The time-resolved spectra of several gamma-ray bursts have shown that near
the beginning of the burst, some absorption mechanism makes the spectra inc
onsistent with the simple optically-thin synchrotron shock model. We fit GR
B 970111, which shows strong evidence for such absorption, with a synchrotr
on shock spectra suffering self-absorption. The synchrotron self-absorption
shape does fit the BATSE time-evolving spectra, although it may be inconsi
stent with BeppoSAX WFC data. If the turnover just below the spectral break
is due to synchrotron self-absorption, a magnetic field strength of 4 10(7
) G is required.