Refractive
Index Approximation
In his book Optical
Aberration Coefficients, H.A. Buchdahl suggests a version of dispersion
equation based upon &omega:
&omega = &delta&lambda / ( 1 + 2.5 &delta&lambda )
where &delta&lambda is &lambda &lambdaD. This
definition of &omega has a zero at the D-line and a singularity at about
187 nm. An alternative dispersion
equation base is:
H = &deltaf2 / ( 1 - 0.04 &deltaf2 )
where &deltaf2 = f2 fe2 and f = 1 / &lambda. This base has the singularity at
about the same wavelength as the Buchdahl base, but, of course, has its zero at
the e-line. Relative to f2,
the value of H is invertible, in that:
f2 = fe2 + H / ( 1 + 0.04 H )
the first few derivatives
of which are:
df2/&deltaH = 1 / ( 1 + 0.04 H )2
d2f2/&deltaH2 = -2 * 0.04 / ( 1
+ 0.04 H )3
d3f2/&deltaH3 = 6 * 0.042
/ ( 1 + 0.04 H )4
If S is a function of f2,
then the derivatives of
S
= &deltaf2/&deltaH * &deltaS/&deltaf2
S
= (&deltaf2/&deltaH)2 * &delta2S/&delta(f2)2 +
&delta2f2/&deltaH2 * dS/&deltaf2
S =
(&deltaf2/&deltaH)3 * &delta3S/&delta(f2)3 +
3 &deltaf2/&deltaH * &delta2f2/&deltaH2 * &delta2S/&delta(f2)2 +
&delta3f2/&deltaH3 * &deltaS/&deltaf2
the attempt here being
S* = Se + Se H + Se
H2 / 2 + Se H3 / 6
within a small region
about the e-line. According to Buchdahl,
using his original base allowed good approximations with very few terms. This note will ignore beyond the third
derivative.
We are interested in two
related forms of S; the six-term Schott dispersion equation
(also known as the Cauchy dispersion equation):
n2 = A2 (f2)-1
+ A0 + A-2 f2 + A-4 (f2)2
+ A-6 (f2)3 + A-8 (f2)4
The coefficients, A2
A-8,
are specific to the glass type.
and the three-term
Sellmeier dispersion equation:
n2 1 = E1 + E2 + E3
where Ei = Bi
/ ( 1 Ci f2 ).
The coefficients, Bi and Ci, are
The derivatives of the
Cauchy equation are found from:
2*n*&deltan/&deltaf2 = -A2 (f2)-2 +
A-2 + 2A-4 f2 + 3A-6 (f2)2
+ 4A-8 (f2)3
2*n*&delta2n/&delta(f2)2 = 2*(A2
(f2)-3 + A-4 + 3A-6 f2 +
6A-8 (f2)2 - (&deltan/&deltaf2)2)
2*n*&delta3n/&delta(f2)3 = 6*(-A2
(f2)-4 + A-6 + 4A-8 f2
&deltan/&deltaf2*&delta2n/&delta(f2)2)
The derivatives of the
Sellmeier equation can be from from:
2*n*&deltan/&deltaf2 = E1 D1 + E2 D2 + E3 D3
2*n*&delta2n/&delta(f2)2 =
2*(E1 D12 + E2 D22
+ E3 D32 - (&deltan/&deltaf2)2)
2*n*&delta3n/&delta(f2)3 =
6*(E1 D13 + E2 D23
+ E3 D33 - &deltan/&deltaf2*&delta2n/&delta(f2)2)
where Di = Ci
/ ( 1 Ci f2 ).
Typically, glass catalogs
can list the refractive index n, the
PF,e = 0.4884 0.000526 v + &DeltaPF,e
Pg,F = 0.6438 0.001682 v + &DeltaPg,F
If none of these is
available, it may be assumed the glass is a normal glass, with &DeltaPF,e
= &DeltaPg,F = 0.
If only one of the partial dispersions is missing, the other may be
derived from the empirical formula:
&DeltaPg,F = 4.0 * &DeltaPF,e
These values may be related
to the derivatives by:
n = Se
&Deltan*( PF,e
1 ) = HC Se + HC2
Se/2 + HC3 Se/6
&Deltan*PF,e = HF Se + HF2
Se/2 + HF3 Se/6
&Deltan*( PF,e +
Pg,F ) = Hg Se + Hg2
Se/2 + Hg3 Se/6
This matrix form is
invertible. Its inverse may be used to derive values of Se, Se,
Se, and Se from the glass catalog values.
The values of HC,
HF and Hg used in the matrix above need not change when a
minimum focus wavelength other than the e-line is used. They will simply represent analogous
translations from that new wavelength, and not necessarily back to the C, F and
g lines themselves.