The linear transport model for the proton aurora developed at the Air Force
Research Laboratory is reviewed. Emphasis is given on the discussion of th
e studies where the predictions of the model were compared with those of ot
her theoretical methods and with the available data. The excellent agreemen
t between the linear transport model and other theoretical methods gives cr
edence to the accuracy of the numerical technique adopted in solving the tr
ansport equations, while good to excellent agreements between theory and ob
servations indicate that the transport model adequately describes the impor
tant physics issues of the problem. It is concluded here that our ability t
o accurately model the proton aurora is limited only by the uncertainties i
n the input cross-section data (for some collision processes) and by our in
adequate information about the incident proton spectra. Some discussions in
this regard are included.