HRC-I On-Orbit Shutter Focus Simulations
This page summarizes the simulations of the HRC-I on-orbit
shutter focus algorithm. The simulations represent measurements
HI-2.[6,7]
and HI-4.2. Using spectra for LMC
X-1 and HR1099
and exposure times from the OAC
timeline, the simulations explore the effects on the
determination of focus and inter-optic tilts of
- the placement of the SIM along the optical axis;
- uncertainty in the position of the shutters relative to the image;
- uncertainty in the angular positions of the shutters,
- uncertainty in the source's position relative to the optical axis
The shutter focus algorithm is derived from the alignment
formulae described in L. Van Speybroeck's 01/03/1990 memo
X-ray Alignment Formulae and
implemented in the script qsf.
The alignment algorithm uses the HRC shutters as quadrant
shutters. Centroids are calculated for each quadrant and
combined as described in X-ray Alignment
Formulae to determine the defocus and tilts
between the optics.
Rays were generated using trace-nest1 with the orbit_XRCF+tilts_01
configuration database. Initially, 100 independent simulations
were run for both sources, with the detector centered on the
image in the focal plane, the shutters in their ideal positions,
and ideal source position (on-axis) for the following defocus
values: ± 1, ± 0.5, ± 0.25, ± 0.1,
± 0.05, and 0 mm.
Three additional studies were run with LMC X-1 as the source,
with the following scenarios:
-
The image was not placed at the nominal position relative to
the shutters.
The shutters were positioned nominally and the image was
positioned at the interstices of a 5 x 5 grid with 10
micrometer spacing, centered at the nominal image position.
-
The shutter blades had incorrect angular positions.
The shutters were positioned at ± 0.25, ± 0.125,
± 0.0625, and 0 degrees relative to their nominal
positions. These correspond to ± 4, ± 2, ±
1, and 0 encoder steps, respectively. The focus calculations
were done assuming the nominal angular positions.
-
The source was not placed on axis.
The source was placed in each of 24 different positions
relative to the optical axis. Source positions were defined
in polar coordinates, with theta equal to 0, 5, and 10
arcseconds and phi equal to 45, 90, 135, 180, 225, 270, 315
degrees.
Again, 100 independent simulations were run for each different configuration.
For each scenario the following plots are presented:
-
Focus error vs. Defocus
These show the error in the focal position derived by the
quadrant shutter algorithm as a function of the SIM X offset
from nominal focus. Positive numbers indicate that the
determined focus was too close to the HRMA. A focus error of
0 indicates a spot-on prediction. Results from all 100
simulations are shown.
-
95 Percentile Focus error vs. Defocus
These present the 95% confidence levels as a function of the
SIM X offset from nominal focus; 95% of the simulations
derived a focal error less than or equal to that plotted.
Smaller is better.
-
Y Tilts vs. Defocus, Y Tilts vs. Defocus
Plots of Y and Z inter-optic tilts. What's important here is
the stability of the determination, rather than its actual value.
Results for the various scenarios are available here. Summary plots of the minimum and
maximum values of the 95% confidence level in the focus error as a
function of SIM X offset from nominal focus are shown below:
While the magnitude of the various offsets we have chosen are
fairly significant, their effects on the focus error are small.
The 95th percentile focus errors vary by no more than 0.009 mm
for any given position along the optical axis.
One interesting trend to note is that the magnitude of the focus
error is not symmetric about the focal point. Instead, it
reaches its minimum 0.25 mm towards the HRMA. This implies that
to attain best focus, we would like to place the detector one
the +X side of the focal point, towards the HRMA.
Below are links to navigation maps and tables for the detailed
plots for each configuration. One can use either the maps or
the tables. To use the maps, simply click on the colored points
in the map; each point represents an offset from the ideal
detector, shutter, and source placement. To use the tables,
click on the checkmarks. Clicking on the images of the plots
will bring up PostScript figures for your amusement.
|
| Theta | Phi | Y | Z | +Y | -Y | GIF |
| 0 | 0 | -0.02 | 0.02 | 0.0000 | 0.0000 |  |
| 0 | 0 | -0.02 | 0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | -0.02 | -0.00 | 0.0000 | 0.0000 |  |
| 0 | 0 | -0.02 | -0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | -0.02 | -0.02 | 0.0000 | 0.0000 |  |
| 0 | 0 | -0.01 | 0.02 | 0.0000 | 0.0000 |  |
| 0 | 0 | -0.01 | 0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | -0.01 | -0.00 | 0.0000 | 0.0000 |  |
| 0 | 0 | -0.01 | -0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | -0.01 | -0.02 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.00 | 0.02 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.00 | 0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.00 | -0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.00 | -0.02 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.01 | 0.02 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.01 | 0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.01 | -0.00 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.01 | -0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.01 | -0.02 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.02 | 0.02 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.02 | 0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.02 | -0.00 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.02 | -0.01 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.02 | -0.02 | 0.0000 | 0.0000 |  |
|
|
| Theta | Phi | Y | Z | +Y | -Y | GIF |
| 0 | 0 | 0.00 | -0.00 | -0.2500 | 0.0000 |  |
| 0 | 0 | 0.00 | -0.00 | -0.1250 | 0.0000 |  |
| 0 | 0 | 0.00 | -0.00 | -0.0625 | 0.0000 |  |
| 0 | 0 | 0.00 | -0.00 | 0.0000 | -0.2500 |  |
| 0 | 0 | 0.00 | -0.00 | 0.0000 | -0.1250 |  |
| 0 | 0 | 0.00 | -0.00 | 0.0000 | -0.0625 |  |
| 0 | 0 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 0 | 0 | 0.00 | -0.00 | 0.0000 | 0.0625 |  |
| 0 | 0 | 0.00 | -0.00 | 0.0000 | 0.1250 |  |
| 0 | 0 | 0.00 | -0.00 | 0.0000 | 0.2500 |  |
| 0 | 0 | 0.00 | -0.00 | 0.0625 | 0.0000 |  |
| 0 | 0 | 0.00 | -0.00 | 0.1250 | 0.0000 |  |
| 0 | 0 | 0.00 | -0.00 | 0.2500 | 0.0000 |  |
|
|
| Theta | Phi | Y | Z | +Y | -Y | GIF |
| 0 | 0 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 5 | 0 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 5 | 45 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 5 | 90 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 5 | 135 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 5 | 180 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 5 | 225 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 5 | 270 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 5 | 315 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 10 | 0 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 10 | 45 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 10 | 90 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 10 | 135 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 10 | 180 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 10 | 225 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 10 | 270 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 10 | 315 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 15 | 0 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 15 | 45 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 15 | 90 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 15 | 135 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 15 | 180 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 15 | 225 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 15 | 270 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
| 15 | 315 | 0.00 | -0.00 | 0.0000 | 0.0000 |  |
|
A link to the original
simulations is provided here. It is here simply for
completeness. The new simulations referenced on this page supercede
the results presented with the older simulations. The simulations
on this page are more realistic and explore a wider range of effects
on the focus determination. If you do compare between the old and
new simulations please note that we have changed coordinate systems
between the two. This older simulations were done using the OSAC
coordinate system and the newer simulations on this page were done
using the HRMA coordinate system. This is evident is the plots of
focus error vs. distance from focus where the slope of the plot is
reversed due to the change in sign of the optical axis in the two
systems.
M. Tibbetts