On Tue, Oct 28, 2014 at 12:36 PM, Alan Fletcher <[email protected]> wrote:
Basically what happens is that as the temperature changes the peak of the > blackbody spectrum moves through different parts of the > emissivity/wavelength curve. Are you assuming a standard Boltzmann curve that just shifts its peak according to emittance? Is it possible that the frequency and heat-dependant combination of emittance, transmissivity and reflection make it so that there is a distribution other than a Boltzmann distribution for the alumina shell? Eric
