2/1/2017 1
Motion and optical flow
Thurs Feb 2, 2017 Kristen Grauman UT Austin
Announcements
- A1 due tomorrow, Friday
- Due to AAAI travel
Motion and optical flow Thurs Feb 2, 2017 Kristen Grauman UT - - PDF document
2/1/2017 Motion and optical flow Thurs Feb 2, 2017 Kristen Grauman UT Austin Announcements A1 due tomorrow, Friday Due to AAAI travel Office hours Tues Feb 7 cancelled (by appt) Lecture Tues is ON as normal 1 2/1/2017
Figure from Michael Black, Ph.D. Thesis
points closer to the camera move more quickly across the image plane
Zoom out Zoom in Pan right to left
image brightness variations
Figure from Horn book
– given a pixel in H, look for nearby pixels of the same color in I
– For grayscale images, this is brightness constancy
Slide credit: Steve Seitz
Figure by Michael Black
Slide credit: Steve Seitz
Slide credit: Steve Seitz
Slide credit: Steve Seitz
Figure by Michael Black
Slide credit: Steve Seitz
Prob: we have more equations than unknowns
Solution: solve least squares problem
Slide credit: Steve Seitz
TA should be invertible
TA should not be very small
– eigenvalues l1 and l2 of A
TA should not be very small
TA should be well-conditioned
– l1/ l2 should not be too large (l1 = larger eigenvalue)
Slide by Steve Seitz, UW
– gradients very large or very small – large l1, small l2
Slide credit: Steve Seitz
– small l1, small l2
Slide credit: Steve Seitz
– large l1, large l2
Slide credit: Steve Seitz
http://www.fxguide.com/article333.html
http://www.fxguide.com/article333.html
image brightness variations
Liu et al. SIGGRAPH 2005
to a single ray in space
255
Alyosha Efros, CMU
Alyosha Efros, CMU
Alyosha Efros, CMU
Slide credit: Birgi Tamersoy
Slide credit: Birgi Tamersoy
Slide credit: Birgi Tamersoy Slide credit: Birgi Tamersoy
Slide credit: Birgi Tamersoy
Slide credit: Birgi Tamersoy
Alyosha Efros, CMU
Alyosha Efros, CMU
Adaptive Background Mixture Models for Real-Time Tracking, 1999, Chris Stauer & W.E.L. Grimson
Slide credit: Kristen Grauman