The principal component analysis method has been applied to two sample
s of nearby and distant quasars with well known radio data. Relationsh
ips between physical parameters pertinent to radio morphology has been
searched and the significant number of dimensions of the manifold has
been found to be two. The results of this analysis confirm the existe
nce of a redshift luminosity correlation for a subset of 36 nearby, bu
t to a lesser extent for 43 distant, quasars. An anticorrelation seems
to exist between luminosity and linear sizes for the last sample. On
the other hand, application of this analysis to the above samples indi
cates no correlation between the viewing angle and the other physical
parameters.