Extending Global Helioseismic Measurements From MDI to HMI

Details Extending Global Helioseismic Measurements From MDI to HMI Extending Global Helioseismic Measurements From MDI to HMI

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.1605s&link_type=abstract

American Astronomical Society, SPD meeting #42, #16.05; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

With the end of regular observations using MDI the question arises if we can provide good continuity between MDI and HMI. In particular MDI has shown intriguing differences in the torsional oscillation between the two most recent 11-year solar cycles. In this poster we will discuss some of the instrumental differences as well as examine the differences in global mode parameters and inferred quantities between the two during the period of overlap of MDI and HMI observations.
This work is supported by NASA contract NAS5-02139 to Stanford University.

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