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Multidimensional Fechnerian Scaling: Probability-Distance Hypothesis

Journal of Mathematical Psychology, 2002
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The Cosmic Distance Scale

1988
A first requirement for the establishment of a cosmic distance scale is the correct measurement of distances within the solar system. The basic step in this procedure is the measurement of the distance to Venus. The most precise way of obtaining this distance is through the use of radar techniques. Another method is described in problems 2–2 and 2–3 at
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Multidimensional Scaling and Distance Geometry

2013
Imagine you have a map of a particular geographical region, which includes a number of cities and towns. Usually, such a map will be accompanied by a two-way table displaying how close a selected number of those towns and cities are to each other. Each cell of that table will show the degree of “closeness” (or proximity) of the row city to the column ...
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Basic Distance-Scale Problems

Publications of the Astronomical Society of the Pacific, 1961
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