Unit 30 Probability limits

First, go back and review the GLP, and understanf that ARMA processes can be expressed in GLP form as:

Xtμ=j=0ψjatj, where at is normal white noise. some more math: the forecast error is defined as:

et0()=Xt0+ˆXt0() We can rewrite this in GLP form as =1k=0ψkat0+k Since a is normal, e should also be normal, its expeced value should be zero, and its variance is just the variance of it in GLP form. We can rewrite this as: var(et0())=σ2a1j=0ψ2j This saves us a bunch of time and we just need to calculate the white noise variance. This is hard so we can just get it from one of the outputs of fore.arma.wge, and then do the math from there.

30.1 An alternatve way to calculate psi weights

ϕ(B)Xt=θ(B)atXt=θ(B)ψ(B)at=j=0ψjBjat Then you just do the long division and get your answers, by dividing off that tricky a_t component.

30.2 Calculating them

Since we know all this, we have that et0()0[σ2a1j=0ψ2j]1/2N(0,1) =Xt0+ˆXt0()[σ2a1j=0ψ2j]1/2

Given the above, we have that the probability of the above lying in betwieen ±1.96 is about 0.95. Then we expand that out, rewriting it/

P(1.96Xt0+ˆXt0()[σ2a1j=0ψ2j]1/21.96) P(1.96[σ2a1j=0ψ2j]1/2Xt0+ˆXt0()1.96[σ2a1j=0ψ2j]1/2)=0.95

We then have

P(ˆXt0()1.96[σ2a1j=0ψ2j]1/2Xt0+ˆXt0()+1.96[σ2a1j=0ψ2j]1/2)=0.95

This gives us our result!!! Note that this is a huge simplification of the actual method of doing this, it is actually much more complicated what our computer does.