jairusgarcia
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R=\epsilon\sigmaT^{4}
\epsilon --> emmisivity
\sigma --> Steffan's constant
T[ --> Temp (in Kelvin)
should i start with steffan-boltzmann's equation (since its the nearest formula)?
thanks... ^_^
\epsilon --> emmisivity
\sigma --> Steffan's constant
T[ --> Temp (in Kelvin)
should i start with steffan-boltzmann's equation (since its the nearest formula)?
thanks... ^_^