12
MAP OF STANDARDS QTR 3
Energy in Earth Systems, Structure
and Composition of the Atmosphere
Science Standards and Frameworks, pg. 263-268, 274-
4a-4b. Students know the relative amount of incoming solar energy
compared with
Earth’s internal energy
and the
energy used by society.
4c.
Students know
the different
atmospheric gases
that absorb
the Earth’s thermal radiation
and explain the mechanism and significance
of the greenhouse
effect.
8a.
Students know
the thermal
structure and chemical composition
of the
atmosphere
.
8c.
Students know
the
location of the ozone layer
in
the upper atmosphere, its role
in absorbing ultraviolet
radiation
, and the way in
which 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, dust
atmospheric gases, Earth’s surface, plants] and photosynthesis
[absorbed
light]. 2. Students should be able to create, as well as analyze, a diagram that describes the fate of incoming solar radiation
in
% reflection, % absorption, and % photosynthesis.
- Students should be able to enumerate the different atmospheric gases
that absorb
Earth’s thermal radiation. 2. Students should be able to explain the mechanism of greenhouse effect
[create and
analyze a diagram of the phenomenon]. 3. Students should be able to discuss the significance of the greenhouse effect
[effect on
ecosystems, weather] and analyze potential solutions.
- Students should be able to describe the gaseous composition
of the atmosphere
and how density decreases with elevation.
- Students should be able to discuss the thermal structure of the atmosphere
by identifying
the four layers
that make it
up 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 absorbing
harmful UV radiation.
- Students should be able to explain how certain human activities have caused damage to
the ozone layer
and
suggest possible solutions.
5a
. Students will explain
and diagram
how
differential heating
of the
Earth results in circulation patterns in the atmos
phere 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
that
exist on Earth and how these cycles influence weather patterns.
- Students should be able to explain how unequal heating of the Earth’s surface
also
causes large thermally-driven currents in the oceans.
- Students should be able to explain the occurrence of seasons and diagram
[or
analyze one] the different Earth positions corresponding to the different seasons.
5b.
Students know the
relationship
between the rotation
of 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
causes
the direction of fluid flow
to be
different in the North and South hemispheres.
- Student should be able to create a model or diagram
of
how Earth’s rotation and the Coriolis effect
can lead to the
creation of circular motions of air in pressure centers.
5d.
Students know
properties of ocean water
, such as
temperature and salinity
, can be used to explain the layered
structure of the oceans
, the generation of horizontal and
vertical ocean currents, and th
e geographic distribution of
marine organisms.
a. Students will enumerate the different properties of ocean water,
such
as temperature, salinity, density and describe how each is measured. b. Students should be able to describe how density differences
can drive
circulations in oceans
and how temperature differences can be used to
explain the layered structure
of 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 evol
ved over geologic time
and know the effect of outgassing, the variations of carbon dioxide concentration, and the origin of atmos
pheric ox
yg
en.
- 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 CO
build-up in 2
the atmosphere of today.