kelvin (version 1.2-1)

Keir: Solutions to the Kelvin differential equations: 'Kei' and 'Ker'

Description

This function calculates the complex solution to the Kelvin differential equations using modified Bessel function of the second kind, specifically that which is produced by Bessel::BesselK.

Usage

Keir(xseq, nu. = 0, nSeq. = 1, add.tol = TRUE,
    return.list = FALSE, show.scaling = FALSE, ...)
  ## S3 method for class 'default':
Keir(xseq, nu. = 0, nSeq. = 1,
    add.tol = TRUE, return.list = FALSE,
    show.scaling = FALSE, ...)

Arguments

xseq

vector; values to evaluate the complex solution at

nu.

scalar; value of $\nu$ in $\mathcal{K}_\nu$

nSeq.

positive integer; if $nSeq > 1$, computes the result for a sequence of values; if $\nu >= 0: \nu, \nu+1, \cdots, \nu+nSeq-1$, if $\nu < 0: \nu, \nu-1, \cdots, \nu-nSeq+1$.

add.tol

boolean; fudge factor to prevent an error for zero-values

return.list

boolean; Should the result be a list instead of matrix?

show.scaling

boolean; Should the normalization values be given as a message?

...

additional parameters (currently unused)

Value

• If return.list==FALSE (default), a complex matrix with as many columns as using nSeq. creates. Otherwise the result is a list with matrices for Real and Imaginary components.

  NULL

References

http://mathworld.wolfram.com/KelvinFunctions.html

See Also

Ker, Kei, Beir

Examples

Keir(1:10)    # defaults to nu.=0, nSeq=1
Keir(1:10,nSeq=2)
Keir(1:10,nSeq=2,return.list=FALSE)