Hi Anthony. There are generally two ways to compute the seeing FWHM,
neither of which can be done very well using the PHD2 data. The best
approach is with a seeing monitor and that's typically what's used at remote
observatories. Lacking that, you can roughly measure it yourself by
shooting a series of 5-10 sec exposures with your main imaging camera and
computing the average stellar FWHM. That assumes, of course, that your
image scale is no larger than about 30% of the expected seeing value. So
accurately measuring a seeing FWHM of 2.0 arc-sec will probably require an
image scale of around 0.6 arc-sec/px - and certainly not more than 1
arc-sec/px. This approach also assumes that the optics are well collimated
and aligned and capable of producing small Airy disks whose size is actually
seeing-limited.
The FWHM values displayed by the Star Profile tool aren't very useful for
getting a quantitative measure of the seeing. The two things are related but
not translatable in a reliable way. The closest thing in PHD2 is the
measurement done by the Guiding Assistant. But that is directed toward
setting a min-move, in pixels, below which the guide star movement is
dominated by seeing effects.
Hope this helps,
Bruce
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