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SOT optical performance Focus stability in orbit

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(reimaging lens air-vac. diff) Initial offset. FPP (CLU air-vac. diff) Temperature change. Initial offset (-2.3 ) CFRP dehydration. OTA ... – PowerPoint PPT presentation

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Title: SOT optical performance Focus stability in orbit


1
SOT optical performanceFocus stability in orbit
  • Y. Katsukawa (NAOJ) and SOT team

2
SOT focus design
  • OTA is designed to provide collimated beam into
    FPP in air, and provides a weakly converging beam
    (f?200m) in vacuum. Air-to-vacuum difference of
    the focus position of OTA and FPP are adjusted by
    initial setting of the re-imaging lens
    position.
  • The 4 optical paths (BFI, NFI, SP, and CT) are
    designed to be kept in co-focal without any focus
    adjustment.

3
Focus adjustment by the re-imaging lens
  • Focus shift originating in OTA and FPP can be
    compensated by movement of the re-imaging lens
    along the optical axis during the mission
    operation. We plan to adjust the focus position
    occasionally to compensate seasonal variation.
  • No need to adjust the position within one orbital
    cycle because orbital variation is supposed to be
    negligible.
  • Mechanisms for the motion of the re-imaging lens
    have the specifications shown below.

Reimaging lens
M2
M1
4
Focus shift in orbit
  • Focus shift is caused by displacement of optical
    elements along the optical axis. The change of
    M1-M2 distance is most sensitive to the focus
    shift.
  • Mechanical environmental (vibration and acoustic)
    tests showed no significant change in focus
    position.
  • The thermal environment in orbit is very
    different from that on the ground. In order to
    predict the focus shift in orbit, we performed
    thermal-optical test of the telescope, and
    determined the defocus sensitivity for major
    components experimentally.
  • Focus errors (including margins) are controlled
    by a focus error budget table. The focus position
    is confirmed to be well within adjustable range
    by the re-imaging lens for the mission period.

5
Focus position in the first light phase
  • After the telescope top-door is opened, the
    temperatures inside the telescope increase, and
    are settled within several hours.
  • The telescope main structure is made of CFRP
    (carbon fiber reinforced plastic). The
    dehydration of CFRP makes M1-M2 distance smaller
    in vacuum. The speed of the shrinkage is
    temperature dependent.

6
Focus shift by CFRP dehydration
1 month (?) later
Just after launch
M2
M2
M1
M1
-8.3mm ? -4.2mm
?0mm
7
Temperature dependence of CFRP dehydration
2nd test on May 2004 OTA temperature was kept
?20C during the test.
A20 (lambda, DP)
Time constant ? 400hrs
Time (hour)
4th test on Mar 2005 Focus position did not
change during the cold mode.
Cold mode
Hot mode
Time (hour)
8
Orbital variation by temperature ripple
  • The temperature prediction in orbit tells that
    there is 1-2?C temperature ripple within one
    orbital cycle especially around M2.
  • The focus shift within one orbital cycle is
    expected to be around 0.2mm at the re-imaging
    lens focus. This corresponds to one or two steps
    of the focus adjustment, and is within focal
    depth.

Temperature and focus ripple within one orbital
cycle
(Only major components are shown in the table.)
9
Focus change between DC and Limb obs.
  • In limb observations, heat inputs to the
    telescope become smaller than those in DC obs.
    This makes the temperatures 1 - 2 ?C lower.
  • This temperature change causes small focus shift,
    but the shift is expected to be about 0.1mm, and
    is negligible.

Temperature and focus change between DC and Limb
obs.
(Only major components are shown in the table.)
10
Long-term focus shift
  • Because of the contamination on the mirror
    surface, the temperature inside the telescope
    tends to increase gradually through the mission
    life.
  • The temperature increase causes gradual focus
    shift, and will be compensated by the re-imaging
    lens.

Temperature and focus change through the mission
life
(Only major components are shown in the table.)
11
Summary
  • The orbital and DC-Limb variation are expected to
    be 1-2 steps of the focus adjustment, and well
    within focal depth.
  • We should verify orbital and DC-Limb variation in
    the first light phase.
  • The seasonal and long-term focus shift will be
    compensated by occasional adjustment of the
    re-imaging lens position.
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