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Fig. 3

image

Composite images for Stokes I at 327 MHz on Aug. 27, 2002 at 08:27:43. The color scales are linear BW. In the right frame, the image is saturated at 32% of its maximum. The limits of the field of view (units of R) is (−0.25, + 0.80) for EW and (−0.80,0.00) for NS. The solid line is the solar limb. The storm near the western limb is simple. The storms near the center of the disk are more extended. The aspect of the main storm in Stokes V (not shown) is similar to that in Stokes I. The vertical bars on the left side of images are proportional to log (TBmax), with TBmax ranging from 106 K at the bottom of the frame, to 1010 K at its top. Negative artifacts have been suppressed for giving a dark background at zero level. The relative value of the deepest negative artifact is proportional to the length of the vertical bars on the right side, with ticks at 10% and 20%. Same for Figs. 4 and 5.

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