www.delorie.com/gnu/docs/calc/calc_271.html | search |
Buy the book! | |
[ < ] | [ > ] | [ << ] | [ Up ] | [ >> ] | [Top] | [Contents] | [Index] | [ ? ] |
The a F command also accepts other kinds of models besides lines and polynomials. Some common models have quick single-key abbreviations; others must be entered by hand as algebraic formulas.
Here is a complete list of the standard models recognized by a F:
All of these models are used in the usual way; just press the appropriate letter at the model prompt, and choose variable names if you wish. The result will be a formula as shown in the above table, with the best-fit values of the parameters substituted. (You may find it easier to read the parameter values from the vector that is placed in the trail.)
All models except Gaussian and polynomials can generalize as shown to any number of independent variables. Also, all the built-in models have an additive or multiplicative parameter shown as a in the above table which can be replaced by zero or one, as appropriate, by typing h before the model key.
Note that many of these models are essentially equivalent, but express the parameters slightly differently. For example, a b^x and the other two exponential models are all algebraic rearrangements of each other. Also, the "quadratic" model is just a degree-2 polynomial with the parameters expressed differently. Use whichever form best matches the problem.
The HP-28/48 calculators support four different models for curve
fitting, called LIN
, LOG
, EXP
, and PWR
.
These correspond to Calc models `a + b x', `a + b ln(x)',
`a exp(b x)', and `a x^b', respectively. In each case,
a is what the HP-48 identifies as the "intercept," and
b is what it calls the "slope."
If the model you want doesn't appear on this list, press ' (the apostrophe key) at the model prompt to enter any algebraic formula, such as m x - b, as the model. (Not all models will work, though--see the next section for details.)
The model can also be an equation like y = m x + b. In this case, Calc thinks of all the rows of the data matrix on equal terms; this model effectively has two parameters (m and b) and two independent variables (x and y), with no "dependent" variables. Model equations do not need to take this y = form. For example, the implicit line equation a x + b y = 1 works fine as a model.
When you enter a model, Calc makes an alphabetical list of all the variables that appear in the model. These are used for the default parameters, independent variables, and dependent variable (in that order). If you enter a plain formula (not an equation), Calc assumes the dependent variable does not appear in the formula and thus does not need a name.
For example, if the model formula has the variables a,mu,sigma,t,x, and the data matrix has three rows (meaning two independent variables), Calc will use a,mu,sigma as the default parameters, and the data rows will be named t and x, respectively. If you enter an equation instead of a plain formula, Calc will use a,mu as the parameters, and sigma,t,x as the three independent variables.
You can, of course, override these choices by entering something different at the prompt. If you leave some variables out of the list, those variables must have stored values and those stored values will be used as constants in the model. (Stored values for the parameters and independent variables are ignored by the a F command.) If you list only independent variables, all the remaining variables in the model formula will become parameters.
If there are $ signs in the model you type, they will stand for parameters and all other variables (in alphabetical order) will be independent. Use $ for one parameter, $$ for another, and so on. Thus $ x + $$ is another way to describe a linear model.
If you type a $ instead of ' at the model prompt itself, Calc will take the model formula from the stack. (The data must then appear at the second stack level.) The same conventions are used to choose which variables in the formula are independent by default and which are parameters.
Models taken from the stack can also be expressed as vectors of two or three elements, [model, vars] or [model, vars, params]. Each of vars and params may be either a variable or a vector of variables. (If params is omitted, all variables in model except those listed as vars are parameters.)
When you enter a model manually with ', Calc puts a 3-vector describing the model in the trail so you can get it back if you wish.
Finally, you can store a model in one of the Calc variables
Model1
or Model2
, then use this model by typing
a F u or a F U (respectively). The value stored in
the variable can be any of the formats that a F $ would
accept for a model on the stack.
Calc uses the principal values of inverse functions like ln
and arcsin
when doing fits. For example, when you enter
the model `y = sin(a t + b)' Calc actually uses the easier
form `arcsin(y) = a t + b'. The arcsin
function always
returns results in the range from -90 to 90 degrees (or the
equivalent range in radians). Suppose you had data that you
believed to represent roughly three oscillations of a sine wave,
so that the argument of the sine might go from zero to
3*360 degrees.
The above model would appear to be a good way to determine the
true frequency and phase of the sine wave, but in practice it
would fail utterly. The righthand side of the actual model
`arcsin(y) = a t + b' will grow smoothly with t, but
the lefthand side will bounce back and forth between -90 and 90.
No values of a and b can make the two sides match,
even approximately.
There is no good solution to this problem at present. You could restrict your data to small enough ranges so that the above problem doesn't occur (i.e., not straddling any peaks in the sine wave). Or, in this case, you could use a totally different method such as Fourier analysis, which is beyond the scope of the a F command. (Unfortunately, Calc does not currently have any facilities for taking Fourier and related transforms.)
[ < ] | [ > ] | [ << ] | [ Up ] | [ >> ] | [Top] | [Contents] | [Index] | [ ? ] |
webmaster | delorie software privacy |
Copyright © 2003 by The Free Software Foundation | Updated Jun 2003 |