A quantitative study of magnetic flux transport on the Sun

Details A quantitative study of magnetic flux transport on the Sun A quantitative study of magnetic flux transport on the Sun

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983iaus..102....2s&link_type=abstract

Presented at the IAU Symp. No. 102 on Solar and Stellar Magnetic Fields: Origins and Coronal Effects, Zurich, 2-6 Aug. 1982

Statistics

Computation

1

Magnetic Fields, Magnetic Flux, Solar Activity, Quantitative Analysis, Sun

Scientific paper

A computational model, based on diffusion, differential rotation, and meridional flow, has been developed to simulate the transport of magnetic flux on the Sun. Using Kitt Peak magnetograms as input, as have determined a best-fit diffusion constant by comparing the computed and observed fields at later times. This paper presents the initial results of a project to simulate the transport of solar magnetic flux using diffusion, differential rotation, and meridional flow. The study concerns the evolution of large-scale fields on a time scale of weeks of years, and ignores the rapid changes that accompany the emergence of new magnetic regions and the day-to-day changes of the supergranular network itself.

Affiliated with

Also associated with

No associations

Rating

A quantitative study of magnetic flux transport on the Sun 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 A quantitative study of magnetic flux transport on the Sun, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A quantitative study of magnetic flux transport on the Sun will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1306403