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On 15 August 1991 a modification was made to the BATSE analysis software to take
into account the increased absorption by the aluminum window as the detectors
become more oblique to the Sun.  Previously, we were only taking into account
the change in geometric area as a function of the obliquity.  In the standard
flare plots, the flare count rate has been normalized to that of a single BATSE
LAD with the Sun directly along the detector axis.  As a result, all of the
standard flare plots have been redrawn, and the peak rate and total count
entries in the BATSE flare catalog have been recalculated.  Also, the most
intense flares sometimes have detector rates which cannot be corrected due to
extreme deadtime and/or pulse-pileup effects.  The standard flare plots for 
these events have labels to warn users of this possibility.

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