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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

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