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Multivariate adaptive regression splines
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Multivariate adaptive regression splines : ウィキペディア英語版
Multivariate adaptive regression splines
In statistics, multivariate adaptive regression splines (MARS) is a form of regression analysis introduced by Jerome H. Friedman in 1991. It is a non-parametric regression technique
and can be seen as an extension of linear models that
automatically models nonlinearities and interactions between variables.
The term "MARS" is trademarked and licensed to Salford Systems. In order to avoid trademark infringements, many open source implementations of MARS are called "Earth".〔(CRAN Package earth )〕〔(Earth - Multivariate adaptive regression splines in Orange (Python machine learning library) )〕
== The basics ==

This section introduces MARS using a few examples. We start with a set of data: a matrix of input variables ''x'', and a vector of the observed responses ''y'', with a response for each row in ''x''. For example, the data could be:
Here there is only one independent variable, so the ''x'' matrix is just a single column. Given these measurements, we would like to build a model which predicts the expected ''y'' for a given ''x''.
A linear model for the above data is
:
\hat = -37 + 5.1 x

The hat on the \hat indicates that \hat is estimated from the data. The figure on the right shows a plot of this function:
a line giving the predicted \hat versus ''x'', with the original values of ''y'' shown as red dots.
The data at the extremes of ''x'' indicates that the relationship between ''y'' and ''x'' may be non-linear (look at the red dots relative to the regression line at low and high values of ''x''). We thus turn to MARS to automatically build a model taking into account non-linearities. MARS software constructs a model from the given ''x'' and ''y'' as follows
:
\begin
\hat = &\ 25 \\
& + 6.1 \max(0, x - 13) \\
& - 3.1 \max(0, 13 - x) \\
\end

The figure on the right shows a plot of this function: the predicted \hat versus ''x'', with the original values of y once again shown as red dots. The predicted response is now a better fit to the original ''y'' values.
MARS has automatically produced a kink
in the predicted ''y'' to take into account non-linearity.
The kink is produced by ''hinge functions''.
The hinge functions are the expressions starting with \max
(where \max(a,b)
is a if a > b, else b).
Hinge functions are described in more detail below.
In this simple example, we can easily see from the plot that
''y'' has a non-linear relationship with ''x''
(and might perhaps guess that y varies with the square of ''x'').
However, in general there will be multiple
independent variables,
and the relationship between ''y'' and these variables will be unclear
and not easily visible by plotting.
We can use MARS to discover that non-linear relationship.
An example MARS expression with multiple variables is
:
\begin
\mathrm = &\ 5.2 \\
& + 0.93 \max(0, \mathrm - 58) \\
& - 0.64 \max(0, \mathrm - 68) \\
& - 0.046 \max(0, 234 - \mathrm) \\
& - 0.016 \max(0, \mathrm - 7) \max(0, 200 - \mathrm)\\
\end

This expression models air pollution (the ozone level)
as a function of the temperature and a few other variables.
Note that the last term in the formula (on the last line)
incorporates an interaction between \mathrm
and \mathrm.
The figure on the right plots the predicted
\mathrm as \mathrm and
\mathrm vary,
with the other variables fixed at their median values.
The figure shows that wind does not affect the ozone
level unless visibility is low.
We see that MARS can build quite flexible regression surfaces
by combining hinge functions.
To obtain the above expression, the MARS model building procedure
automatically selects which variables to use (some variables are
important, others not), the positions of the kinks in the hinge
functions, and how the hinge functions are combined.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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