Currently, pointing loss is determined by a function built-in to the telescope object. This assumes that beams are gaussian. However, other kinds of beam with other intensity distributions are possible and will have slightly different pointing losses for the same rms jitter.
Therefore, some method of implementing different intensity distributions (e.g. flat-top beams) will be necessary. Most notably for modelling the downlink beacon from the satellite, which has a flat-top intensity distribution.
Currently, pointing loss is determined by a function built-in to the telescope object. This assumes that beams are gaussian. However, other kinds of beam with other intensity distributions are possible and will have slightly different pointing losses for the same rms jitter.
Therefore, some method of implementing different intensity distributions (e.g. flat-top beams) will be necessary. Most notably for modelling the downlink beacon from the satellite, which has a flat-top intensity distribution.