Up: Stellar coronagraphy with prolate
The circular prolate functions used in this paper can be defined in terms of Slepian's "generalized prolate
spheroidal functions''
(Slepian 1964):
 |
(C.1) |
Here N is the order of the Hankel transform, n the order of the prolate function, and
the
prolateness parameter. In this paper we are primarily interested in the case N=n=0, and for convenience
have generally omitted these labels.
The functions
are solutions of a generalized spheroidal differential equation,
 |
(C.2) |
with eigenvalues
.
They are conventionally normalized so that
 |
(C.3) |
When c=0, Eq. (C.2) is satisfied by the functions
TN,n(x), defined by
 |
(C.4) |
where
2F1(a,b;c;z) is Gauss' hypergeometric function (Abramowitz & Stegun 1965), and the eigenvalue is
.
The
TN,n(x) satisfy the three-term recurrence relation
 |
(C.5) |
where
For general c, the functions
are expanded in a series of the
TN,k(x):
 |
(C.7) |
Substituting this expansion into Eq. (C.2) and using Eq. (C.5), we obtain a three-term
recurrence for the series coefficients
dkN,n(c):
 |
|
|
(C.8) |
The eigenvalues
and the coefficients
dkN,n(c) can be computed from this equation
using the standard tridiagonal matrix or continued fraction methods (Falloon 2001). For x > 1,
can be computed using the series
 |
(C.9) |
where
 |
(C.10) |
The eigenvalues of the integral equation (Eq. (B.3)),
,
can be found using
 |
(C.11) |
Up: Stellar coronagraphy with prolate
Copyright ESO 2003