All indications are that the visible spectrum contains very little of the 
energy being radiated so what we see can not be used to figure the radiated 
power.   Many other variables appear to get into the fray which forces us to 
rely upon calibration if we are to achieve accurate accounting of the radiated 
and convected power.  It is unfortunate that the input power was not the same 
during both the dummy run and the active one since the increased apparent 
temperature would have clearly demonstrated excess power if any was present.

I am left with believing that excess power was generated due to the rapid 
increase in calculated output power when a small increase in input power was 
applied.  This is a characteristic of an ECAT system with positive thermal 
feedback.  A passive system would not display this behavior.

Dave

 

 

 

-----Original Message-----
From: Alan Fletcher <[email protected]>
To: vortex-l <[email protected]>
Sent: Wed, Oct 29, 2014 11:35 am
Subject: Re: [Vo]:MFMP interviews spokesman from WILLIAMSON



From: "Eric Walker" <[email protected]>
Sent: Tuesday, October 28, 2014 10:20:52 PM




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


Yes, that's how Planck's formula/integration works. It TRIES to send a 
Boltzmann curve, but this is modulated by the emissivity spectrum.
As the temperature increases the spectral peak get higher and shifts to shorter 
wavelengths. If the emissivity is higher  then the total power will increase, 
otherwise (as in this case) it decreases.


Per Manara the transmission looks negligible outside the visible range, where 
there's practically no blackbody power anyway up to 1400C. (It moves to the 
visible at much higher temperatures -- 4000  to 6000C).








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