Variations in Rotation Rate Within the Solar Convection Zone From GONG and MDI 1995-2000

Details Variations in Rotation Rate Within the Solar Convection Zone From GONG and MDI 1995-2000 Variations in Rotation Rate Within the Solar Convection Zone From GONG and MDI 1995-2000

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sp31a15h&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SP31A-15

Physics

7522 Helioseismology

Scientific paper

Helioseismic measurements with the Michelson Doppler Imager (MDI) instrument aboard SOHO, and complementary measurements from the Global Oscillation Network Group (GONG) project, are revealing changes deep within the Sun as the solar cycle progresses. We will present the latest results based on recent data from both experiments, including flows in the upper part of the convection zone and variations in the rotation rate near its base.

Affiliated with

Also associated with

No associations

Rating

Variations in Rotation Rate Within the Solar Convection Zone From GONG and MDI 1995-2000 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 Variations in Rotation Rate Within the Solar Convection Zone From GONG and MDI 1995-2000, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variations in Rotation Rate Within the Solar Convection Zone From GONG and MDI 1995-2000 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1279120