Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008apj...689..593c&link_type=abstract
The Astrophysical Journal, Volume 689, Issue 1, pp. 593-612.
Astronomy and Astrophysics
Astronomy
22
Methods: Data Analysis, Sun: Atmospheric Motions, Techniques: Image Processing
Scientific paper
A time sequence of high-quality images currently produced by high-resolution observations either from the ground or in space may be utilized to determine the transverse flow field on the plane of the sky with the help of optical flow techniques. We have examined the performance of three different methods-a well-known technique called local correlation tracking (LCT), a recently developed technique called the differential affine velocity estimator (DAVE), and a new technique called the nonlinear affine velocity estimator (NAVE)-using three kinds of image data: mapping-based synthetic images, a set of MHD simulation data, and real images (magnetograms) taken by the Solar Optical Telescope on board Hinode. We have generalized the model equation of image evolution by adding to the continuity equation a source term that is proportional to the image value. Synthetic images were constructed based on the analytical solution of this equation with different velocity profiles: uniform, affine, or nonaffine. The tests with the synthetic data indicated that NAVE is very good at detecting subpixel motions, superpixel motions, and nonuniform motions, while LCT is not good at detecting nonuniform motions, especially around critical points, and the performance of DAVE is degraded in the presence of superpixel motions. In all the methods, the performance became worse as the velocity field deviated more from an affine one. We also found that the MHD simulation data we used are not quite suited for discriminating between the three methods, maybe because the data do not contain enough structural information to be used for tracing. In contrast, the determination of velocity fields from the real image data was somewhat sensitive to the technique adopted. The technique of NAVE with the source term produced velocity fields that are the most consistent with the data.
Chae Jongchul
Sakurai Takashi
No associations
LandOfFree
A Test of Three Optical Flow Techniques-LCT, DAVE, and NAVE 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 A Test of Three Optical Flow Techniques-LCT, DAVE, and NAVE, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Test of Three Optical Flow Techniques-LCT, DAVE, and NAVE will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1102179