Temperature of Medium given Emissive Power of Blackbody Solution

STEP 0: Pre-Calculation Summary
Formula Used
Temperature of Medium = (Emissive Power of Blackbody through Medium/[Stefan-BoltZ])^(1/4)
Tm = (Ebm/[Stefan-BoltZ])^(1/4)
This formula uses 1 Constants, 2 Variables
Constants Used
[Stefan-BoltZ] - Stefan-Boltzmann Constant Value Taken As 5.670367E-8
Variables Used
Temperature of Medium - (Measured in Kelvin) - Temperature of Medium is defined as the degree of hotness or coldness of the Transparent medium.
Emissive Power of Blackbody through Medium - (Measured in Watt per Square Meter) - Emissive Power of Blackbody through Medium is the energy of thermal radiation emitted in all directions per unit time from each unit area of a surface of blackbody at any given temperature.
STEP 1: Convert Input(s) to Base Unit
Emissive Power of Blackbody through Medium: 265 Watt per Square Meter --> 265 Watt per Square Meter No Conversion Required
STEP 2: Evaluate Formula
Substituting Input Values in Formula
Tm = (Ebm/[Stefan-BoltZ])^(1/4) --> (265/[Stefan-BoltZ])^(1/4)
Evaluating ... ...
Tm = 261.462058687104
STEP 3: Convert Result to Output's Unit
261.462058687104 Kelvin --> No Conversion Required
FINAL ANSWER
261.462058687104 261.4621 Kelvin <-- Temperature of Medium
(Calculation completed in 00.004 seconds)

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University School of Chemical Technology-USCT (GGSIPU), New Delhi
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Radiation System consisting of Transmitting and Absorbing Medium between Two Planes. Calculators

Net Heat Exchange in Transmission Process
​ LaTeX ​ Go Radiation Heat Transfer = Surface Area of Body 1*Radiation Shape Factor 12*Transmissivity of Transparent Medium*(Radiosity of 1st Body-Radiosity of 2nd Body)
Energy Leaving Surface 1 that is Transmitted through Medium
​ LaTeX ​ Go Energy Leaving Surface = Radiosity of 1st Body*Surface Area of Body 1*Radiation Shape Factor 12*Transmissivity of Transparent Medium
Energy Emitted by Medium
​ LaTeX ​ Go Radiosity for Transparent Medium = Emissivity of Medium*Emissive Power of Blackbody through Medium
Emissive Power of Blackbody through Medium
​ LaTeX ​ Go Emissive Power of Blackbody through Medium = [Stefan-BoltZ]*(Temperature of Medium^4)

Important Formulas in Gas Radiation, Radiation Exchange with Specular Surfaces and more Special Cases Calculators

Initial Radiation Intensity
​ LaTeX ​ Go Initial Radiation Intensity = Radiation Intensity at Distance x/exp(-(Monochromatic Absorption Coefficient*Distance))
Monochromatic Transmissivity
​ LaTeX ​ Go Monochromatic Transmissivity = exp(-(Monochromatic Absorption Coefficient*Distance))
Monochromatic Absorption Coefficient if Gas is Non-Reflecting
​ LaTeX ​ Go Monochromatic Absorption Coefficient = 1-Monochromatic Transmissivity
Monochromatic Transmissivity if Gas is Non Reflecting
​ LaTeX ​ Go Monochromatic Transmissivity = 1-Monochromatic Absorption Coefficient

Temperature of Medium given Emissive Power of Blackbody Formula

​LaTeX ​Go
Temperature of Medium = (Emissive Power of Blackbody through Medium/[Stefan-BoltZ])^(1/4)
Tm = (Ebm/[Stefan-BoltZ])^(1/4)

What is Radiation?

Radiation is energy that comes from a source and travels through space at the speed of light. This energy has an electric field and a magnetic field associated with it, and has wave-like properties. You could also call radiation “electromagnetic waves”.

What is Emissivity?

Emissivity is defined as the ratio of the energy radiated from a material's surface to that radiated from a perfect emitter, known as a blackbody, at the same temperature and wavelength and under the same viewing conditions. It is a dimensionless number between 0 (for a perfect reflector) and 1 (for a perfect emitter).

How to Calculate Temperature of Medium given Emissive Power of Blackbody?

Temperature of Medium given Emissive Power of Blackbody calculator uses Temperature of Medium = (Emissive Power of Blackbody through Medium/[Stefan-BoltZ])^(1/4) to calculate the Temperature of Medium, The Temperature of Medium given Emissive Power of Blackbody formula is defined as the function of emissive power of blackbody and Stefan Boltzmann constant. The emissive power of a body is defined as the ratio of energy emitted (or radiated) per unit area per second to the amount of heat energy emitted per unit area per second by a perfectly black body at the same temperature. When a body’s temperature rises above absolute zero, it emits heat, which is referred to as emission. When this emitted heat travels in the form of an electromagnetic wave, it is referred to as thermal radiation. At any given temperature, this power is the energy of thermal radiation emitted in all directions per unit time per unit area of a surface. Temperature of Medium is denoted by Tm symbol.

How to calculate Temperature of Medium given Emissive Power of Blackbody using this online calculator? To use this online calculator for Temperature of Medium given Emissive Power of Blackbody, enter Emissive Power of Blackbody through Medium (Ebm) and hit the calculate button. Here is how the Temperature of Medium given Emissive Power of Blackbody calculation can be explained with given input values -> 261.4621 = (265/[Stefan-BoltZ])^(1/4).

FAQ

What is Temperature of Medium given Emissive Power of Blackbody?
The Temperature of Medium given Emissive Power of Blackbody formula is defined as the function of emissive power of blackbody and Stefan Boltzmann constant. The emissive power of a body is defined as the ratio of energy emitted (or radiated) per unit area per second to the amount of heat energy emitted per unit area per second by a perfectly black body at the same temperature. When a body’s temperature rises above absolute zero, it emits heat, which is referred to as emission. When this emitted heat travels in the form of an electromagnetic wave, it is referred to as thermal radiation. At any given temperature, this power is the energy of thermal radiation emitted in all directions per unit time per unit area of a surface and is represented as Tm = (Ebm/[Stefan-BoltZ])^(1/4) or Temperature of Medium = (Emissive Power of Blackbody through Medium/[Stefan-BoltZ])^(1/4). Emissive Power of Blackbody through Medium is the energy of thermal radiation emitted in all directions per unit time from each unit area of a surface of blackbody at any given temperature.
How to calculate Temperature of Medium given Emissive Power of Blackbody?
The Temperature of Medium given Emissive Power of Blackbody formula is defined as the function of emissive power of blackbody and Stefan Boltzmann constant. The emissive power of a body is defined as the ratio of energy emitted (or radiated) per unit area per second to the amount of heat energy emitted per unit area per second by a perfectly black body at the same temperature. When a body’s temperature rises above absolute zero, it emits heat, which is referred to as emission. When this emitted heat travels in the form of an electromagnetic wave, it is referred to as thermal radiation. At any given temperature, this power is the energy of thermal radiation emitted in all directions per unit time per unit area of a surface is calculated using Temperature of Medium = (Emissive Power of Blackbody through Medium/[Stefan-BoltZ])^(1/4). To calculate Temperature of Medium given Emissive Power of Blackbody, you need Emissive Power of Blackbody through Medium (Ebm). With our tool, you need to enter the respective value for Emissive Power of Blackbody through Medium and hit the calculate button. You can also select the units (if any) for Input(s) and the Output as well.
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