6 folier pr. side - NTNU
6 folier pr. side - NTNU
6 folier pr. side - NTNU
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<strong>NTNU</strong><br />
<strong>NTNU</strong><br />
<strong>NTNU</strong><br />
Slide 373<br />
Slide 375<br />
Slide 377<br />
Resulterende pu-modell for<br />
asynkronmaskinen på komponentform<br />
k<br />
k k 1 dψ<br />
sα<br />
k<br />
u sα<br />
= rs<br />
⋅ isα<br />
+ − f k ⋅ ψ sβ<br />
ωn<br />
dt<br />
k<br />
1 dψ<br />
k k<br />
sβ<br />
k<br />
u sβ<br />
= rs<br />
⋅ isβ<br />
+ + f k ⋅ ψ sα<br />
ωn<br />
dt<br />
k<br />
1 dψ<br />
k k<br />
sγ<br />
u sγ<br />
= rs<br />
⋅ isγ<br />
+<br />
ωn<br />
dt<br />
dθ<br />
k<br />
= ωn<br />
⋅ f k<br />
dt<br />
ψ<br />
ψ<br />
k<br />
sα<br />
k<br />
sβ<br />
k<br />
sγ<br />
= x ⋅ i<br />
s<br />
s<br />
sσ<br />
k<br />
sα<br />
k<br />
sβ<br />
k<br />
sγ<br />
h<br />
h<br />
k<br />
rα<br />
+ x ⋅ i<br />
k<br />
rβ<br />
= x ⋅ i + x ⋅ i<br />
ψ = x ⋅ i<br />
k<br />
k k 1 dψ<br />
rα<br />
k<br />
u rα<br />
= rr<br />
⋅ i rα<br />
+ − ( f k − n)<br />
⋅ ψ rβ<br />
ωn<br />
dt<br />
k<br />
1 dψ<br />
k k<br />
rβ<br />
k<br />
u rβ<br />
= rr<br />
⋅ i rβ<br />
+ + ( f k − n)<br />
⋅ ψ rα<br />
ωn<br />
dt<br />
k<br />
1 dψ<br />
k k<br />
rγ<br />
u rγ<br />
= rr<br />
⋅ i rγ<br />
+<br />
ωn<br />
dt<br />
dθr<br />
= ωn<br />
⋅ f r = ωn<br />
⋅ ( f k − n)<br />
dt<br />
k<br />
rα<br />
k<br />
rγ<br />
rσ<br />
k<br />
sα<br />
k<br />
rγ<br />
k<br />
rα<br />
ψ = x h ⋅ i + x r ⋅ i<br />
k<br />
k<br />
ψ rβ<br />
= x h ⋅ i sβ<br />
+ x r ⋅ i<br />
ψ = x ⋅ i<br />
k<br />
rβ<br />
Trondheim 2000<br />
Definisjoner av magnetiseringsstrømmer<br />
■ Sammenheng mellom flukser og magnetiseringsstrømmer:<br />
k<br />
s<br />
h<br />
k<br />
μs<br />
k<br />
r<br />
k<br />
μr<br />
ψ = x ⋅ i ψ = x ⋅ i ψ = x ⋅ iμ<br />
■ Settes inn i uttrykkene for fluksforslyngningene:<br />
k k<br />
k<br />
ψ = x s s ⋅ is<br />
+ x h ⋅ i r<br />
k<br />
k k<br />
ψ = x r h ⋅ i s + x r ⋅ i r<br />
h<br />
k<br />
h<br />
x s = x h + x sσ<br />
= x h + σs<br />
x h = (1+<br />
σs<br />
) ⋅ x h<br />
x r = x h + x rσ<br />
= x h + σr<br />
x h = (1+<br />
σr<br />
) ⋅ x h<br />
k<br />
k k<br />
k k<br />
k<br />
k k k<br />
i μs<br />
= ( 1+<br />
σs<br />
) ⋅ i s + i r i μr<br />
= is<br />
+ ( 1 + σr<br />
) ⋅ i r iμ<br />
= i s + i r<br />
Statororientert modell<br />
■ Aksesystemet og de ������� stator og rotor viklinger er spikret<br />
fast i forhold til ������:<br />
dθ<br />
k<br />
= ωn<br />
⋅ f k ≡ 0<br />
dt<br />
dθ<br />
= ωn<br />
⋅ n<br />
dt<br />
θ r = −θ<br />
■ Settes inn i uttrykkene for fluksforslyngningene:<br />
s<br />
s s 1 dψ<br />
s<br />
s s<br />
s<br />
u s = rs<br />
⋅ is<br />
+<br />
ψ = x s s ⋅ is<br />
+ x h ⋅ i r<br />
ω dt<br />
n<br />
s<br />
s 1 dψ<br />
r<br />
s<br />
0 = rr<br />
⋅ i r + − �⋅<br />
n ⋅ ψ r<br />
ωn<br />
dt<br />
me<br />
=<br />
s T ( is<br />
)<br />
s s s s s<br />
�ψ<br />
= ψ s sα<br />
⋅ isβ<br />
− ψ sβ<br />
⋅ isα<br />
s<br />
s s<br />
ψ = x r h ⋅ i s + x r ⋅ i r<br />
■ For to dimensjonale romvektorer har man at romvektoren i<br />
statorkoordinater lik dens koordinatvektor<br />
s s ⎡1⎤<br />
⎡0⎤<br />
⎡I<br />
a ⎤ s<br />
I s = Ia<br />
a + Ib<br />
b = Ia<br />
⎢ I b = ⎢ = Is<br />
0<br />
⎥ + ⎢<br />
1<br />
⎥<br />
I<br />
⎥<br />
⎣ ⎦ ⎣ ⎦ ⎣ b ⎦<br />
h<br />
k<br />
Trondheim 2000<br />
Trondheim 2000<br />
<strong>NTNU</strong><br />
<strong>NTNU</strong><br />
<strong>NTNU</strong><br />
Slide 374<br />
Slide 376<br />
Slide 378<br />
Ser bort i fra γ-systemet ……….<br />
■ Kan da benytte to-dimensjonale romvektorer:<br />
k<br />
k k 1 dψ<br />
s<br />
k<br />
u s = rs<br />
⋅ i s + + � ⋅ f k ⋅ ψ s<br />
ωn<br />
dt<br />
k<br />
k k 1 dψ<br />
r<br />
k<br />
u r = rr<br />
⋅ i r + + � ⋅ ( f k − n)<br />
⋅ ψ r<br />
ωn<br />
dt<br />
m e =<br />
k T k k k k k<br />
( is<br />
) � ψ = ψ ⋅ i − ψ ⋅ i<br />
dn<br />
Tm<br />
= m e − m L<br />
dt<br />
dθ<br />
k<br />
= ωn<br />
⋅ f k<br />
dt<br />
s<br />
sα<br />
sβ<br />
sβ<br />
sα<br />
2<br />
J ⋅ Ω basis<br />
Tm<br />
=<br />
Sn<br />
dθ<br />
= ωn<br />
⋅ n<br />
dt<br />
k<br />
k<br />
k<br />
k ⎡i<br />
⎤ ⎡ ⎤ ⎡ψ<br />
⎤<br />
sα<br />
k u sα<br />
k sα<br />
i s = ⎢ k ⎥ u s = ⎢ k ⎥ ψ s = ⎢ k ⎥<br />
⎢⎣<br />
i sβ<br />
⎥⎦<br />
⎢⎣<br />
u sβ<br />
⎥⎦<br />
⎢⎣<br />
ψ sβ<br />
⎥⎦<br />
k k<br />
k<br />
ψ = x s s ⋅ is<br />
+ x h ⋅ i r<br />
k<br />
k k<br />
ψ = x r h ⋅ is<br />
+ x r ⋅ i r<br />
θ r = θk<br />
− θ<br />
⎡0 −1⎤<br />
= ⎢ ⎥<br />
⎣1<br />
0 ⎦<br />
Orientering av aksesystem<br />
■ Følgende orienteringer<br />
av aksesystem er vanlig:<br />
➨ Statororientert modell;<br />
dvs. at α k orienteres etter<br />
stator a-fase viklingsakse<br />
a s ; dvs. at f k=0<br />
➨ Rotororientert modell;<br />
dvs. at α k orienteres etter<br />
����� a-fase viklingsakse<br />
a r ; dvs. at f k=n<br />
➨ Romvektor-orientering;<br />
dvs. at α k orienteres etter<br />
en romvektor. Det er<br />
vanlig å benytte<br />
rotorfluksens romvektor;<br />
dvs. at f k= f ψr . Stasjonært<br />
lik f s<br />
k<br />
β<br />
�<br />
s<br />
b<br />
θ�<br />
Rotorfluksorientert modell<br />
■ Aksen α k ”spikres” fast<br />
til rotorfluksvektoren:<br />
s<br />
θk<br />
= ξr<br />
k<br />
dψ<br />
k rβ<br />
ψ rβ<br />
≡ ≡ 0<br />
dt<br />
⇓<br />
r<br />
θr<br />
= ξ r<br />
s r<br />
ξr<br />
= ξr<br />
+ θ<br />
■ Romvektoren i α k -<br />
aksen:<br />
dψ<br />
k rβ<br />
ψ rβ<br />
≡ ≡ 0<br />
dt<br />
k<br />
ψ ≡ ψ<br />
rα<br />
k<br />
r<br />
k<br />
β<br />
s<br />
b<br />
θ�<br />
Trondheim 2000<br />
k<br />
α<br />
Ψr<br />
s<br />
a<br />
Trondheim 2000<br />
k<br />
α<br />
Ψr<br />
s<br />
a<br />
Trondheim 2000