Cycle 24 - An Inside Perspective

Details Cycle 24 - An Inside Perspective Cycle 24 - An Inside Perspective

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.3501s&link_type=abstract

American Astronomical Society, SPD meeting #40, #35.01; Bulletin of the American Astronomical Society, Vol. 41, p.867

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Scientific paper

One of the prime goals for SDO is to increase understanding of the processes that generate dynamical magnetic disturbances that are the proximate cause of "space weather." Existing helioseismic series from GONG and SOHO/MDI cover the full span of cycle 23. One must ask what can we accomplish with another five years. Solar minimum is a good time to begin a new set of observations. Due to extreme patience on the part of the Sun, SDO is scheduled to be in place to allow observations near the beginning of cycle 24. SDO/HMI should provide modest improvement for global scale measurements and significant improvement for near surface studies. This talk will provide a brief overview of what we know about magnetic fields in the interior and what we hope to learn with SDO.

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