我想将一个完整的非线性模型与一个空模型进行比较。考虑到例如通常使用glm的方法,这是可能的吗?就我而言:
#Packages
library(minpack.lm)
# Data set - Diameter in function of Feature and Age
Feature<-sort(rep(c("A","B"),22))
Age<-c(60,72,88,96,27,
36,48,60,72,88,96,27,36,48,60,72,
88,96,27,36,48,60,27,27,36,48,60,
72,88,96,27,36,48,60,72,88,96,27,
36,48,60,72,88,96)
Diameter<-c(13.9,16.2,
19.1,19.3,4.7,6.7,9.6,11.2,13.1,15.3,
15.4,5.4,7,9.9,11.7,13.4,16.1,16.2,
5.9,8.3,12.3,14.5,2.3,5.2,6.2,8.6,9.3,
11.3,15.1,15.5,5,7,7.9,8.4,10.5,14,14,
4.1,4.9,6,6.7,7.7,8,8.2)
d<-dados <- data.frame(Feature,Age,Diameter)
str(d)
# Complet model
e1<- Diameter ~ a1 * Age^a2
#Algoritm Levenberg-Marquardt
m1 <- nlsLM(e1, data = d,
start = list(a1 = 0.1, a2 = 10),
control = nls.control(maxiter = 1000))
#Null model
e2<- Diameter ~ 1
#Algoritm Levenberg-Marquardt
m0 <- nlsLM(e1, data = d,
control = nls.control(maxiter = 1000))
Warning message:
In nlsLM(e1, data = d, control = nls.control(maxiter = 1000)) :
No starting values specified for some parameters.
Initializing ‘a1’, ‘a2’ to '1.'.
Consider specifying 'start' or using a selfStart model
不起作用,我的最终目标是:
anova(m1,m0)
在非线性宇宙中这可能吗?谢谢你。
答案 0 :(得分:1)
是的,R中定义了anova.nls
methods("anova")
## [1] anova.glm* anova.glmlist* anova.lm* anova.lmlist*
## [5] anova.loess* anova.mlm* anova.nls* anova.quantmod*
## see '?methods' for accessing help and source code
但是,问题中的代码存在一些问题:
尝试一下:
o <- order(d$Age)
# Complet model
e1<- Diameter ~ Age^a2
m1a <- nls(e1, data = d[o, ], start = list(a2 = 10), alg = "plinear")
#Null model
ones <- rep(1, nrow(d))
e2 <- Diameter ~ a * ones
m0a <- nls(e2, data = d[o, ], start = list(a = 1))
anova(m1a, m0a)
## Analysis of Variance Table
##
## Model 1: Diameter ~ Age^a2
## Model 2: Diameter ~ a * ones
## Res.Df Res.Sum Sq Df Sum Sq F value Pr(>F)
## 1 42 270.96
## 2 43 823.73 -1 -552.77 85.68 1.07e-11 ***
## ---
## Signif. codes: 0 ‘***’ 0.001 ‘**’ 0.01 ‘*’ 0.05 ‘.’ 0.1 ‘ ’ 1
plot(Diameter ~ Age, d)
lines(fitted(m0a) ~ Age, d[o, ], col = "blue")
lines(fitted(m1a) ~ Age, d[o, ], col = "red")