Affiliated with

Also associated with

No associations

Rating

Response of the Coronal N-S Asymmetry to its Manifestations in the Photosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Response of the Coronal N-S Asymmetry to its Manifestations in the Photosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Response of the Coronal N-S Asymmetry to its Manifestations in the Photosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1784122