Some deprecated functions, originally used purely for light level estimation before the sampling algorithm was generalized for satellite models as well.
mkElevationSeg(segments, day)mkNLPosterior(segments, day, light, calib)
old.dist.gc(x1, x2 = NULL)
old.find.init(mask, nseg, nlpost, pars = c("Lon", "Lat", "k"))
old.metropolis(nlpost, lookup, p0, cov0, start, end, iter = 1000, step = 100)
old.mkLookup(x, binArray = TRUE)
k.prior(seg, ps)
If it is a LIST, use
vector identifying the segment of each time and light value
date-time values in POSIXct
vector of light data
calibration function for light levels
matrix of track locations
matrix of track locations (optional second part)
image object of masked areas
number of (twilight) segments
negative log posterior function
names of parameters
lookup function for masked areas
initial locations for sampler
covariance matrix for sampler
known start parameters
known end parameters
number of iterations
number of thinning iterations per iter
image-like object of matrix or array of binary masks
logical: are the masks compressed into bits?
segment
light attenuation value
Michael D. Sumner
These functions are included for legacy purposes, this was the original implementation.
Please use the more up to date function
metropolis, with the models such as
solar.model or satellite.model.