Initial Results from SDO/HMI Time-Distance Helioseismology Data Analysis Pipeline

Details Initial Results from SDO/HMI Time-Distance Helioseismology Data Analysis Pipeline Initial Results from SDO/HMI Time-Distance Helioseismology Data Analysis Pipeline

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh14a..08z&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH14A-08

Astronomy and Astrophysics

Astrophysics

[7522] Solar Physics, Astrophysics, And Astronomy / Helioseismology, [7594] Solar Physics, Astrophysics, And Astronomy / Instruments And Techniques

Scientific paper

The Helioseismic and Magnetic Imager on Solar Dynamics Observatory provides uninterrupted high-resolution observations of solar oscillations over the entire disk. Time-distance helioseismology data analysis pipeline was developed to perform a near real-time analysis of these observations, and provide full-disk subsurface flow fields and wave-speed perturbation maps every 8 hours. These routine productions give us substantial information of the solar interior, and are very useful to study the solar interior dynamics, connections between subsurface dynamics and photospheric activities, and solar large-scale and global-scale flows and structures. We present our initial results in these respects.

Affiliated with

Also associated with

No associations

Rating

Initial Results from SDO/HMI Time-Distance Helioseismology Data Analysis Pipeline does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Initial Results from SDO/HMI Time-Distance Helioseismology Data Analysis Pipeline, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Initial Results from SDO/HMI Time-Distance Helioseismology Data Analysis Pipeline will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1507652