-
Physical Distance Represented by
Latitude and Longitude :
-
DD system
- use decimal degrees.
- In this method, each degree is divided into a base ten system
-
DMS system
- 1. is a method of dividing degrees into minutes and
- Seconds
- - A circle can be divided into 360º
- -A Degree can divided into 60 minutes (60’)
- -A minute can be divided into 60 seconds
-
Incidence of Solar Radiation on Latitudes
- Low angle of incoming sunlight (North Pole 60ºN,
- Sunlight Directly overhead(30ºN Tropic of
- Cancer, 0º Equater, Tropic of Capricorn 30ºS), Low angle of incoming
- sunlight 60º South Pole)
-
meridian
- a Line connecting all points at the same
- longitudinal angel.
-
longitude
- is an angular or arc distance east or west of a point
- on Earth’s surface measured from the center of Earth ,
-
parallel
- A line connectin all points at the same
- latitudinal angel.
-
Latitude
- – is an angular or arc distance north or south
- of the equator measured from the center of Earth.
-
Distribution of water in Earth
- 1. Earths
- water is Primarily Ocean water, Groundwater, Lakes and Fresh water(Groundwater, polar ice, other ice &
- snow, Lakes, Soil Moisture, Atmospheric Water, Marshes, Rivers and Biological
- water.)
-
Content of
Lithosphere
- 1. (Continental
- crust, Oceanic Crust & sedmentary Deposits) – it is part of the upper
- mantle & consists of the oceanic crust, continental crust, and uppermost
- mantle. Beneath the lithosphere is the asthenosphere. Sedimentary deposits are
- commonly found at the boundaries between the continental and oceaninic crust.
- The Soil layer is called the edaphosphere and generally covers Earth’s land
- surface.
-
System Equilibrium
- – when the rates of inputs and outputs in the
- system are equal and the amounts of energy and matter in storage within the
- system are constant the system is in steady- State equilibrium.
-
Which has the bad effect on nature and why
- in natural system, such unchecked positive feedback growth can reach a critical
- limit, leading to instability, disruption, or death of organisms. Global
- climate change creates an example of positive feedback. (i.e. wildfires)
-
How to identify a positive feedback
- – If Feedback information encourages increased response in the system, it is
- Positive Feedback.(like good reviews affecting ticket sales for a movie) or a
- negative feedback – The Feedback information discourages response in the
- system, (like bad reviews affecting ticket sales), Such negative causes
- self-regulation in a natural system , stabilizing the system.
-
System feedback loop
- As a system opertates, it generates outputs that influence its own operations.
- These outputs function as “information” that is returned to various points in
- the system via pathways called FEEDBACK LOOPS.
-
How to identify an open system or a close system
- ie. (Figure 1.4 Plant photosenythesis & respiration) The Photosynthesis, plants
- use sunlight as an energy input and material inputs of water nutrients, and
- carbon dioxide. The Photosynthetic process converts these inputs to stored
- chemical energy in the form of plant sugars (carbohydrates). The process also
- releases an ouput from the plant system: the oxygen we breathe.
-
Isolated system
(No exchange of energy or matter)
-
Closed system-
- Exchange of Energy but no exchange of matters
- across boundary)
-
Open system
- Exchange of Energy as well as matters across the
- boundaries)
-
System
- The Part of the universe whose properties are
- under consideration, The system is separated from the rest of the Universe,
- known as surrounding by a boundary whose properties can be defined.
-
How to calculate time on Earth
- 1. The basis of time is that Earth revolves 360º every
- 24 hours, or 15º per hour (360º + 24= 15º). Thus, a time zone of 1 hour is
- established, spanning 7.5º on either side of a central meridian.
- - Assuming it is
- 9:00 P.M. in Greenwich, then it is 4:00 P.M. in Baltimore(+5hr), 3:00 P.M. in
- Oklahoma City (+6hr), 2:00 P.M. in Salt Lake City (+7hr, 1:00P.M. in Seattle
- and Los Angles (+8hr), noon in Anchorage (+9hr), and 11:00 A.M. in Honolulu
- (+10hr).
-
International Date Line
- 1. An important corollary of the prime meridian is the
- 180º meridian on the opposite side of the planet. This meridian is the
- Ingternational Date Line and Marks the Place where each day officially
- begins(at 12:01 A.M.) From this “Line” the new day sweeps west-ward. This
- westward movement of time is created by Earth’s turning eastward on its axis.
-
Normal lapse rate
When the temperature decreases with altitude. 3.5º F/1000 ft. 6.4ºC/ 1000m
-
Transmission
refers to the passage of shortwave and longwave energy through either the atmosphere or water.
-
Scattering
Is the changing of direction of lights movement w/out altering its wavelength
-
Reflection
is a portion of energy that bounces directly back into space w/out being absorbed.
-
Refraction
is the change in speed and direction of light
-
Absorption
is the assimilation of radiation molecules of matter and its conversion from one form of energy to another.
-
Why is the Sky blue?
because the lighter blue is being scattered from the visible spectrum because it is a shorter wavelength.
-
Why are the Clouds white?
- Clouds are white because their water droplets or ice
- crystals are large enough to scatter the light of the visible spectrum which combines
- to produce white light.
-
The color of sea water is blue – Why?
- Blue wavelengths are absorbed the least by the deep ocean
- water and are scattered and reflected back to the observer’s eye.
-
False image (like mirage) due to refraction
- Refraction is the bending of a wave when it enters a medium
- where its speed is different. The refraction of light when it passes from a
- fast medium to a slow medium bends the light ray toward the normal to the
- boundary between the two media. The amount of bending depends on the indices of
- refraction of the two media (eg – Mirage is a refraction effect).
-
Albedo– reflectivity of different surfaces
- The albedo of an object is the extent to which it reflects
- light, defined as the ratio of reflected to incident electromagnetic radiation.
- It is a unitless measure indicative of a surface's or body's diffuse
- reflectivity.
-
The
greenhouse effect
- Visible energy from the sun passes through the glass and
- heats the ground. Infrared energy from the ground is partly reflected by the
- glass and some is trapped inside the greenhouse.
-
Cloud’s greenhouse forcing
- Clouds
- absorb and reradiate longwave radiation emitted by Earth; some longwave energy
- returns to space and some is radiated toward the surface.
-
Heat Transfer
- A pan of water on the stove illustrates heat transfer.
- Infrared energy radiates from the burner to the saucepan and the air. Energy
- conducts through the molecules of the pan and the handle. The water physically
- mixes, carrying heat energy by convection. The energy in the water and handle
- is measurable as sensible heat. The vapor leaving the surface of the water
- contains the latent heat absorbed in the change of water to water vapor.
-
Earth–AtmosphereRadiation Balance
- Solar energy cascades through the lower atmosphere where it
- is absorbed, reflected, and scattered. Clouds, atmosphere, and the surface
- reflect 31% of this insolation back to space. Atmospheric gases and dust and
- Earth's surface absorb energy and radiate longwave radiation. Over time, Earth
- emits, on average, 69% of incoming energy to space. When added to Earth's
- average albedo (31%, reflected energy), this equals the total energy input from
- the Sun (100%).
-
Map scale
- 1. The ratio of the image ona map to the real world; it
- realtes a unit on the map to a similar unit on the ground. A 1:1 scale means
- that a centimeter on the map represents a centimeter on the ground an
- appropriate scale for a local map is1:24,000, in which 1 unit on the map
- represents 24,000 identical units on the ground., Representative fraction
- – Cartographers express map scale as
- this; with either a colon or a slash, as in 1: 125,000 or 1/125,000.
-
position on Earth
- •
- Latitude and longitude combine to make a
- grid (geographic grid) that can be used to determine your location on Earth.
- •
- For greater precision, degrees of
- latitude and longitude are divided into 60 minutes (symbolized by '), and
- minutes are divided into 60 seconds (symbolized by ").
- •
- Maps are often marked with parallels and
- meridians. The latitude and longitude of a point are called its coordinates. If
- you know the coordinates, you can use a map to locate any point on Earth.
-
Perihelion
- Earth’s
- closest position to the Sun (Northern Hemisphere Winter January 3rd)
-
Aphelion
- 1. Earth’s farthest position to the Sun 152.083
- M km
Or 94.5 M mi (Northern Hemisphere Summer July 4)
-
wavelength
the distance between corresponding points on any two successive waves
-
frequency -
- The number of waves
- passing a fixed point in 1 second
-
composition of solar energy:
- UV, X Ray, Gamma Ray=8% ,
- Visible = 47% ,
- Infrared = 45%
-
How do we see color?
- green leaf- reflects green light and absorbs red and blue light, and the amounts of
- light reflected and absorbed are dependent upon the amount of chlorophyll in
- the leaf. ,blue ball etc)
-
Why do we see fall colors?
- 1.Daylight (white visible light) is made up of
- numerous waves or impulses each having different dimensions or wavelengths.
- When separated, any single wavelength will produce a specific color impression
- to the human eye. What we actually see as color is known as its color effect. When an object is hit
- (bombarded) with light rays, the object absorbs certain waves and reflects
- others, this determines the color effect.
-
Uneven Distribution of Insolation
- Differences in the angle of solar rays at each latitude result in an
- uneven distribution of insolation and heating.)
-
Subsolar points
- Point on earth’s surface which receives insolation perpendicular to the
- surface. During the year this point occur at lower latitude between tropic of
- Cancer and tropic of Capricorn where the energy is more concentrated.
-
other than subsolar point?
1. All other places away from the subsolar point receiveinsolation at an angle less than 900 and thus experience morediffuse energy.
-
Sun’s altitude
angle above horizon
-
Declination -
- latitude of the Subsolar point. It annually migrates through 470
- of latitude (from Tropic of Cancer to Tropic of Capricorn…Find out the angular
- and physical distance in miles,
-
Daylength -
- duration of exposure
- to insolation.
-
Effect of rotation
- The Earth rotates from west to east or eastword. This cause Sun’s
- apparent daily journey from sunrise in the east and sunset in the waste. Earth rotates on its
- axis once every 24 hours
-
Revolution
- A revolution is also called a year. The Earth takes 365.25 days to revolve around the sun. It is during this year or revolution that
- brings Earth it’s seasons,
-
Axial Tilt -
- • Tilt of
- Earth’s axis ;Axis is tilted 23.5° from plane of ecliptic, Axial
- parallelism Axis maintains alignment during orbit around the Sun North pole points toward the North Star (Polaris)
-
Circle of Illumination
- The Circle of Illumination is the boundary between
- day and night. The edge of the sunlit hemisphere, which forms a circular
- boundary separating the earth into a light half and a dark half.
-
Solstice and Equinox
- 1. Four days
- during our calendar year — two solstices and two equinoxes — mark the
- beginnings of the four seasons. At the extremes are the winter and summer
- solstices, with the vernal and autumnal equinoxes occupying the midpoints.
- The solstices and equinoxes also mark four important points in Earth's
- orbit around the Sun. It's Earth's position in its orbit — and the orientation
- of its tilted axis at these points in its orbit — that defines the seasons.
- The solstices are six months apart and mark the days when the northern
- and southern hemispheres receive either maximum (summer) or minimum (winter)
- sunshine. In the north, the summer solstice, usually around June 21, is the
- longest day of the year; the winter solstice, six months later, is the shortest
- day of the year.
- The two
- equinoxes occur roughly midway between the solstices: the autumnal equinox in
- September and spring equinox in March. At these times, day and night are
- roughly of equal length.
-
How to determine daylength
- 1. Daylength
- is the interval between sunrise and the sunset.
- It is the most obvious way of sensing change in season at latitudes away from the
- equator.
-
Heterosphere -
- 1.
- (hetero – not uniform)
– Its gases are not evenly mixed
-- outer atmosphere
- 80
- km (50 mi) outward, to thermosphere
- Layers
- of gases sorted by gravity. It is organized in layers based on the weight of
- gases.
-
Homosphere –
• (homo - uniform)
—It is an even mixture of gases, “air.”
– inner atmosphere
– Surface to 80km (50 mi)
– Gases evenly blended
-
Components of Homosphere
NITROGEN, OXYGEN, ARGON & CARBON DIOXIDE
-
The reasons of temperature change at different levels of atmosphere
- Temperature
- variations in the four layers are due to the way solar energy is absorbed as it
- moves downward through the atmosphere. The Earth’s surface is the primary absorber of
- solar energy. Some of this energy is reradiated by the Earth as heat, which warms the
- overlying troposphere. The global average temperature in the troposphere rapidly
- decreases with altitude until the tropopause, the boundary between the troposphere and
- the stratosphere. The temperature begins to increase with altitude in the stratosphere. This warming is
- caused by a form of oxygen called ozone (O3) absorbing ultraviolet radiation from the
- sun. Ozone protects us from most of the sun’s ultraviolet radiation, which can cause
- cancer, genetic mutations, and sunburn. Scientists are concerned that human activity is
- contributing to a decrease in stratospheric ozone. Nitric oxide, which is the exhaust of
- high- flying jets, and chlorofluorocarbons (CFCs), which are used as refrigerants, may
- contribute to ozone depletion. At the stratopause, the temperature stops increasing with altitude. The overlying
- mesosphere does not absorb solar radiation, so the temperature decreases with altitude.
- At the mesopause, the temperature begins to increase with altitude, and this trend
- continues in the thermosphere. Here solar radiation first hits the Earth’s atmosphere and
- heats it. Because the atmosphere is so thin, a thermometer cannot measure the
- temperature accurately and special instruments are needed.
-
Good ozone and bad ozone-
- Stratospheric
- ozone is found in the
- stratosphere, a layer of air way up in the atmosphere. The stratosphere is
- between 8 and 30 miles above the ground - too far away for you to breathe any
- of its air! The ozone in this layer of air protects plants, animals, and us by
- blocking the most harmful rays of the sun.
-
Tropospheric ozone,
- ground-level ozone) is found in the
- tropospheric, which is the layer of air closet to Earth’s surface. The
- troposphere is the air from the ground to about 8 miles up into the
- atmosphere- it’s the air we breathe.
- Ozone does not naturally occur at harmful levels in the troposphere. Our
- ground-level ozone problems are caused by human activities. Read “Hot Summer Days” to learn
- how humans cause “bad ozone”
|
|