Fig. 6
From: On the effect of model mismatch for sequential Info-Greedy Sensing
Recovery of solar flare images of size 224 by 288 with K=90 measurements and no sensing noise. We used the first 50 frames to estimate the mean and covariance matrix of a single Gaussian. a original image for 300th frame. b Ordered relative recovery error of the 200th to the 300th frames. c Recovered the 300th frame using random measurement. d Recovered the 300th frame using Info-Greedy Sensing