# EESA01H3 Lecture Notes - Lecture 5: Solar Constant, Heat Flux, Global Warming

93 views11 pages
Published on 25 Oct 2013
School
Course
Professor
Environment lecture 5
Assignments due 15 days after tutorial, due in dropboxes
Midterm covers all up to 6th lecture
Water- relates to second assignment
Energy flux
The rate (amount per time) of energy (joules) received at a surface= power in J/s aka a Watt (W)
Energy we get is emitted at us as a wave, that wavelength is inversely proportional to the temp
of the surface of what is emitting the radiation
How much energy is coming in? Relates to how you feel, eg hot or cold
Power per surface area is an Energy Flux and is measured in W/m^2
o If take watt, and see how much there is over a meter squared = energy flux
o We talk about how much energy we get from sun in W/m^2
Physical equation- Stefan boltzmann law
o Stefan Boltzmann law- The rate of energy emitted by a substance
o
o Temp to the power of 4 in kelvin. eg temp of earth into kelvin to the power of 4
o Sigma is the constant. 5678 easy to remember, will be given
o Epsilon- a characteristic called emissivity, the efficiency at which a given surface can
emit energy. Eg fuel efficiency. 97% fuel efficient, 3% is lost
o Only thing that has an emissivity of 1.0 is the sun, a black body emitter, emit at 100%
efficiency, everything else has emissivity between 0 and 9.999
Eg find the variables and ask about the energy flux
Solar constant
Solar constant- the rate at which insolation (incoming solar radiation) is received at the outer
atm of Earth
Energy flux is important because we want to know how much energy is going in and coming out
Solar constant 1367 watts per meter squared
Energy hitting earth averages at 342 W/m^2
Energy hitting the earth is way less, because it is geometric problem
o When sun radiation is hitting the earth, it’s not hitting the whole sphere, just a circle
o 4πr^2 vs πr^2
o 1367/4=342
Unlock document

This preview shows pages 1-3 of the document.
Unlock all 11 pages and 3 million more documents.

Already have an account? Log in
o
Latitude controls Fig 14.4
Not to say 342 watts everywhere on average, lots of other major controls on how much solar
radiation hits the surface of the earth
Latitude- how direct the hit is
o Thickness of the atmosphere of which the radiation has to move through
o Eg equator, direct hit, going through least amount of atm possible and concentrating
more sunlight on one spot
o Higher latitudes- same amount of radiation spread out big area therefore it’s cooler as
you go away from equator
o Also If wrapped atm of equal width around the earth ,at the higher latitudes the atm
start to bend towards the poles, and so same thickness but some rays are hitting the
earth at an angle eg 60 degree angle, so more atmosphere the sunlight has to go
through eg greenhouse gases and clouds. More chances if it being absorbed and
reflected
Unlock document

This preview shows pages 1-3 of the document.
Unlock all 11 pages and 3 million more documents.

Already have an account? Log in
At equator- sunlight directly hitting directly- air obsorbs less energy ue to shorter path through
atm
o More sunlight per unit of surface area
Near poles- low angle of incoming sunlight- air absorbs more energy due to longer path through
atm
o Less sunlight per unit of surface area
Earth’s energy balance Fg 15.1
Incoming solar radiation 342, as get close to surface of earth, have greenhouse gases
o Most abundant greenhouse gas is water, eg as clouds
o Relative constant amount of water whereas the other gases like co2 is increasing
o Solar radiation comes in, a lot gets absorbed by atm, a lot is reflected and 50% is
actually absorbed into surface
o If have incoming shortwave radiation, and is reflected away, that reflected radiation
remains as same wavelength, shortwave
o If it is absorbed by the surface of the earth and remitted it is remitted according to
wien’s displacement law, as to the temp of the earth not the sun. So when absorbed
and re-emitted the earth is much cooler, so less energy flux, so it is much longer
wavelength. That’s why most radiation outgoing from earth is long wave
Some energy going through transpiration, and thermals (temp related things)
Unlock document

This preview shows pages 1-3 of the document.
Unlock all 11 pages and 3 million more documents.

Already have an account? Log in

# Get OneClass Notes+

Unlimited access to class notes and textbook notes.

75% OFF
\$8 USD/m
###### Monthly
\$30 USD/m
You will be charged \$96 USD upfront and auto renewed at the end of each cycle. You may cancel anytime under Payment Settings. For more information, see our Terms and Privacy.
Payments are encrypted using 256-bit SSL. Powered by Stripe.