Abstract
The Helioseismic and Magnetic Imager onboard Solar Dynamics Observatory provides uninterrupted high-resolution observations of solar oscillations over the entire disk. This gives a unique opportunity for mapping subsurface flows and wave-speed structures and investigating their role in the Sun's dynamics and magnetic activity on various scales by methods of local helioseismology. A data analysis pipeline for the time-distance helioseismology analysis has been developed and implemented at the SDO Joint Science Operation Center (JSOC) at Stanford. It provides near-real time processing of the helioseismology data. We provide an overview of this pipeline, including the data flow procedures, measurement and inversion codes, and our data products.
Original language | English (US) |
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Article number | 012063 |
Journal | Journal of Physics: Conference Series |
Volume | 271 |
Issue number | 1 |
DOIs | |
State | Published - 2011 |
Externally published | Yes |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy