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Apochromatic
lens designs for astrotelescopes
In this section
are described
several designs for high performance lenses for telescopes being used
with eyepieces. The general specification is that the image
field
is 20mm diameter and axial and lateral aberration and the polychromatic
modulation transfer function at an image spatial frequency of
100cycles/mm should
exceed about 30% for focal ratios less than F/8. Because the
lenses will be used with an eyepiece, the eye focus setting can be used
to compensate for some field curvature, but astigmatism is also to be
within the tolerance.
1.
The
600mm F/8
objective lensThe maximum aperture of the lenses is restricted to about 100mm. Much above this, and the cost of the raw glass blanks begins to escalate without a significant increase in light-gathering or image sharpness. The following lenses are described: (1) A 600mm F/8 apochromat formed by a two element objective and a meniscus field flattener. (2) A 600mm F/6 apochromat formed by a three element objective and a meniscus field-flattener. (3) A 400mm F/4 apochromat formed by a three element objective and a meniscus field-flattener. A common thread to these designs is the use of the SUMITA PFK85 'fluorite' glass and the SCHOTT N-LAK10 glass. This glass pair is remarkably well matched for partial dispersion throughout the complete spectrum 0.45µm to 1.2µm. Note however that if the full spectral range is required, then it must be SCHOTT N-LAK10. There are between the identically named SUMITA and SCHOTT N-LAK10 glasses small but significant differences in the fourth decimal place of the index value. The following image shows the air-spaced Fraunhofer ( 'flint' leading) configuration. The relatively durable glass N-LAK10 is external and protecting the rather more fragile PFK85. ![]() The following image shows the meniscus field-flattening lens close to the focal position. ![]() The
following image shows that the lens is effectively diffraction limited
over the full field of 1.9degrees.
![]() This following
image shows the
remarkable 'apochromatic' correction of axial colour over the waveband
accessible to the eye and to silicon based photodetectors.
Although the deviation seems high at about 250µm it must be
remembered that the tolerance for defocus is in the region 600
wavelengths, i.e about 300µm.
![]() The following
table shows the
prescription. Notice that there is a common curvature on the
objective elements- this saves tooling costs.
![]() 2.
The
600mm F/6 objective lens
A
substantial increase in image brightness and
resolveable frequencies, or a shortening of exposure time can be
achieved by splitting the fluorite into two elements. The
excellent apochromatic correction is retained.
![]()
Notice
the useful increase in MTF at 200cycles/mm as a result of the increase
in numerical aperture.
This is the prescription. Notice that there are still only five curvature values, plus plano. ![]() 3.
The
400mm
F/4 objective lens
The
three element objective group design can be extended to a 400mm F/4
configuration, covering a field diameter of 2.9degrees.
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| ©
Don
Barron 2005 |
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