The solar dynamo in the light of the distribution of various sunspot magnetic classes over butterfly diagram

Details The solar dynamo in the light of the distribution of various sunspot magnetic classes over butterfly diagram The solar dynamo in the light of the distribution of various sunspot magnetic classes over butterfly diagram

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010an....331...82s&link_type=abstract

Astronomische Nachrichten, Vol.331, Issue 1, p.82

Statistics

2

Magnetic Fields, Sun: Activity, Sunspots

Scientific paper

We present the data concerning the distribution of various sunspot magnetic classes over the solar butterfly diagram and discuss how this data can inform solar dynamo models. We use the statistics of sunspots that violate the Hale polarity law to estimate the ratio of the fluctuating and mean components of the toroidal magnetic field inside the solar convective zone. An analysis of the spatial distribution of bipolar, unipolar and complex sunspot groups in the context of simple dynamo models results in the conclusion that the mean toroidal field is relatively simple and maintains its shape during the course of the solar cycle.

Affiliated with

Also associated with

No associations

Rating

The solar dynamo in the light of the distribution of various sunspot magnetic classes over butterfly diagram 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 The solar dynamo in the light of the distribution of various sunspot magnetic classes over butterfly diagram, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The solar dynamo in the light of the distribution of various sunspot magnetic classes over butterfly diagram will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1888885