Time-distance helioseismology data-analysis pipeline for helioseismic and magnetic imager onboard solar dynamics observatory (SDO/HMI) and its initial results

J. Zhao, S. Couvidat, R. S. Bogart, K. V. Parchevsky, A. C. Birch, T. L. Duvall, J. G. Beck, A. G. Kosovichev, P. H. Scherrer

Research output: Chapter in Book/Report/Conference proceedingChapter

Abstract

The Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory (SDO/HMI) provides continuous full-disk observations of solar oscillations. We develop a data-analysis pipeline based on the time-distance helioseismology method to measure acoustic travel times using HMI Doppler-shift observations, and infer solar interior properties by inverting these measurements. The pipeline is used for routine production of near-real-time full-disk maps of subsurface wave-speed perturbations and horizontal flow velocities for depths ranging from 0 to 20 Mm, every eight hours. In addition, Carrington synoptic maps for the subsurface properties are made from these full-disk maps. The pipeline can also be used for selected target areas and time periods. We explain details of the pipeline organization and procedures, including processing of the HMI Doppler observations, measurements of the travel times, inversions, and constructions of the full-disk and synoptic maps. Some initial results from the pipeline, including full-disk flow maps, sunspot subsurface flow fields, and the interior rotation and meridional flow speeds, are presented.

Original languageEnglish (US)
Title of host publicationThe Solar Dynamics Observatory
PublisherSpringer US
Pages375-390
Number of pages16
Volume9781461436737
ISBN (Electronic)9781461436737
ISBN (Print)1461436729, 9781461436720
DOIs
StatePublished - Nov 1 2012
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Keywords

  • Sun: SDO
  • Sun: helioseismology
  • Sun: oscillations

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