Backprojection filtering algorithms are presented for three variable o
rbit fan-beam geometries. Expressions for the fan-beam projection and
backprojection operators are given for a flat detector fan-beam geomet
ry with fixed focal length, with variable focal length, and with fixed
focal length and off-center focusing. Backprojection operators are de
rived for each geometry using transformation of coordinates to transfo
rm from a parallel geometry backprojector to a fan-beam backprojector
for the appropriate geometry. The backprojection operator includes a f
actor which is a function of the coordinates of the projection ray and
the coordinates of the pixel in the backprojected image. The backproj
ection filtering algorithm first backprojects the variable orbit fan-b
eam projection data using the appropriately derived backprojector to o
btain a 1/r blurring of the original image, then takes the two-dimensi
onal (2D) Fast Fourier Transform (FFT) of the backprojected image, the
n multiples the transformed image by the 2D ramp filter function, and
finally takes the inverse 2D FFT to obtain the reconstructed image. Co
mputer simulations verify that backprojectors with appropriate weighti
ng give artifact free reconstructions of simulated line integral proje
ctions. Also, it is shown that it is not necessary to assume a project
ion model of line integrals, but the projector and backprojector can b
e defined to model the physics of the imaging detection process. A bac
kprojector for variable orbit fan-beam tomography with fixed focal len
gth is derived which includes an additional factor which is a function
of the flux density along the hat detector. It is shown that the impu
lse response for the composite of the projection and backprojection op
erations is equal to 1/r.