Terminology and
definitions
The envelope of gasses surrounding the earth is bound to it
more or less permanently by the earth’s gravitational field.
As the atmosphere extends from the surface
to an indefinite height, density and pressure asymptotically approaching that
of interplanetary space.

The radius of the earth (Re)
~ 6370 km
Atmospheric density
also decreases in an
approximately exponential fashion and, if measured in
, would appear numerically to match the above diagram quite
closely. If, indeed, we assume that pressure and density decrease exponentially
with height, we can write
where the quantity H, with
dimensions of a length, is called the scale height of the atmosphere and is
approximated equal to 8.5 km for troposphere.
At this height, pressure and density are equal to 1/e (0.37) of their
sea level values. z is the height above sea level. P(0) and
are p and
at the sea level. (will derive scale height in the future. Note: don’t apply linear interpolation to
pressure and density fields)
·
Show vertical variation of pressure and density.
Note:
The equations above are strictly valid only if the atmosphere were isothermal
(constant in temperature) and dry whereas, in fact, temperature is a strong
function of height above the earth’s surface and the atmosphere is not dry.
In large measure, the
atmosphere rotates with the earth as it rotes in space such that, averaged over
the globe, there is no net motion towards the east or the west relative to the
earth’s surface. Note that, at the equator, the earth’s surface is moving
towards the east at a rate of about 1000 miles/hr.
1 mile=1609 m
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At approximately what
latitude is the earth’s surface traveling at 500 miles/hr? (60o)
= speed x cos 60o
We are at latitude 38o
N, how fast are we moving toward the east? (800 miles/hr or 1314 km/hr)
=
speed x cos38o
The
study of the phenomena of the atmosphere.
In ancient times, however, the Greeks applied the term “meteorologia”
to all heavenly phenomena. It derived from “meteoron” which meant phenomenon in
the sky. Nowadays, “meteor” is used as a term for the phenomena accompanying a
body from space, a meteoroid, in its passage through the atmosphere. A
meteorite is a meteoroid that reaches the surface.
Note: There
is no distinction between “meteorology” and “atmospheric science”, although, at
times, “meteorology” has been used to refer the aspects of the atmosphere
related to weather phenomena. This is not a universal definition.
Weather:
The
state of the atmosphere, mainly with respect to its effects on life and human
activities. Weather is normally thought of in terms of a number of weather
elements:
Temperature
Humidity
Precipitation (type,
intensity)
Cloudiness, fog (cover,
density, height, type)
Brightness
Visibility
Wind (speed, direction,
gustness)
Pressure
While
we respond directly, but to varying degrees to the first seven of these
elements, pressure is considered important because pressure patterns largely
govern atmospheric motions and the passage of storm systems. (See weather map
symbols, Appendix B of Ahrens)
Note: Explain vapor
pressure, saturation vapor pressure, and dew point here
Vapor
pressure
Saturated
air

Water vapor
evaporates so that water vapor pressure in the air increases. Eventually an
equilibrium state will be reached where
evaporation rate condensation rate
from the water =
on the water
The air is then saturated.
Dew
point
is the T to which air must be cooled at
constant pressure in order for it to become saturated with respect to a plane
surface of water.
Climate:
The long-term manifestations
of the weather. It is represented by the statistical collective of weather
conditions over a specified (long) interval of time, usually several decades
(e.g., 30 years).
Hence, climatology (a
division of meteorology) and climatic classification (division of the earth’s
climates into a system of contiguous regions- marine, Mediterranean, tropical
etc.)