The combination of high resolution, spatial coverage, and continuity of photospheric Doppler and other data from HMI has allowed us to embark on a program of systematic exploration of solar subsurface flows and thermal structure variations using the technique of ring-diagram analysis on an unprecedented scale. There are two ring-diagrams pipelines, as described in [1]. In this paper we discuss the synoptic pipeline execution and describe the data being processed and produced. © Published under licence by IOP Publishing Ltd.
CITATION STYLE
Bogart, R. S., Baldner, C., Basu, S., Haber, D. A., & Rabello-Soares, M. C. (2011). HMI ring diagram analysis II. Data products. In Journal of Physics: Conference Series (Vol. 271). Institute of Physics Publishing. https://doi.org/10.1088/1742-6596/271/1/012009
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