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Here, we take d as a variable parameter in our calculations.
M is a variable parameter.
Y is a random variable parameter.
The technique of the analysis includes: (a) calculation of asymptotic cones of ground-based detectors; (b) modeling of cosmic ray detector responses at variable parameters of the flux of solar relativistic protons; (c) determination of primary solar proton parameters outside magnetosphere by comparison of computed responses with observations.
Variable importance thus quantifies the contribution of each input variable (parameter) for a given output variable.
We define the pupil diameter as D and the Gaussian beam diameter at 1/e is h D. The variable parameter, the fill-factor, h, is the ratio of the 1/e diameter of the Gaussian beam to the diameter (D) of the full-pupil.
This comes as a surprise, as fitting with two variable parameters should give at least as good a fit as fitting with only one variable parameter.
I suppose it was written at a variable speed.
Yet often these analyses are based on studies of such varying quality, and with variable parameters – age of pupils and research design, for example – that it is difficult to arrive at sound conclusions.
Accordingly, studies were systematically carried out by varying the stated parameters, through the one-variable-at-a-time approach.
Physical parameters such as pH, agitation, and nutritional parameters, that is, carbon and nitrogen sources, were first standardized by one-variable-at-a-time method.
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CEO of Professional Science Editing for Scientists @ prosciediting.com