View source: R/cop_smacofSym.R
| cop_smacofSym | R Documentation | 
The free parameter is lambda for power transformations the observed proximities. The fitted distances power is internally fixed to 1 and the power for the weights is 1.
cop_smacofSym(
  dis,
  theta = 1,
  type = "ratio",
  ndim = 2,
  weightmat = 1 - diag(nrow(dis)),
  init = NULL,
  itmaxi = 1000,
  ...,
  stressweight = 1,
  cordweight = 0.5,
  q = 1,
  minpts = ndim + 1,
  epsilon = 10,
  rang = NULL,
  verbose = 0,
  normed = TRUE,
  scale = "sd",
  stresstype = "default"
)
| dis | numeric matrix or dist object of a matrix of proximities | 
| theta | the theta vector; should be a scalar for the lambda (proximity) transformation. Defaults to 1. | 
| type | MDS type. | 
| ndim | number of dimensions of the target space | 
| weightmat | (optional) a matrix of nonnegative weights | 
| init | (optional) initial configuration | 
| itmaxi | number of iterations. default is 1000 | 
| ... | additional arguments to be passed to the fitting procedure | 
| stressweight | weight to be used for the fit measure; defaults to 1 | 
| cordweight | weight to be used for the cordillera; defaults to 0.5 | 
| q | the norm of the cordillera; defaults to 1 | 
| minpts | the minimum points to make up a cluster in OPTICS; defaults to ndim+1 | 
| epsilon | the epsilon parameter of OPTICS, the neighbourhood that is checked; defaults to 10 | 
| rang | range of the distances (min distance minus max distance). If NULL (default) the cordillera will be normed to each configuration's maximum distance, so an absolute value of goodness-of-clusteredness. | 
| verbose | numeric value hat prints information on the fitting process; >2 is extremely verbose | 
| normed | should the cordillera be normed; defaults to TRUE | 
| scale | should the configuration be scale adjusted | 
| stresstype | which stress to report. Only takes smacofs default stress currrently. | 
A list with the components
stress: the stress
stress.m: default normalized stress
copstress: the weighted loss value
OC: the Optics cordillera value
parameters: the parameters used for fitting (lambda)
fit: the returned object of the fitting procedure
cordillera: the cordillera object
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