2.3. The Gaussian Distribution 109
I 0 (m)
m
0 5 10
0
1000
2000
3000
A(m)
m
0 5 10
0
0.5
1
Figure 2.20 Plot of the Bessel functionI 0 (m)defined by (2.180), together with the functionA(m)defined by
(2.186).
Setting the derivative with respect toθ 0 equal to zero gives
∑N
n=1
sin(θn−θ 0 )=0. (2.182)
To solve forθ 0 , we make use of the trigonometric identity
sin(A−B)=cosBsinA−cosAsinB (2.183)
Exercise 2.53 from which we obtain
θML 0 = tan−^1
{∑
∑nsinθn
ncosθn
}
(2.184)
which we recognize as the result (2.169) obtained earlier for the mean of the obser-
vations viewed in a two-dimensional Cartesian space.
Similarly, maximizing (2.181) with respect tom, and making use ofI′ 0 (m)=
I 1 (m)(Abramowitz and Stegun, 1965), we have
A(m)=
1
N
∑N
n=1
cos(θn−θML 0 ) (2.185)
where we have substituted for the maximum likelihood solution forθ 0 ML(recalling
that we are performing a joint optimization overθandm), and we have defined
A(m)=
I 1 (m)
I 0 (m)
. (2.186)
The functionA(m)is plotted in Figure 2.20. Making use of the trigonometric iden-
tity (2.178), we can write (2.185) in the form
A(mML)=
(
1
N
∑N
n=1
cosθn
)
cosθML 0 −
(
1
N
∑N
n=1
sinθn
)
sinθML 0. (2.187)