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[ See also Previous notes TCF-S Focuser Notes 1 - 2008-02-19 ]
Initial Impressions / benefits at 2008-03-19:
The new focuser equipment arrived in mid-February and initial impression
after 3 sessions was that the TCF-S is a worthwhile investment, providing :
firmer connection between CCD Camera and Scope.
repeatability in focuser position, with digital readout of focus position
remote focusing capability through network / observatory laptop
automated focus adjustment for changing ambient temperature (correcting focus drift)
realtime and recorded measurement of ambient temperature and temperature changes
The TCF-S is a far more heavy duty focuser, than my previous NGF-S focuser, which removes the previous collimation-limiting flexure between the scope and CCD camera. This should also mean that I will also get better/more reliable flat frames. With the step motor in the TCF-S I can now move to / return to a specific focus position with confidence. I don't have to wait at/revisit the observatory to make focusing adjustments. I can also maintain better focus as the temperature increases/decreases during unattended or automated operation of the observatory.
Earlier Teething problems
Teething problems with TCF-S focuser
shut-down issue.
After shutting down CCDSoft and hibernating the Observatory Laptop, I find that I'm unable to turn-off the focuser at the hand set. I have to restart the laptop and fiddle around with focuser PC connection to get to a position where I can switch off the focuser. (Simply turning off the Power to Focuser would of course mean that the current focus position/temperature are not stored on the EPROM ready for the next session)
FWHM Improvements
Although TCF-S has improved focus quality, sharpness of stars under my normal imaging conditions (5-180s exposure, unguided, near sea-level site) is still significantly impacted by factors other than focus qualiity, these factors are general poor seeing, seeing variations/cloud, wind/telescope shake, residual periodic error, star drift due to residual polar misalignment, star drift due to drive/post slew errors for certain poorly balanced sky positions.
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Focus profile was measured on a couple of occasions during Session 267 (2008-02-22). These are shown in the graph below.
Various Focuser Profiles recorded at
3 different temperatures |
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Based on focus measurements from several sessions (S267 to S275), including points measured in profiles above, a temperature coefficient of -158 steps per deg C has been estimated by my LX200 telescope normal setup (LX200 8", f/10 - operating at f7.4 , focal length 1498mm)
This Web Page: | Notes - Session 276 (2008-03-12) |
Last Updated : | 2015-05-16 |
Site Owner : | David Richards |
Home Page : | David's Astronomy Web Site |