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THERMODYNAMICS (RADIATION)

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THERMODYNAMICS (RADIATION)

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FINAL EXAMINATION

Created by

Grace Balahay
Grace Balahay
United States

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THERMODYNAMICS (RADIATION)
 

THERMODYNAMICS (RADIATION)Online version

FINAL EXAMINATION

by Grace Balahay
1

is transported through electromagnetic mechanism, which allows energy emission through regions of space, similar in nature as light and radio waves.

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2

it is the energy flow impinging per unit time and unit area at the interface, denoted by I.

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3

it is the energy leaving the interface back into the medium 1.

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4

the ratio of the reflected to the incident radiation

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5

it is the energy absorbed while the in medium 2.

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6

the ratio of the absorbed to the incident radiation

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7

it is the radiant energy leaving medium 2 somewhere through its surfaces.

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8

the ratio of the transmitted to the incident radation

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9

it is the radiative energy flux that travel through the interface into medium 1 in a direction opposite the incident radiation

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10

it is the total radiant energy leaving a unit of surface area per unit time, emitted and reflected energy.

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11

it is the total radiation energy incident upon a unit of surface area per unit time

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12

it is the total emitted thermal radiation leaving a unit of black body surface area per unit of time, reflected energy not included

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13

not constant property but usually it varies with the temperature and wavelength of the radiating body

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14

absorptivity and the emissivity of a body are the same when the body is in thermal equilibrium with its surroundings

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15

states that the amount of radiation from a block body is proportional to the fourth power of the absolute temperature

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16

indicates the maximum level in the planck's distribution of thermal radiation

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17

is defined as the fraction of thermal radiation that leaves a surface and intercepted by another surface

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18

also called as gray body is technically defined as that the monochromatic emissivity ελ of the body is independent of wavelength.

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19

is the ratio of the monochromatic emissive powers of a body to the blackbody at certain wavelength and temperature.

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