Time-distance helioseismology pipeline generates subsurface horizontal flow-field maps and wave-speed perturbation maps for full-disk Sun and for selected active regions. All results are obtained from an 8-hour period, and covers 30° x 30° horizontally and 0 -- 20 Mm in depth.
The basic procedure for the time-distance data-analysis pipeline is as follows:
Thus, our products include two sets of acoustic travel times and four sets of inversion results in both flow fields and wave-speed perturbation fields.
For full-disk data, 25 areas are selected and are processed separately. Each day is divided into three 8-hr periods: 00:00 -- 07:59UT, 08:00 -- 15:59UT, and 16:00 -- 23:59UT. For each of these 25 areas and for each time period, we provide fitted travel times and inverted flow fields and wave-perturbations.
Full-disk flow map and wave-perturbation map are then made by merging these 25 areas. Data sequence yet to be defined.
Detailed procedure and description of results can be found in the paper : Time-Distance Helioseismology Data-Analysis Pipeline for Helioseismic and Magnetic Imager Onboard Solar Dynamics Observatory (SDO/HMI) and Its Initial Results
For details of the travel-time fittings and comparion of different fitting methods, please refer to the paper:
Implementation and Comparison of Acoustic
Travel-Time Measurement Procedures for the Solar Dynamics Observatory/Helioseismic and Magnetic Imager Time-Distance Helioseismology Pipeline