Synoptic Maps of Subphotospheric Flows

preliminary page - under development

Synoptic maps of subphotospheric flows are obtained by the method of time-distance helioseismology using the full-disk Doppler images from the MDI instrument on SOHO. These data are currently available only during MDI Dynamics Campaigns, for 2-3 months every year since 1996. This data analysis is under development, and at this moment we provide only an example of these maps. For questions or comments e-mail to Junwei Zhao or Alexander Kosovichev
Carrington Rotation depth 0-3 Mm
1923 PS;   GIF;  
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