unit 3, exam 1 Flashcards

1
Q

energy

A

ability of object or system to do work

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2
Q

temp

A

how we quantify energy of a system

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3
Q

absolute 0

A

never observed in natural world.

basically no energy

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4
Q

1st law of thermodynamics

A

energy never created or destroyed

conservation of energy

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5
Q

2nd law of thermodynaics

A

energy flows form regions of higher concentration to regions of lower concentration

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6
Q

electromagnetic radiation

A

transfer of energy in the form of waves that move at the speed of light

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7
Q

electromagnetic spectrum

A

devised to differentiate the varying properties of these waves according to wavelength

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8
Q

heat

A

the sensible component of energy moving from a higher (warmer)state to a lower(cooler) state

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9
Q

blackbody

A

an object that is a perfect absorber and a perfect emitter

no such objects but some are close (earth)

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10
Q

wiens displacement law

A

physical relationship describing the intensity of an objects emitted energy across the electromagnetic spectrum.

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11
Q

shortwave radiation

A

suns energy

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12
Q

longwave radiation

A

earths energy

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13
Q

flux

A

watts per square meter

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14
Q

stefan boltzmann law

A

total energy flux emitted by a blackbody across all wavelengths is proportioned to the fourth power of the absolute T of the object
E=o*T^4

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15
Q

global radiation budget

A

our way of keeping track of how radiation travels through the atmosphere on its incoming and outgoing travel

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16
Q

scatter

A

solar radiation dispersing forward, backward adn sideways after hitting a particle

17
Q

relection

A

special case of scattering at the interface between two different media (such as air and cloud)
ex)sky blue, sunset red

18
Q

albedo

A

fraction of radiation redirected (reflected) by some interface

19
Q

dark surfaces

A

low albedo

20
Q

white surfaces

A

high albedo

21
Q

temperature gradiant

A

difference in T over a distance

22
Q

circle of illumination

A

distinguishing line between day and night

23
Q

aphelion

A

july earth is furthest form sun

24
Q

perihelion

A

january earth is closest to the sun

25
Q

radiation heating

A

absorbing faster than emitting therefore T increases

26
Q

radiation cooling

A

emits faster than absorbs therefore T decreases

27
Q

conduction

A

transfer through contact
thermal conductivity-metal vs styrofoam
heat conductivity-ration of rate of heat transport

28
Q

convection

A

heat transfer by fluid motions

buoyancy on air parcels

29
Q

Diurnal

A

reoccurring daily cycle