Abramowitz and Stegun give an approximation for the standard normal's complementary cumulative distribution function (CCDF) in Formula 26.2.23
I understand this to be an approximation for when $\mu = 0$ and $\sigma = 1.$ Is there a procedure to transform the coefficients to generate an approximation fitting a CCDF for different values of $\mu$ and $\sigma?$

Comment (with room for notation and code).
In R statistical software the standard normal CDF $\Phi$ is denoted as
pnorm: that is, $P(Z \le 1.96) = 0.975,$ where $Z \sim \mathsf{Norm}(\mu=0, \sigma=1).$Also, the inverse CDF $\Phi^{-1}$ or 'quantile function' of $Z$ is denoted as
qnorm: that is $c = 1.96$ has $P(Z \le c) = 0.975.$The CDF of $X \sim \mathsf{Norm}(\mu, \sigma),$ for general mean $\mu$ and standard deviation $\sigma$ is denoted by
pnormwith the mean as the second argument and the SD as the third. And similarly for the quantile functionqnorm. Letting $\mu = 100$ and $\sigma = 10,$ we have:The relationship between the quantile function of standard normal and the quantile function of $\mathsf{Norm}(100, 10)$ is suggested by:
Maybe this answers some of your questions. I will leave it to you to put this into your favorite notation.
Notes: I believe you may want to use the quantile function to generate random samples from a normal distribution. In R, the straightforward way is to use the function
rnormwith appropriate parameters.The method behind
rnormis to use pseudorandom numbers that behave as a random sample from $\mathsf{Unif}(0,1)$ followed by a rational approximation of $\Phi^{-1}$ due to Michael Wichura. The approximation is accurate to within the ability of R to represent results in double precision. This can be demonstrated by generating a single standard normal observation, as shown below. (You can read more about this on the R documentation page forrnorm.)To simulate an observation from $\mathsf{Norm}(100, 10),$ we can use: