The solar rotation rate from solar minimum to maximum

Details The solar rotation rate from solar minimum to maximum The solar rotation rate from solar minimum to maximum

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508...59b&link_type=abstract

In: Proceedings of the SOHO 11 Symposium on From Solar Min to Max: Half a Solar Cycle with SOHO, 11-15 March 2002, Davos, Switze

Physics

2

Sun: Oscillations, Sun: Rotation, Sun: Interior

Scientific paper

Frequency splittings obtained from GONG and MDI observations over the last 6 years are used to study how the rotation rate in the solar convection zone has evolved with time. The pole rotation rate is found to have had a minimum in 1999, distinctly before the maximum solar activity. The bands of faster and slower than average rotation rate are found to move towards the equator at low latitudes and towards the poles at high latitudes.

Affiliated with

Also associated with

No associations

Rating

The solar rotation rate from solar minimum to maximum 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 rotation rate from solar minimum to maximum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The solar rotation rate from solar minimum to maximum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1893838