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Copyright © 1996-2005 jsd
20 The Atmosphere
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If you don’t like the weather in Ithaca, just wait
a few minutes. It’ll get worse.
--- apologies to Mark Twain
20.1 Circulation Around Fronts and Low Pressure Centers
Because the earth is spinning and the air is moving, there are
significant Coriolis effects.1 You’ll
never understand how weather systems work unless you pay attention to
this.
Based on their everyday indoor experience, people think they
understand how air behaves:
-
They know that the stream of air from a fan moves in a
straight line, with no particular tendency to curve right or left.
- They know that once the fan is switched off, the airflow
won’t last very long or travel very far before being overcome by
friction.
However, when we consider the outdoor airflow patterns that Mother
Nature creates, the story changes completely. In a chunk of air that
is many miles across, a mile thick, and a mile away from the surface,
there can be airflow patterns that last for hours or days, because
there is so much more inertia and so much less friction. During these
hours or days, the earth will rotate quite a bit, so Coriolis effects
will be very important.
We are accustomed to seeing the rotation of storm systems depicted on
the evening news, but you should remember that even a chunk of air
that appears absolutely still on the weather map is rotating, because
of the rotation of the earth as a whole. Any chunk of air that
appears to rotate on the map must be rotating faster or slower
than the underlying surface. (In particular, the air in a storm
generally rotates faster, not slower.)
Note: In this chapter, I will use the § symbol to indicate words
that are correct in the northern hemisphere but which need to be
reversed in the southern hemisphere. Readers in the northern
hemisphere can ignore the § symbol.
20.1.1 Flow Around a Low
Suppose we start out in a situation where there is no wind, and where
everything is in equilibrium. We choose the rotating Earth as our
reference frame, which is a traditional and sensible choice. In this
rotating frame we observe a centrifugal field, as well as the usual
gravitational field, but the air has long ago distributed itself so
that its pressure is in equilibrium with those fields.
Then suppose the pressure is suddenly changed, so there is a region
where the pressure is lower than the aforementioned equilibrium
pressure.
In some cases the low pressure region is roughly the same size in
every direction, in which case it is called a low pressure
center (or simply a low) and is marked with a big “L” on
weather maps. In other cases, the low pressure region is quite long
and skinny, in which case it is called a trough and is marked
“trof” on the maps. See figure 20.1.
In either case, we have a pressure gradient.2 Each air parcel is subjected
to an unbalanced force due to the pressure gradient.
Initially, each air parcel moves directly inward, in the direction of
the pressure gradient, but whenever it moves it is subject to large
sideways Coriolis forces, as shown in figure figure 20.2.
Before long, the motion is almost pure counterclockwise§ circulation
around the low, as shown in figure 20.3, and this
pattern persists throughout most of the life of the low-pressure
region. If you face downwind at locations such as the one marked A,
the pressure gradient toward the left§ is just balanced by the
Coriolis force to the right§, and the wind blows in a straight line
parallel to the trough. At locations such as the one marked B, the
pressure gradient is stronger than the Coriolis force. The net force
deflects the air.
Now we must must account for friction (in addition to
the other forces just
mentioned). The direction of the frictional force will be opposite to
the direction of motion. This will reduce the circulatory velocity.
This allows the air to gradually spiral inward.
The unsophisticated idea that air should flow from a high pressure
region toward a low pressure region is only correct in the very lowest
layers of the atmosphere, where friction is dominant. If it weren’t
for friction, the low would never get filled in. At any reasonable
altitude, friction is negligible --- so the air aloft just spins
around and around the low pressure region.
The astute reader may have noticed a similarity between the air in
figure 20.2 and the bean-bag in figure 19.12. In
one case, something gets pulled inwards and increases its circulatory
motion “because” of Coriolis force, and in the other case something
gets pulled inwards and increases its circulatory motion “because”
of conservation of angular momentum. For a
bean-bag, you can analyze it either way, and get
the same answer. Also for a simple low-pressure center, you can
analyze it either way, and get the same answer. For a trough,
however, there is no convenient way to apply the conservation
argument.
In any case, please do not get the idea that the air spins around a low
partly because of conservation of angular momentum and partly because
of the Coriolis force. Those are just two ways of looking at the same
thing; they are not cumulative.
20.1.2 Fronts and Troughs
As mentioned above, whenever the wind is blowing in a more-or-less
straight line, there must low pressure on the left§ to balance the
Coriolis force to the right§ (assuming you are facing downwind).
In particular, the classic cold front wind pattern (shown
in figure 20.4) is associated with a trough, (as shown in
figure 20.5). The force generated by the low pressure is the
only thing that could set up the characteristic frontal flow pattern.
The wind shift is what defines the existence of the front. Air flows one way on one side of the
front, and the other way on the other side (as shown in
figure 20.4).
Usually the front is oriented approximately north/south, and the whole
system is being carried west-to-east by the prevailing westerlies. In
this case, we have the classic cold front scenario, as shown in
figure 20.4, figure 20.5, and figure 20.6.
Ahead of the front, warm moist air flows in from the south§. Behind
the front, the cold dry air flows in from the north§. Therefore the
temperature drops when the front passes. In between cold fronts,
there is typically a non-frontal gradual warming trend, with light
winds.
You can use wind patterns
to your advantage when you fly cross-country. If there is a
front or a pressure center near your route,
explore the winds aloft forecasts. Start by choosing a route that
keeps the low pressure to your left§. By adjusting your altitude
and/or route you can often find a substantial tailwind (or at least a
substantially decreased headwind).
Note: by ancient tradition, meteorologists name winds by the direction
from whence they come. A south wind (or
southerly wind) blows from south to north. Almost
everything else is named the other way. An aircraft on a southerly
heading is flying toward the south. Physicists and
mathematicians name all vectors by the direction toward which
they point. To avoid confusion, it is better to say “wind from the
south” rather than “south wind”.
A warm front is in many ways the same as a cold
front. It is certainly not the opposite of a cold front. In
particular, it is also a trough, and has the same cyclonic flow
pattern.
A warm front typically results when a piece of normal
cold front gets caught and spun backwards by the east-to-west
flow just north§ of a strong low pressure center, as shown
in figure 20.7. That is, near the low pressure center,
the wind circulating around the center is stronger
than the overall west-to-east drift of the whole system.
If a warm front passes a given point, a cold front
must have passed through a day or so earlier. The converse does
not hold --- cold front passage does not mean you should
expect a warm front a day or so later. More commonly, the pressure
is more-or-less equally low along most of the trough. There will
be no warm front, and the cold front will be followed by fair
weather until the next cold front.
Low pressure --- including cold fronts and warm fronts --- is
associated with bad weather for a simple reason. The low pressure was
created by an updraft that removed some of the air, carrying it up to
the stratosphere. The air cools adiabatically as it rises.
When it cools to its dew point, clouds and precipitation result. The
latent heat of condensation makes the air warmer than its
surroundings, strengthening the updraft.
Ascending air ⇒ low pressure at the surface
Ascending air ⇒ clouds
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The return flow down from the stratosphere (high pressure, very dry
descending air, and no clouds) generally occurs over a wide area, not
concentrated into any sort of front. There is no
sudden wind shift, and no sudden change in temperature. This is not
considered “significant weather” and is not marked on the charts at
all.
20.2 Pressure and Winds Aloft
Air shrinks when it gets cold. This simple idea has some important
consequences. It affects your altimeter, as will be discussed in
section 20.2.4. It also explains some basic facts about the
winds aloft, which we will discuss now.
20.2.1 Thermal Gradient Wind
Most non-pilots are not very aware of the winds aloft. Any pilot who
has every flown westbound in the winter is keenly aware of some basic
facts:
- The winds aloft tend to come from the west.
- They are much stronger in the winter.
- They get stronger and stronger as altitude increases.
A typical situation is shown in figure 20.8. In
January, the average temperature in Vero Beach, Florida,
is about 15 Centigrade (59 Fahrenheit), while the average temperature
in Oshkosh, Wisconsin is about minus 10 Centigrade (14
Fahrenheit). Imagine a day where surface winds are very weak, and the
sea-level barometric pressure is the same everywhere, namely 1013
millibars (29.92 inches of mercury).
The pressure above Vero Beach will decrease with
altitude. According to the International Standard Atmosphere
(ISA), we expect the pressure to be 697 millibars at 10,000 feet.
Of course the pressure above Oshkosh will decrease
with altitude, too, but it will not exactly follow the ISA, because
the air is 25 centigrade colder than standard. Air shrinks when
it gets cold. In the figure, I have drawn a stack of ten boxes
at each site. Each box at VRB contains the same number of air
molecules as the corresponding box at OSH.3 The pile of boxes is shorter at OSH than it is at VRB.
The fact that the OSH air column has shrunk (while
the VRB air column has not) produces a big effect on the winds
aloft. As we mentioned above, the pressure at VRB is 697 millibars
at 10,000 feet. In contrast, the pressure at OSH is 672 millibars
at the same altitude --- a difference of 25 millibars.
This puts a huge force on the air. This force produces a motion,
namely a wind of 28 knots out of the west. (Once again, the Coriolis
effect is at work: during most of the life of this pressure pattern,
the wind flows from west to east, producing a Coriolis force toward
the south, which just balances the pressure-gradient force toward the
north.) This is the average wind at 10,000 feet, everywhere between
VRB and OSH.
More generally, suppose surface pressures are reasonably uniform
(which usually the case) and temperatures are not uniform (which is
usually the case, especially in winter). If you have low temperature
on your left§ and high temperature on your right§, you will have a
tailwind aloft. The higher you go, the stronger the wind. This is
called thermal gradient wind.
The wind speed will be proportional to the temperature
gradient. Above a large airmass with uniform temperature, there
will be no thermal gradient wind. But if there is a front between
a warm airmass and a cold airmass, there will be a large temperature
change over a short distance, and this can lead to truly enormous
winds aloft.
In July, OSH warms up considerably, to about 20 centigrade,
while VRB only warms up slightly, to about 25 centigrade. This
is why the thermal gradient winds are typically much weaker in
summer than in winter --- only about 5 knots on the average at
10,000 feet.
In reality, the temperature change from Florida to
Wisconsin does not occur perfectly smoothly; there may be large
regions of relatively uniform temperature separated by rather
abrupt temperature gradients --- cold fronts or warm fronts. Above
the uniform regions the thermal gradient winds will be weak, while
above the fronts they will be much stronger.
For simplicity, the foregoing discussion assumed the sea-level
pressure was the same everywhere. It also assumed that the
temperature profile above any given point was determined by the
surface temperature and the “standard atmosphere” lapse rate.
You don’t need to worry about such details; as a pilot you don’t need to
calculate your own winds-aloft forecasts. The purpose here is to make
the official forecasts less surprising, less confusing, and easier to
remember.
Several different notions of “altitude” are used in aviation.
We start with true altitude, which is the simplest. This is
what non-pilots think of as “the” altitude or elevation, namely
height above sea level, as measured with an accurate ruler. True
altitude is labelled MSL (referring to Mean Sea Level). For instance,
when they say that the elevation of Aspen is 7820 feet MSL, that is a
true altitude.
Before proceeding, we need to introduce the notion of
international standard atmosphere (ISA). The ISA is a set of
formulas that define a certain temperature and pressure as a function
of altitude. For example, at zero altitude, the ISA temperature is 15
degrees centigrade, and the ISA pressure is 1013.25 millibars, or
equivalently 29.92126 inches of mercury. As the altitude increases,
the ISA temperature decreases at a rate of 6.5 degrees centigrade per
kilometer, or very nearly 2 degrees C per thousand feet. The pressure
at 18,000 feet is very nearly half of the sea-level pressure, and the
pressure at 36,000 feet is somewhat less than one quarter of the
sea-level pressure -- so you can see the pressure is falling off
slightly faster than exponentially. If you want additional details on
this, a good place to look is the Aviation Formulary web site.
Remember, the ISA is an imaginary, mathematical construction.
However, the formulas were chosen so that the ISA is fairly close to
the average properties of the real atmosphere.
Now we can define the notion of pressure altitude. This is not
really an altitude; it is just a way of describing pressure.
Specifically, you measure the pressure, and then figure out how high
you would have to go in the international standard atmosphere to
find that pressure. That height is called the pressure altitude.
One tricky thing is that low pressure corresponds to high pressure
altitude and vice versa.
Pressure altitude (i.e. pressure) is worth knowing for several
reasons. For one thing, if the pressure altitude is too high, you
will have trouble breathing. The regulations on oxygen usage are
expressed in terms of pressure altitude. Also, engine performance is
sensitive to pressure altitude (among other factors). Thirdly, at
high altitudes, pressure altitude is used for vertical separation of
air traffic. This works fine, even though the pressure altitude may
be significantly different from the true altitude (because on any
given day, the actual atmosphere may be different from the ISA). The
point is that two aircraft at the same pressure level will be at the
same altitude, and two aircraft with “enough” difference in pressure
altitude will have “enough” difference in true altitude.
To determine your pressure altitude, set the Kollsman window on your
altimeter to the standard value: 29.92 inches, or equivalently 1013
millibars. Then the reading on the instrument will be the pressure
altitude (plus or minus nonidealities, as discussed in
section 20.2.3).
This brings us to the subject of calibrated altitude and
indicated altitude. At low altitudes -- when we need to worry
about obstacle clearance, not just traffic separation --
pressure altitude is not good enough, because the pressure at any
given true altitude varies with the weather. The solution is to use
indicated altitude, which is based on pressure (which is convenient to
measure), but with most of the weather-dependence factored out. To
determine your indicated altitude, obtain a so-called altimeter
setting from an appropriate nearby weather-reporting station, and
dial it into the Kollsman window on your altimeter. Then the reading
on the instrument will be the indicated altitude. (Calibrated
altitude is the same thing, but does not include nonidealities,
whereas indicated altitude is disturbed by nonidealities of the sort
discussed in section 20.2.3.)
The altimeter setting is arranged so that right at the reporting
station, calibrated altitude agrees exactly with the station
elevation. By extension, if you are reasonably close to the station,
your calibrated altitude should be a reasonable estimate of your true
altitude ... although not necessarily good enough, as discussed in
section 20.2.3 and section 20.2.4).
Next we turn to the notion of absolute altitude. This is
defined to be the height above the surface of the earth. Here is a
useful mnemonic for keeping the names straight: the Absolute
Altitude is what you see on the rAdAr altimeter.
Absolute altitude is labelled “AGL” (above ground level). It is
much less useful than you might have guessed. One major problem is
that there may be trees and structures that stick up above the surface
of the earth, and absolute altitude does not account for them.
Another problem is that the surface of the earth is uneven, and if you
tried to maintain a constant absolute altitude, it might require wild
changes in your true altitude, which would play havoc with your energy
budget. Therefore the usual practice in general aviation is to figure
out a suitable indicated altitude and stick to it.
Another type of altitude is altitude above field elevation,
where field means airfield, i.e. airport. This is similar to absolute
altitude, but much more widely used. For instance, the
traffic-pattern altitude might be specified as 1000 feet above field
elevation. Also, weather reports give the ceiling in terms of
height above field elevation. This is definitely not the same as
absolute altitude, because if there are hills near the field, 1000
feet above the field might be zero feet above the terrain. Altitude
above field elevation should be labelled “AFE” but much more
commonly it is labelled “AGL”. If the terrain is hilly “AGL” is
a serious misnomer.
Finally we come to the notion of density altitude. This is not
really an altitude; it is just a way of describing density. The
official definition works like this: you measure the density, and then
figure out how high you would have to go in the ISA to find that
density. That height is called the density altitude. Beware
that low density corresponds to high density altitude and
vice versa.
Operationally, you can get a decent estimate of the density altitude
by measuring the pressure altitude and temperature, and then
calculating the density altitude using the graphs or tables in your
POH. This is only an estimate, because it doesn’t account for
humidity, but it is close enough for most purposes.
Density altitude is worth knowing for several reasons. For one thing,
the TAS/CAS relationship is determined by density. Secondly, engine
performance depends strongly on density (as well as pressure and other
factors). Obviously TAS and engine performance are relevant to every
phase of flight -- sometimes critically important.
20.2.3 Altimeter Errors
As discussed in the previous section, an aircraft altimeter does not
measure true altitude. It really measures pressure, which is
related to altitude, but it’s not quite the same thing.
In order to estimate the true altitude, the altimeter depends two
factors: the pressure, and the altimeter setting in the Kollsman
window. The altimeter setting is needed to correct for local
variations in barometric pressure. You should set this on the runway
before takeoff, and for extended flights you should get updated
settings via radio. If you neglect this, you could find yourself at a
too-low altitude, if you fly to a region where the barometric pressure
is lower. The mnemonic is: “High to low, look out below”.
Altimeters are not perfect. Even if the altimeter
and airplane were inspected yesterday, and found to be within tolerances,
-
The altimeter could be off by 30 feet when it reads
2500 (according to the tolerances in FAR 43 Appendix E).
- If the airplane is moving at 100 knots, the indicated
altitude could be
off by another 30 feet, due to nonidealities in the arrangement of
the static port (FAR 23.1325).
- If the airplane is descending at 750 FPM, the altimeter could
be off by an additional 70 feet, due to friction in the mechanism
(FAR 43 Appendix E).
- There could be 30 feet of hysteresis, if you have recently
descended from a very high altitude (FAR 43 Appendix E).
- Wind flowing over a nice airfoil-shaped hill can produce low
pressure there. A 35-knot wind could produce a 50-foot altimetry error. See
section 3.4.1.
The first item could be off in either direction, but the other items
will almost certainly be off in the bad direction when you are
descending. Also, if the airplane has been in service for a few
months since the last inspection, the calibration could have drifted a
bit. All in all, it would be perfectly plausible to find that your
altimeter was off by 50 feet when parked on the ground, and off by 200
feet in descending flight over hilly terrain.
20.2.4 High Altimeter due to Low Temperature
The altimeter measures a pressure and converts it to a so-called
altitude. The conversion is based on the assumption that the actual
atmospheric pressure varies with altitude the same way the the
standard atmosphere would. The pressure decreases by roughly 3.5%
per thousand feet, more or less, depending on temperature.
The problem is that the instrument does not account for nonstandard
temperature. Therefore if you set the altimeter to indicate correctly
on the runway at a cold place, it will be inaccurate in flight. It
will indicate that you are higher than you really are. This could get
you into trouble if you are relying on the altimeter for terrain
clearance. The mnemonic is HALT --- High Altimeter because of Low
Temperature.
As an example: Suppose you are flying an instrument approach into
Saranac Lake, NY, according to the FAA-approved “Localizer Runway 23”
procedure. The airport elevation is 1663 feet. You obtain an
altimeter setting from the airport by radio, since you want your
altimeter to be as accurate as possible when you reach the runway.
You also learn that the surface temperature is -32 Centigrade, which
is rather cold but not unheard-of at this location. That means the
atmosphere is about 45 C colder than the standard atmosphere. That in
turn means the air has shrunk by about 16%. Throughout the approach,
you will be too low by an amount that is 16% of your height above the
airport.
The procedure calls for crossing the outer marker at 3600 MSL and then
descending to 2820 MSL, which is the Minimum Descent Altitude. That
means that on final approach, you are supposed to be 1157 feet
above the airport. If you blindly trust your altimeter, you will be
1157 “shrunken feet” above the airport, which is only about 980 real
feet. You will be 180 real feet (210 shrunken feet) lower than you
think. To put that number in perspective, remember that localizer
approaches are designed to provide only 250 feet of obstacle
clearance.4
You must combine this HALT error with the ordinary altimetry errors
discussed in section 20.2.3. The combination means you could be
400 feet lower than what the altimeter indicates --- well below the
protected airspace. You could hit the trees on Blue Hill, 3.9 nm
northeast of the airport.
Indeed, you may be wondering why there haven’t been lots of crashes
already -- especially since the Minimum Descent Altitude used to be
lower (1117 feet, until mid-year 2001). Possible explanations
include:
-
Most people use the ILS approach instead of the localizer
approach. That provides electronic vertical guidance that isn’t
affected by temperature.
- In winter, the real atmosphere usually has a
smaller lapse rate than the standard atmosphere, especially at the
lower altitudes, so the errors are usually less than what
simple theory would suggest.
- The FAA has overestimated the height of the trees. They
routinely assume there will be small structures and trees rising 200
feet above the land surface, but the trees on Blue Hill are probably
closer to 100 feet. This is helpful, but we shouldn’t rely on it.
The trees are still growing, and other trees in the vicinity are over
150 feet tall. Furthermore, if somebody built a 190-foot
tower atop Blue Hill, the FAA would not change the Minimum Descent
Altitude for this procedure, and there would be problems for sure.
- The new 1157-foot Minimum Descent Altitude is about 40 feet
higher than what you would expect just based on the height of the
hill. I’m told this represents an allowance for the effect of wind
blowing over hilly terrain as mentioned above.
Even if people don’t “usually” crash, we still need to do something
to increase the margin for error.
There is an obvious way to improve the situation: In cold weather, you
need to apply temperature compensation to all critical
obstacle-clearance altitudes.
You can do an approximate calculation in your head: If it’s cold, add
10%. If it’s really, really cold, add 20%. Approximate
compensation is a whole lot better than no compensation.
The percentages here are applied to the height above the field,
or, more precisely, to the height above the facility that is giving you
your altimeter setting. In the present example, 20% of 1157 is about
230. Add that to 2820 to get 3050, which is the number you want to
see on your altimeter during final approach. Note that this number,
3050, represents a peculiar mixture: 1663 real feet plus 1387 shrunken
feet.
For better accuracy, you can use the following equation. The
indicated altitude you want to see is:
In this formula, F is the facility elevation, Ar is the true
altitude you want to fly (so Ar-F is the height above the facility,
in real feet), λ is the standard lapse rate (2 °C per thousand feet), Tf is the temperature at
the facility, 273.15 is the conversion from Centigrade to absolute
temperature (Kelvin), and 15 C = 288.15 K is the sea-level temperature
of the standard atmosphere. The denominator (273.15 + Tf) is the
absolute temperature observed at the facility, while the numerator
(288.15-λ F) is what the absolute temperature would be in
standard conditions.
You might want to pre-compute this for a range of temperatures,
and tabulate the results. An example is shown in
table 20.1. Make a row for each of the critical
altitudes, not just the Minimum Descent Altitude. Then, for each
flight, find the column that applies to the current conditions and
pencil-in each number where it belongs on the approach plate.
| Facility Temp, °C |
12 |
0 |
-10 |
-20 |
-30 |
-40 |
| South Sector |
6600 |
6820 |
7000 |
7220 |
7440 |
7700 |
| Northeast Sector |
5100 |
5240 |
5380 |
5540 |
5680 |
5860 |
| Northwest Sector |
4100 |
4200 |
4300 |
4400 |
4520 |
4640 |
| Procedure Turn |
4800 |
4940 |
5060 |
5200 |
5340 |
5500 |
| Crossing Outer Marker |
3600 |
3680 |
3760 |
3840 |
3940 |
4020 |
| Minimum Descent Alt |
2820 |
2860 |
2920 |
2960 |
3020 |
3080 |
Table 20.1: Saranac Lake Critical Altimeter Readings
It is dangerously easy to get complacent about the temperature
compensation. You could live in New Jersey for years without needing
to think about it -- but then you could fly to Saranac Lake in a
couple of hours, and get a nasty surprise.
The HALT corrrection is important whenever temperatures are below
standard and your height above the terrain is a small fraction of your
height above the facility that gave you your altimeter setting. This
can happen enroute or on approach: -
When flying over tall mountains, you might need to apply a
great deal of compensation; 11,000 shrunken feet might not be enough
to get you over a 10,000-foot mountain.
- When flying a localizer approach where the minimum descent
altitude is 1000 feet above the facility, you might need to apply more
than 100 feet of compensation. This might make the difference between
crashing and not crashing.
If it’s cold, add 10%.
If it’s really, really cold, add 20%.
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20.3 Prevailing Winds and Seasonal Winds
A parcel of air will have less density if it has
- a higher temperature,
- a higher dewpoint, and/or
- a lower pressure.
If a parcel of air is less dense than the surrounding
air, it will be subject to an upward force.5
20.3.1 Primary Circulation Patterns
As everyone knows, the tropics are hotter and more humid than
the polar regions. Therefore there tends to be permanently rising air
at the equator, and permanently sinking air at each
pole.6 This explains why equatorial regions are
known for having a great deal of cloudy, rainy weather, and why the
polar regions have remarkably clear skies.
You might think that the air would rise at the equator, travel to the
poles at high altitude, descend at the poles, and travel back to the
equator at low altitude. The actual situation is a bit more
complicated, more like what is shown in figure 20.9. In each
hemisphere, there are actually three giant cells of circulation.
Roughly speaking, there is rising air at the equator, descending air
at 25 degrees latitude, rising air at 55 degrees latitude, and
descending air at the poles. This helps explain why there are great
deserts near latitude 25 degrees in several parts of the world.
The three cells are named as follows: the Hadley cell (after
the person who first surmised that such things existed, way back in
1735), the Ferrel cell, and the polar cell. The whole
picture is called the tricellular theory or tricellular
model. It correctly describes some interesting features of the
real-world situation, but there are other features that it does not
describe correctly, so it shouldn’t be taken overly-seriously.
You may be wondering why there are three cells in each hemisphere, as
opposed to one, or five, or some other number. The answer has to do
with the size of the earth (24,000 miles in circumference), its speed
of rotation, the thickness of the atmosphere (a few miles), the
viscosity of the air, the brightness of the sun, and so forth. I
don’t know how to prove that three is the right answer --- so let’s
just take it as an observed fact.
Low pressure near 55 degrees coupled with high pressure near 25
degrees creates a force pushing the air towards the north§ in the
temperate regions. This force is mostly balanced by the Coriolis
force associated with motion in the perpendicular direction, namely
from west to east. As shown in figure 20.10, these are the
prevailing westerlies that are familiar to people who live in
these areas.
According to the same logic, low pressure near the equator coupled
with high pressure near 25 degrees creates a force toward the equator.
This force is mostly balanced by the Coriolis force associated with
motion from east to west. These are the famous trade winds,
which are typically found at low latitudes in each hemisphere, as
shown in figure 20.10.
In days of old, sailing-ship captains would use the
trade winds to travel in one direction and use the prevailing
westerlies to travel in the other direction. The regions in between,
where there was sunny weather but no prevailing wind, were named
the horse latitudes. The region near the equator where
there was cloudy weather and no prevailing wind was called the
doldrums.
The boundaries of these great circulatory cells move with the sun.
That is, they are found in more northerly positions in July and in
more southerly positions in January. In certain locales, this can
produce a tremendous seasonal shift in the prevailing wind, which is
called a monsoon.7
20.3.2 Continental / Oceanic Patterns
Now let us add a couple more facts:
-
The sun
is not very effective at heating the air,
especially dry air. Normally, the sun heats the surface of the
planet, then the air gains heat from the surface --- partly by simple
contact, and partly by absorbing energy-rich water vapor that
evaporates from the surface.
- When we change from winter to summer, solar heating
warms the dry land much more quickly than the ocean.8 This is because the ocean is constantly being stirred. To
heat up the land, you need only heat up the top few inches of soil.
To heat up the ocean, you need to heat up several feet of water.
As a consequence, in temperate latitudes, we find that in summer, the
land is hotter than the ocean (other things, such as latitude,
being constant), whereas in winter the land is colder than the
ocean.
This dissimilar heating of land and water creates huge areas of low
pressure, rising air, and cyclonic flow over the oceans in
winter, along with a huge area of high pressure and descending air
over Siberia. Conversely there are huge areas of high pressure,
descending air, and anticyclonic flow over the oceans in summer.
These continental / oceanic patterns are superimposed
on the primary circulation patterns. In some parts of the world,
one or the other is dominant. In other parts of the world, there
is a day-by-day struggle between them.
Very near the surface (where friction dominates),
air flows from high pressure to low pressure, just as water flows
downhill. Meanwhile, in the other 99% of the atmosphere (where
Coriolis effects dominate) the motion tends to be perpendicular
to the applied force. The air flows clockwise§ around a high
pressure center and counterclockwise§ around a low pressure center,
cold front, or warm front.
Although trying to figure out all the details of the atmosphere from
first principles is definitely not worth the trouble, it is comforting
to know that the main features of the wind patterns make sense. They
do not arise by magic; they arise as consequences of ordinary physical
processes like thermal expansion and the Coriolis effect.
If you really want to know what the winds are doing at
10,000 feet, get the latest 700 millibar constant pressure
analysis chart and have a look. These charts used to be nearly
impossible for general-aviation pilots to obtain, but the situation is
improving. Now you can get them by computer network or fax. On a
trip of any length, this is well worth the trouble when you think of
the time and fuel you can save by finding a good tailwind.
A few rules of thumb: eastbound in the winter, fly high. Westbound in
the winter, fly lower. In the summer, it doesn’t matter nearly as
much. In general, try to keep low pressure to your left§ and high
pressure to your right§.
- 1
- The origin of
the Coriolis effect is discussed in section 19.3.
- 2
- In
general, a gradient has to do with how steeply
something changes from place to place.
- 3
- The
bottom box starts at sea level at both sites. We ignore the fact
that OSH is actually 808 feet above sea level. The fact that
the ground “sticks up” into the bottom box doesn’t change
the essence of the argument. This is consistent with the notion
that you adjust your altimeter to read 808 (not zero) on the ground
at OSH.
- 4
- The idea to get you down as low as possible, to
maximize your ability to get below the cloud ceiling so you can find
the airport in bad weather.
- 5
- It
would be simpler, but less accurate, to say “hot air rises”.
For one thing, if all the air is hot, none of it will rise.
Secondly, it is important to keep in mind that an upward force
is not necessarily the same as upward motion.
- 6
- Although there is, as expected, somewhat low pressure
at the equator (and very low density, when you take humidity into
account), there is not any noticeable high pressure at the poles. In
fact, there is phenomenally low pressure at the south pole. I have no
idea why this is. Sorry.
- 7
- The word “monsoon” comes from an
Arabic word meaning “season”, hence “seasonal wind”. In
southern Arizona the word is properly used to describe the seasonal
wind that brings rain in July. The rain is not very heavy but
contrasts with rainless June. On the west coast of India, in one
season the wind comes from the ocean, bringing torrential rainfall.
The word properly refers to any seasonal wind, not just the rainy
season, and not necessarily heavy rain. Non-experts commonly use the
word “monsoon” as shorthand for “monsoon rains” or even
“torrential rain” but that’s not recommended.
- 8
- A
similar thing happens, on a smaller scale, when we change from night
to day.
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