Update for this week
I realised that I forgot to point out a critical factor for the
formula stated in the above post:
D = (6x10³ * d / fc) * (sqrt(b / tp))
It is unknown what the value of bitrate (b) actually represents, it
could be:
1) The average desired bitrate
2) The maximum bitrate (when the satellite is directly overhead -
lowest noise)
3) The minimum bitrate (when the satellite is near the horizon -
greatest noise)
Depending on which of these is the correct, the results change wildly.
If it were an average then the results would be similar to those above
(as the decrease in noise when overhead should balance with the
increase near the horizon). If it is the maximum bitrate, then the
antenna would have to be even bigger, whereas if it were a minimum the
antenna diameter could be reduced.
Because of these uncertainties, I think it may be best to ignore the
results derived from this formula until all the variables can be
better established. It would be helpful if someone could find the
formula described elsewhere, preferably with a better description.
Steve had this to say:
We can always trade off antenna size for additional gain in the low-
noise amplifier stages. Of course, this is limited by the noise
temperature of the low-noise amplifier stage, so perhaps if we looked
to see what LNA gains/noise-temperatures are possible (ie. cutting
edge of research), and then look at what is generally commercially
available, then we might find that we have plenty of noise-headroom to
get another 8x or 16x gain out of the LNA's, thus decreasing the dish
size by the same amount - and suddenly you only need a 0.75m diameter
dish. And if that's the case, the antenna becomes pretty insignificant
and I guess it would be a lot easier for your department to justify it
to all the other people who might object (central university buildings
people/safety people/finance people etc...).