  The Brighter-Fatter (hereafter BF) effect in CCD sensors causes increases in
the image size of bright objects due to electrostatic repulsion of collected
charges. Correcting this effect in the LSST camera is required in order to meet
the science goals of the project, especially galaxy shape measurements for weak
lensing. The current plan for BF image correction in the LSST is to use the
deconvolution method described in Coulton, et.al. [1]. In this work, we study
the linearity of the BF effect and effectiveness of the Coulton correction,
using both simulation tools and measurements made on prototype LSST CCDs from
both CCD vendors. We conclude that the proposed image correction method may be
adequate to meet the LSST science goals, although more work is needed on the
algorithms used to generate the image correction kernel from sensor
measurements.
