Helioseismology of Time-Varying Flows Through The Solar Cycle

Details Helioseismology of Time-Varying Flows Through The Solar Cycle Helioseismology of Time-Varying Flows Through The Solar Cycle

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004soph..224..217g&link_type=abstract

Solar Physics, Volume 224, Issue 1-2, pp. 217-228

Physics

28

Scientific paper

Flows in the upper convection zone are measured by helioseismology on a wide variety of scales. These include differential rotation and meridional circulation, local flows around complexes of magnetic activity and sunspots, and convective flows. The temporal evolution of flows through cycle 23 reveals connections between mass motions in the solar interior and the large-scale characteristics of the magnetic cycle. Here I summarize the latest observations and their implications. Observations from local helioseismology suggest that subsurface flows around active regions introduce a solar-cycle variation in the meridional circulation.

Affiliated with

Also associated with

No associations

Rating

Helioseismology of Time-Varying Flows Through The Solar Cycle 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 Helioseismology of Time-Varying Flows Through The Solar Cycle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Helioseismology of Time-Varying Flows Through The Solar Cycle will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1806962