Table 1:
Source widths (half intensity) and flux density of the flare emission at 11:10 UT (extended phase). Note the significantly larger diameter at the higher frequency.
Table 2:
Power-law parameters of the fitted hard X-ray spectra during phases II and III. The spectral indices deduced from gyrosynchrotron modelling are also given.
11:10 UT (extended phase). Note the significantly larger diameter at the higher frequency.