12MAP OF STANDARDS QTR 3
Energy in Earth Systems, Structureand Composition of the AtmosphereScience Standards and Frameworks, pg. 263-268, 274-4a-4b. Students know the relative amount of incoming solar energycompared withEarth’s internal energyand theenergy used by society.4c.Students knowthe differentatmospheric gasesthat absorbthe Earth’s thermal radiation
and explain the mechanism and significanceof the greenhouseeffect.8a.Students knowthe thermalstructure and chemical compositionof theatmosphere.8c.Students knowthelocation of the ozone layerinthe upper atmosphere, its rolein absorbing ultraviolet
radiation, and the way inwhich this layer varies both naturally and in response to human activities.^
- Students should be able to describe the fate of incoming solar radiation [wavelengths]
in terms of reflection
[clouds,atmospheric gases, dust, Earth’s surface, plants], absorption[water vapor, dustatmospheric gases, Earth’s surface, plants] and photosynthesis[absorbedlight]. 2. Students should be able to create, as well as analyze, a diagram that describes the fate of incoming solar radiationin% reflection, % absorption, and % photosynthesis.- Students should be able to enumerate the different atmospheric gases
that absorbEarth’s thermal radiation. 2. Students should be able to explain the mechanism of greenhouse effect[create andanalyze a diagram of the phenomenon]. 3. Students should be able to discuss the significance of the greenhouse effect[effect onecosystems, weather] and analyze potential solutions.- Students should be able to describe the gaseous composition
of the atmosphereand how density decreases with elevation.- Students should be able to discuss the thermal structure of the atmosphere
by identifyingthe four layersthat make itup and describing the characteristics of each layer. 3. Students should be able to analyze a diagram of the structure of the atmosphere.- Students should be able to identify the formation and location of the ozone layer
in the upper atmosphere.- Students should be able to explain the role of the ozone layer
in absorbingharmful UV radiation.- Students should be able to explain how certain human activities have caused damage to
the ozone layerandsuggest possible solutions.5a. Students will explain
and diagram
howdifferential heatingof theEarth results in circulation patterns in the atmosphere and oceans- Students should be able to explain how circulation cells
result from differential heating of the Earth from the Sun. 2. Students should be able to identify and describe the three different circulation cycles
thatexist on Earth and how these cycles influence weather patterns.- Students should be able to explain how unequal heating of the Earth’s surface
alsocauses large thermally-driven currents in the oceans.- Students should be able to explain the occurrence of seasons and diagram
[oranalyze one] the different Earth positions corresponding to the different seasons.5b.Students know the
relationshipbetween the rotationof Earth and the circular motions of ocean currents and air in pressure centers.- Students should be able to describe how Earth’s rotation and the Coriolis effect
causesthe direction of fluid flowto bedifferent in the North and South hemispheres.- Student should be able to create a model or diagram
ofhow Earth’s rotation and the Coriolis effectcan lead to thecreation of circular motions of air in pressure centers.5d.Students knowproperties of ocean water, such astemperature and salinity, can be used to explain the layeredstructure of the oceans, the generation of horizontal andvertical ocean currents, and the geographic distribution ofmarine organisms.
a. Students will enumerate the different properties of ocean water,suchas temperature, salinity, density and describe how each is measured. b. Students should be able to describe how density differencescan drivecirculations in oceansand how temperature differences can be used toexplain the layered structureof the ocean.5c. Students know the origin and effects of temperature inversions.- Students can explain how temperature inversions arise. 2. Students can enumerate possible effects of temperature inversions [e.g. trapping of pollutants].
8b. Students know how the composition of the Earth’s atmosphere has evolved over geologic timeand know the effect of outgassing, the variations of carbon dioxide concentration, and the origin of atmospheric oxygen.- Students can describe how the atmosphere of today differs from the primordial atmosphe
re billions of years ago.- Students can explain how Oxygen build up occurred and how the gaseous composition of early atmosphere changed. 3. Students can explai
n the reason behind CObuild-up in 2the atmosphere of today.