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Notes - Session 360 (2009-04-01)

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(S361)
 
2009-04-01
Bullet Reduced Star Drift
Bullet Tracking Rate Adjustment Trials
Bullet Seeing / Atmospheric Refraction Effect
Bullet Collimation and Image Curvatures Measurements
 
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Goto Images from 2009-04-01


Reduced Star Drift  / Residual PE Measurements

Small adjustments to scope's tracking rate and PEC (Periodic Error Correction) training are now showing some benefits.   The following images compare two sets of stacked frames :  one from the present session (S360) and one from the 'First Light Session' (S356).    Both cover 16 minute intervals 

Results of recent PEC Training and Tracking Rate Adjustment,  2009-04-01

Non-aligned Stacked frames from a 16 minute period (smeared star frames not used) / 
IC 531 starfield
No Guiding, PEC On, Tracking Rate Adjustment +1 (+0.1%)

Star drift (RA) : 0.9 arc secs/min westwards:
Star drift (Dec): 0.6 arc secs/min northwards
Periodic error :  5 arc secs (estimate)  + larger 10 arc sec error 

Image

Annotated CCD Image 
32 x 15s sec exposure (average combined / no alignment on stars)
 3x3 binning, C Filter, Cropped
2009-04-01 20:00 - 21:16h UT (#360001-46)
12" LX200R  (at f/5.7) + ST-10XME

  

Earlier Star drift and periodic error effects  - 2009-03-09

Stacked Images from a 16 minute period, 
C/2007 N3 (Lulin) starfield
No Alignment, No PEC, No Adjustment to Tracking Rate.

Star drift (RA) : 2 arc secs/min westwards:
Star drift (Dec) : 0.25 arc sec/min northwards
Periodic Error : 30 arc secs

Note: Comet C/2007 N3 (Lulin) records a higher drift rate due to its motion relative to background stars.

Image
Annotated CCD Image 
30 x 30s sec exposure (average combined / no alignment on stars or comet)
 3x3 binning, C Filter, Cropped
2009-03-09 21:08 - 21:24h UT (#356006-35)
12" LX200R  (at f/5.8) + ST-10XME

  

Star Drift (RA) Measurements / IC 531 starfield, 2009-04-01

Positional measurements on from a 16 minute period (smeared star frames not used)
No Guiding, PEC On, Tracking Rate Adjustment +1 (+0.1%)

Whilst the first and last frame (16 minutes later) show no RA drift, it is evident that the run comprises two sections
1) initial eastwards drift at 2.5 arc sec/minute   (5 minutes)
2)westwards drift at 0.9 arc secs/minute  (11 miutes)

(The reason of the initial eastwards drift lasting around 5 minutes is currently unexplained)

Assuming the drift rate of 0.9 arc secs/minute for the longer second section, the residual periodic error is around 5 arc secs

Image  

  

Star Drift (RA) Measurements / NGC 2877 starfield, 2009-04-01

Positional measurements on from a 16 minute period (NGC 2877)
No Guiding, PEC On, Tracking Rate Adjustment +2 (+0.2%)

The residual periodic error is around 5.5 arc secs. 

  

Image  

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Tracking Rate Adjustment Trials 

Two additional tracking rate trial were carried out during the present session (including the set described above).

The two new measurements are added to the table below.

Session  Tracking Rate
Adjustment
Star Drift (in RA)    Actual Tracking Rate
  Notes
S356/357  'Sidereal' Westwards by 1.9 arc secs/minute Slow by 0.21%   South Sky Point (w/o Pec)
S358a 'Sidereal'   Westwards by 3.2 arc secs/minute Slow by 0.34% South Sky Point (with Pec)
Westwards by 4.1 arc secs/minute Slow by 0.34% West Sky Point (with Pec)
S358b  +3  Eastwards by 2.5 arc secs/minute Fast by 0.28% South Sky Point (with Pec) 
S359  +1 Westwards by 2.2 arc secs/minute Slow by 0.24% South Sky Point (w/o Pec)
S360  +1 Westwards by 0.9 arc secs/minute ? Slow by 0.09% ? South Sky Point (with Pec)
+2 Eastwards by 1.0 arc secs/minute Fast by 0.11% South Sky Point (with Pec)

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Seeing / Atmospheric Refraction Effect

Several frames collected for star drift tests showed smeared/elongated stars, and were investigated further. 

The star llongation of stars is considered to be some form of seeing/ atmospheric refraction effect as the elongation is clearly perpendicular to the horizon, not to fork arm/RA lines
and other possibilities (tracking, PE, polar misalignement,) can be ruled out by occurrence of normal frames with circular stars.

Results of recent PEC Training and Tracking Rate Adjustment,  2009-04-01

Non-aligned stacked frames from a 16 minute period (all frames)
No Guiding, PEC On, Tracking Rate Adjustment +1 (+0.1%)
RA Drift 
Note : Elongation of stars is at least in part due to a seeing/atmospheric refraction effect 

Image

Annotated CCD Image 
46 x 15s sec exposure (average combined / no alignment on stars)
 3x3 binning, C Filter, Cropped
2009-04-01 20:00 - 21:16h UT (#360001-46)
12" LX200R  (at f/5.7) + ST-10XME

 

Frame with Smeared/Elongated Stars 

Image

Annotated CCD Image (65% size reduction, with 150% size insert)
15s sec exposure (single frame), 3x3 binning, C Filter
2009-04-01 (#360001), 12" LX200R  (at f/5.7) + ST-10XME

  

Normal Frame - circular stars

Image
Annotated CCD Image (65% size reduction, with 150% size insert)
15s sec exposure (single frame),  3x3 binning, C Filter
2009-04-01 (#360029), 12" LX200R  (at f/5.7) + ST-10XME
 

Frames showing orientation of smeared stars relative to horizon grid lines

Image Image
 
Image   Image
CCD Images (Image Linked within TheSky with Horizon Grid lines - brown))
15s sec exposure (single frames),  3x3 binning, C Filter
2009-04-01 (#360001,
360010, 360018, 236004)), 12" LX200R  (at f/5.7) + ST-10XME

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Collimation and Image Curvatures Measurements

An evaluation copy of CCD Inspector 2.1.6 (by CCDWare) was used to re-collimate the LX200 scope using a star field with around 220 stars, lying at around 29 deg altitude. Conditions were not ideal for performing a perfect collimation but an improvement of collimation was undoubtedly achieved and the fine tuning was far easier/more reliable that earlier visual/qualitative method.  It was noted that only very small movements of the collimation screws were necessary (2 - 3 degs of rotation)

Final estimated collimation error was around 3 - 4 arc secs, compared to a immediately prior collimation error of 14 arc secs 
(and compared against original first light collimation error of around 35-42 arc secs)

It is unclear why the collimation error immediately prior to re-collimation attempt (14 arc secs) is rather less than the measurements made during session S358 (31-37 arc secs)   (Mirror slop ?, seeing)

Collimation error, as measured by CCDI, is the offset between the optical center and physical center of the imaging train as measured at the image plane. The secondary mirror is adjusted until this error is minimized. Rules of thumb for collimation error are : An error of 10 arcseconds or less is acceptable, but can be improved upon, if seeing allows - An error of 5 arceconds or less is perfect, and doesn't require adjustment.

Collimation Measurements (pre Re-Collimation)

Image

CCD Inspector plot 
20s sec exposure,  2x2 binning, C Filter (#360245)
12" LX200R  (at f/5.7) + ST-10XME

  

Collimation Measurement  (post Re-Collimation)

Image

CCD Inspector plot 
20s sec exposure, 2x2 binning, C Filter (#360292)
12" LX200R  (at f/5.7) + ST-10XME

  

Image Prior to Re-Collimation

Image

CCD Image  (50% size reduction)
20s sec exposure (single frame),  3x3 binning, C Filter
2009-04-1 21:08 - 21:24h UT (#360245)
12" LX200R  (at f/5.7) + ST-10XME

  

Image After Re-Collimation
Optical centre moved total of 4.9 arc mins during re-collimation as measured by star positions before & after.

Image

CCD Image  (50% size reduction)
20s sec exposure (single frame),  3x3 binning, C Filter
2009-04-1 21:08 - 21:24h UT (#360292)
12" LX200R  (at f/5.7) + ST-10XME
 
Graphs showing progressive improvement in Collimation Quality during re-collimation 
a reasonable collimation position was obtained part way through the sequence 
but was lost again as further improvement was attempted.
Collimation attempt was stopped when approximately equivalent quality was obtained.
 
Image
 
Image

 

Table of Collimation / Curvature Measurements  - 12" LX200R  (at f/5.7) + ST-10XME

Session  Images Stars
Aspect
Ratio
Curvature
   Collimation 
(arc secs)
   Average FWHM
(arc secs)
   Tilt X    Tilt Y    Total Tilt
S356 (First Light Session)  30 x 30s 148 +/- 13 38 % +/- 20% 16 % +/- 1% 41.6" +/- 6.3" 5.4" +/- 0.7"   -0.9" +/- 0.1"   -0.3" +/- 0.1"   16% @ -157 deg
S356 (First Light Session)  6 x 60s 410 +/- 22 38 % +/- 10% 27 % +/- 1% 35.0" +/- 6.5" 5.3" +/- 0.3"   -1.1" +/- 0.2"   +0.5" +/- 0.1"   20% @ -149 deg
S357 collimation attempt
S358  7 x 90s 575 +/- 40 19% +/- 8% 24 % +/- 2% 36.3" +/- 6.3" 5.5" +/- 0.4"   +0.9" +/- 0.2"   +0.1" +/- 0.1"   15% @ - 5 deg
S358  6 x 45s 633 +/- 73 14% +/- 3% 21 % +/- 2% 31.7" +/- 7.6" 4.9" +/- 0.4"   +0.7" +/- 0.2"   +0.3" +/- 0.1"   10% @ - 22 deg
S358  3 x 60s 695 +/- 80 16% +/- 6% 24 % +/- 1% 36.1 +/- 4.0" 5.9" +/- 0.6"   +0.9" +/- 0.1"   +0.1" +/- 0.0"   14% @ - 9 deg
S360  2 x 20s 199 +/- 1 16% +/- 4% 22 % +/- 3% 13.9 +/- 1.3" 4.0" +/- 0.2"   +0.6" +/- 0.1"   +0.0" +/- 1.0"   12% @ - 9 deg
S360  3 x 20s 184 +/- 27 27% +/- 5% 24 % +/- 6% 14.7 +/- 1.5" 4.2" +/- 0.3"   +0.5" +/- 0.1"   -0.1" +/- 0.1"   12% @ 19 deg
S360 - Collimation attempt
S360 - Post Collimation 4 x 20s 223 +/- 13 17% +/- 1% 17 % +/- 3% 3.7 +/- 1.0" 4.0" +/- 0.1"   +0.2" +/- 0.1"   -0.1" +/- 0.1"   4% @ 20 deg

 

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