Views of the Solar Torsional Oscillation

Details Views of the Solar Torsional Oscillation Views of the Solar Torsional Oscillation

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp41a..05h&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SP41A-05

Physics

7522 Helioseismology, 7536 Solar Activity Cycle (2162)

Scientific paper

The pattern of zonal flows migrating towards the equator over the solar cycle, known as the torsional oscillation, is well established from both helioseismology and surface Doppler measurements. However, the exact appearance of the pattern will vary depending on the form of the overall rotation profile that has been subtracted, even when the data cover a full eleven-year cycle. Here we compare the appearance of the flow pattern when applying several different methods to the MDI and GONG data for Solar Cycle 23.

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