The emissive power of a blackbody depends on the fourth power of the temperature and is given by W = AT* where: BTU W = emissive power ft² – hr, BTU A = Stefan – Boltzmann constant, 0.171x10-8 ft2 – hr – °Rª T = temperature in °R What is the value of A in the units; т2 — s — К4

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The emissive power of a blackbody depends on the fourth power of the temperature and is given by
W = AT*
where:
BTU
W
emissive power
ft² – hr,
BTU
A
Stefan – Boltzmann constant, 0.171x10-8.
ft2 – hr – °R4
T
temperature in °R
What is the value of A in the units
т2 — s — K4
Transcribed Image Text:The emissive power of a blackbody depends on the fourth power of the temperature and is given by W = AT* where: BTU W emissive power ft² – hr, BTU A Stefan – Boltzmann constant, 0.171x10-8. ft2 – hr – °R4 T temperature in °R What is the value of A in the units т2 — s — K4
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