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4-cours rayonnement

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Formule simplifiée simplifi e de Wien :<br />

λT <br />

4-4 4 Etude le L λ .<br />

==> exp ( C 2 / λT ) >> 1<br />

CN<br />

L = C λ<br />

Formule de Rayleigh :<br />

L<br />

λ<br />

λT >> C 2 ==> exp ( C 2 / λT ) = 1 + C 2 / λT<br />

: Le spectre de <strong>rayonnement</strong> d’un un corps noir, à la<br />

température temp rature T, présente pr sente un maximum pour la longueur<br />

λmax max : Le spectre de <strong>rayonnement</strong> d<br />

,<br />

T<br />

C N<br />

λ ,<br />

T<br />

=<br />

1<br />

C<br />

C<br />

1<br />

2<br />

−<br />

5<br />

e<br />

T<br />

λ<br />

−<br />

4<br />

C<br />

λ<br />

T<br />

2<br />

34

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