Stefan Boltzmann equation blackbody radiator estimate of optical power output:

A plasma is considered in the blackbody limit when it is optically thick and emits radiation that closely resembles a perfect blackbody spectrum.  This occurs when the plasma is “optically thick, “meaning it is dense enough to absorb and re-emit radiation at all wavelengths.  In the blackbody limit, a plasma’s emission temperature is equal to its kinetic electron temperature (Te).  The electron temperature of a plasma can be determined from its blackbody radiation curve by analyzing the shape and peak wavelength of the emitted spectrum and fitting it to Planck’s Law.  The emissivity of a plasma at the blackbody limit is 1.  The blackbody emission spectrum of the SunCell is typically between 5000K to 5600K corresponding to an irradiance of 3.54408 X 107 W/m2 and 5.57668 X 107 W/m2, respectively.

 

Blackbody calculator:

https://www.spectralcalc.com/blackbody_calculator/blackbody.php

 

The surface area of the plasma that is optically thick can be determined using a camera that captures the central portion that is opaque or thick to radiation as discerned by the absence of transparency.  As shown in the video the central plasma is generated at a temperature between 5000K to 5600K by the hydrino reaction while the neutral gas, quartz dome, injectors, and SunCell reaction chamber remains relatively cold due to the transmission of the blackbody radiation through the quartz dome at nearly 100% efficiency (i.e. near the reflection limit) in wavelength of 160 nm to 3 um.

 

https://www.tydexoptics.com/materials1/for_transmission_optics/crystal_quartz/

 

Estimate of thermal power output:

Approximate radiating SunCell body surfaces not including the dome is 1022 in2 (0.66 m2).  At 800°K the radiative power with e = 1 is 23,226 W/m2 X 0.66 m2 = 15,300 W which matches the required induction heater input power requirement during startup.

 

 

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