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Evolution of the Astronomical Eyepiece - Brayebrook Observatory

Evolution of the Astronomical Eyepiece - Brayebrook Observatory

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EVOLUTION <strong>of</strong> <strong>the</strong> ASTRONOMICAL EYEPIECE<br />

DERIVATIVES OF THE PLÖSSL AND<br />

SYMMETRICAL:<br />

The first wide-angle modification <strong>of</strong> <strong>the</strong><br />

Plössl was <strong>the</strong> aplanatic eyepiece <strong>of</strong> Dr.<br />

Otto Schröder, described in Gill’s articles<br />

on telescopes in <strong>the</strong> 9th. edition <strong>of</strong><br />

<strong>the</strong> Encycl opaedia Britta nica . The<br />

glass employed is re f e r red to as<br />

Dauget’s crown (Cb1) and flint (Fb1). It<br />

comprised a pair <strong>of</strong> achromats spaced<br />

at 83% <strong>the</strong>ir ef fective focal length. The<br />

crown elements being plano-convex,<br />

plane surfaces facing <strong>the</strong> eye, and <strong>the</strong><br />

flin ts being co ncave meniscus. Eye<br />

relief was 0.54Fe, and <strong>the</strong> apparent<br />

field 72˚. Thi s design w as initi ally<br />

employed by Schönfeld in his sou<strong>the</strong><br />

rn Durchm usterung, and su bsequently<br />

marketed by Browning.<br />

ERFLÉ I - A 1-2-2 design having a 60˚<br />

field but eye relief only 0.3Fe. The<br />

glasses used were SF2, PSK3, FK5 and<br />

SF10.<br />

ERFLÉ II - A 2-1-2 design using <strong>the</strong><br />

same glass types having a 70˚ field and<br />

0.6Fe eye clearance. Paten ted after<br />

Erflé’s death in 1923.<br />

ERFLÉ III - A 1-2-2 design using <strong>the</strong><br />

same glass types having a 55˚ field and<br />

eye clearance <strong>of</strong> 0.32Fe. Patented after<br />

Erflé’s death in 1923.<br />

KAPELLA - Patented after Erf l é ’ s<br />

death in 1923 for Zeiss by Kapella, one<br />

<strong>of</strong> his assistants. A 1-2-2 design having<br />

a 70˚ field and 0.685Fe eye clearance.<br />

The glasses used were BK1, SK15 and<br />

FN11.<br />

Zeiss’ m odifi cation <strong>of</strong> t he Plö ssl,<br />

and <strong>the</strong> subse qu en t i nc orporation<br />

<strong>of</strong> <strong>the</strong> field lens to w ide n t he f ield,<br />

led Hein ri ch Erf lé to desi gn th e f irst<br />

true w ide-an gle ey epi ece f or m ili tary<br />

use in 1917 .<br />

36<br />

KASPEREIT - A modification <strong>of</strong> Erflé’s<br />

designs by Kaspereit having a 2-2-2<br />

for m, giving fields in excess <strong>of</strong> 68˚ and<br />

eye r elief 0.3Fe+. The glasses used in<br />

modern variants are SF2, BK7, SK20<br />

and SF10. Some W.W.II (World War II)<br />

variants using Thorium or Uranium<br />

glass have fields wider than 70˚.<br />

All <strong>the</strong>se Erflé types and <strong>the</strong>ir derivatives<br />

suf fer from lateral colour, astigmatism<br />

and rectilinear distortion.

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