2 Energy Flashcards
Energy
an agent capable of setting an object in motion
-• units: joule (J) or calorie (cal) (1 J = 0.239 cal)
power
- power: the rate at which energy is released, transferred, or received
- units: Watts (W) (1 W = 1 J s-1)
Types of Energy
- kinetic energy: energy in use
• could relate to the movement of water through a river, or the
vibration of atoms in a rock
• the rate of vibration determines an objects temperature - potential energy: energy in storage
• potential energy is stored in a raindrop, and when it begins to
fall under the influence of gravity, converts the potential
energy into kinetic energy
the rate of ______ determines an objects temperature
vibration
Energy can be transfered by (3)
1.Conduction:
-energy moves through a substance with minimal
movement of molecules (solids)
2.Convection
-energy is transferred by mixing two substances (gases
and liquids)
-hotest molecules rise and release heat at the top of the pot
3.Radiation
-energy propagates through space from one object to
another
-no contact occurring
Radiation
• everything in the Universe emits radiation • this is known as electromagnetic (EM) radiation • the energy moves as a wave through space • electric and magnetic components oscillate through space together • the length of 1 cycle, or wavelength, determines the quality and quantity of the radiation
Radiation Laws:3
1• Planck’s Law tells us that hot objects release most of their energy at short
wavelengths and that short wavelengths contain more energy
2.• Wien’s Law tells us that the wavelength of maximum emission is inversely
related to the objects temperature
-If temperature goes up, maximum emission wavelength goes down
3.• the Stefan-Boltzmann Law tells us that the total amount of energy
released by an object is directly proportional to its temperature
-as the temp of an object rises, then the release of energy increases
the sun releases ____wave energy while the earth releases ___wave energy
short
long
Sun
• the Sun emits energy at a more or less constant rate
• over very long time spans, the output of the Sun changes
• the Sun emitted 30% less energy 4.5 billion years ago
• on shorter time spans, sunspots can enhance solar output
• the number of sunspots cycles on an
11 year cycle, but there have been
long periods of reduced sunspots
• although sunspots are relatively cool
(ie, less energy), the area around them
is much hotter than the normal Sun
surface
• as the energy moves through space from the Sun toward Earth, it is
distributed over a greater and greater volume of the solar system, which
reduces its intensity
• the surface of the sun emits 3.865 x 1026
joules each second (W), but we are
150,000,000 km away from the Sun
.When energy leaves the sun, it starts to radiate out into the solar system
- becomes diluted as it moves through space
- 8 minutes from surface of sun to us
- 1367 W m shortwave radiation hits the upper atmos
Anything shorter then visible is
ANYTHING LONGER is
ULTRAVIOLET
INFRARED
The solar constant
• 1367 W m-2
: known as the solar constant
• this is the energy received at the top of Earth’s atmosphere, and
therefore available to be used by Earth
•Insolation: a measure of the solar energy received on a surface at a given time
• the Sun emitted less energy in the past
• sunspot cycle results in a 0.11% variation in energy emitted over 11
years
• sometimes Earth is closer to the Sun, reducing the distance between
them and increasing the energy received
• DO THESE AFFECT CLIMATE?
insolation
a measure of the solar energy received on a surface at a given time
• often used as an anagram of incoming solar radiation
• Earth’s atmosphere is not transparent to incoming solar radiation
• insolation can be absorbed by the atmosphere, warming it up
• insolation can be reflected by the atmosphere, scattering the
energy in any direction
• insolation can be transmitted by the atmosphere, in which case it
reaches Earth’s surface
• these 3 processes are responsible for the nature and distribution of
temperature throughout the atmosphere, and explain many atmospheric
phenomena
____W m-2
: known as the solar constant
1367
Earth/Sun Geometry
• Earth is tilted at approximately 23.4° to the orbital plane (the ecliptic)
around the Sun and is rotating on this axis as well as revolving around the
Sun
• this gives us the day and year, as well as the seasons
Absorption
• gases, liquid droplets, and solid particles in Earth’s atmosphere reduce
the intensity of insolation by absorbing some of the Sun’s energy
• this is an energy transfer - the energy is transferred to the absorber,
which gains that energy and warms
• most gases, droplets and particles are only able to absorb a specific
wavelength of insolation
•Ex:ozone is very effective at absorbing ultraviolet wavelengths
• eg, visible light is not absorbed by the atmosphere, thereby allowing
us to see things
• standing at Earth’s surface, we normally do not receive the full spectrum
of solar radiation, only the wavelengths that are able to pass through the
atmosphere
• these are known as atmospheric windows or absorption bands
• water vapour is also a good absorber of insolation, absorbing longer
wavelengths in the infrared part of the spectrum
• the more water vapour in the atmosphere, the more infrared
radiation that will be absorbed
• consider deserts – there is little water vapour in the air, so all of the
infrared radiation reaches the surface and warms your skin, making
you feel hot
• if you find shade, you will cool down because you are out of the
direct sun
• on the other hand, if you were in a jungle where atmospheric
moisture is always high, the infrared radiation is absorbed in the
atmosphere, and the air feels hot
• if you find shade, you will still be hot because the air carries the
heat, not the sunlight
______ light is not absorbed by the atmosphere, thereby allowing
us to see things
visible
• standing at Earth’s surface, we normally do not receive the full spectrum
of solar radiation, only the wavelengths that are able to pass through the
atmosphere
• these are known as _____________ or __________
atmospheric windows
absorption bands
visible light is 0._ to 0._
0.4 to 0.7
Reflectance 2 types
• sometimes, instead of absorbing energy, gases, particles and droplets
simply reflect the energy away
• reflection occurs in 2 ways:
- specular reflection:
is a type of surface reflectance often described as a mirror-like reflection of light from the surface. In specular reflection, the incident light is reflected into a single outgoing direction. - diffuse reflection: the radiation strikes a surface but is reflected as
a large number of weak beams in many different directions
• this is how most natural objects work
albedo
Albedo: the ratio of visible light that is reflected by an object
• generally, we can tell the albedo of an object by its colour
• white objects have a high albedo because they reflect a lot of
visible light
• black objects have a low albedo because they reflect little visible
light
Albedo:%
fresh snow=
wet soil=
80-85
10
scattering
• insolation passing through the atmosphere will
eventually interact with a gas molecule, liquid
droplet, or solid particle
• if not absorbed, the energy will bounce off the
substance and scatter in many directions
• some insolation may go back into space,
some may reach the surface, some may be
scattered again
• when scattered insolation reaches Earth’s
surface, it is diffuse radiation
• diffuse radiation explains why shadows are
not perfectly black