Weather & Climate: Introductory Principles & Exercises
Lead Author(s): Marius Paulikas
Student Price: $49.00
Introductory atmospheric concepts are examined, which include earth-sun relationships, wind dynamics, and precipitation development
CHAPTER 1: INTRODUCTION TO THE ATMOSPHERE
The first chapter addresses the general structure of the atmosphere, and discusses atmospheric principles as they relate to pressure and density. In this chapter, you will also learn about the different gases occupying the earth’s atmosphere, and you will be provided with an overview of the earth's atmospheric layers that are defined by temperature properties.
Section 1: Atmospheric Pressure and Density
The earth’s atmosphere may be regarded as a collection of gases, solids, and liquids which comprise the space located above its ground level. Most of the earth's atmosphere is found near its surface due to the earth's gravitational pull, and the atmosphere rapidly decreases as one ascends with height. While an upper ‘ceiling’ of the earth’s atmosphere does not exist, the atmosphere eventually ‘blends’ into outer space at approximately 100 kilometers (km) above ground.
Two metrics utilized to measure the earth’s atmosphere are atmospheric pressure and density. Pressure is defined as the force exerted on a given area, and may be simply regarded as the ‘weight’ of the atmosphere at a given location. Density refers to the amount of matter (for our purposes, the amount of gas molecules) present within a given unit of space (or volume of air). Because most of the earth’s atmosphere is confined at the lowest altitudes, the density of the earth’s atmosphere is likewise greatest near the mean sea level (or the average ocean height level). Atmospheric density and pressure are directly proportional to each other; if we have more gas molecules present within a given air sample, the air will weigh more and exert a greater force as a result. As atmospheric pressure decreases with height, so does air density.
Atmospheric pressure may be measured in multiple ways (i.e., inches of mercury, pounds per square inch, atmospheres). Meteorologists (or atmospheric scientists) commonly express pressure in millibars (mb). The standard pressure reading at the mean sea level is 1013.25 mb, although for our purposes, it is sufficient to say that sea level pressure values are typically within 50 mb of 1000 mb.
The first set of exercises identifies the general rule of thumb that for every 5.6 kilometers one advances above the earth's surface, both atmospheric pressure and density decrease by approximately 50%, or one-half. In Table 1 below, we begin with the average atmospheric pressure value of 1000 mb at the mean sea level height, and, following the "50% reduction rule," the pressure value is reduced to 500 mb at 5.6 km above the mean sea level.
Make a sketch of the table below and fill the remaining millibar values using the 50% (or one-half) reduction rule from the 11.2 km to the 39.2 km altitude levels. Then, use the values in Table 1 to answer Questions 1-3 below:
Use the values from Table 1 to answer Questions 1-3 below:
What would be the approximate barometric pressure value at 16.8 km?
What would be the approximate barometric pressure value at 39.2 km?
By approximately how much does atmospheric pressure decrease from the mean sea level to the 39.2 km altitude level?
applying the 50% reduction rule, we can take the same approach in
estimating the percentage of the earth’s atmosphere that lies within every 5.6 km
increment of altitude. If, for instance,
the earth’s atmospheric pressure value decreases in half from 1000 to 500 mb from
the mean sea level to the 5.6 km altitude level, this is reflective that 50% of
the earth’s atmospheric gases will be found within this first 5.6 km
increment. As we increase our altitude
to 11.2 km above ground, the remaining 50% of the earth’s atmosphere will be
halved again, and this results in 25% of the earth’s atmosphere being located within
this next increment of height. This is
illustrated in Table 2 below.
Make a sketch of the table below and fill in the remaining values to identify what percentage of the atmosphere lies within every 5.6-km height increment up to the 39.2 km level:
Use the values from Table 2 to answer Questions 4-6 below:
Below the 16.8 km level (all the way to the ground), [?] % of the total atmosphere would be found.
From the 28.0 km altitude level, approximately how much of the Earth's total atmosphere would be located ABOVE you? (Note: This would include altitudes above the 39.2 km level).
Upon reaching the 39.2 km altitude level, approximately how much of the total atmosphere is now below you?
If you successfully answered these first six questions, you'll see that the earth's atmospheric gases certainly decrease very rapidly with height! It is for this reason that airplanes cannot fly beyond a certain altitude, and why humans would not survive if directly exposed to conditions not far from the earth's surface.
Section 2: Permanent and Variable Gases
The earth is approximately 4.5 billion years old, and the concentrations of gases that have populated its atmosphere over this time have varied greatly. Atmospheric nitrogen and carbon dioxide concentrations gradually built up due to volcanic eruptions that have occurred throughout the earth's history. Water Vapor emissions from volcanic eruptions are also believed to have contributed to the current global water supply, much of which resides in the world’s oceans. The build-up of oxygen in the earth’s atmosphere began when primitive plant life first appeared, and began ingesting carbon dioxide, water, and solar energy through the process of photosynthesis. Through photosynthesis, plants produce their own food and also release oxygen. Over billions of years, photosynthesis led to the build-up of atmospheric oxygen which we now breathe on a daily basis!
Today, the earth’s atmosphere may be separated into permanent gases and variable gases. Permanent gases consist of gases that are constant in atmospheric concentration levels, regardless of location. Nitrogen and oxygen, which are the two most common permanent gases, comprise the same fraction of the earth’s atmospheric gas concentrations regardless of location. Variable gases, as the term suggests, fluctuate in atmospheric concentration levels from one location to another. This fluctuation may be the result of surface landscape attributes (i.e., terrain), long-term climate conditions, or both. The concentrations of both permanent and variable gases are shown in Table 3 below:
Given the values shown in Table 3 above, [?] is the most abundant permanent gas while [?] is the most abundant variable gas in some locations.
Oxygen, Carbon Dioxide
Oxygen, Water Vapor
Nitrogen, Water Vapor
Nitrogen, Carbon Dioxide
Atmospheric water vapor content for a given region is largely influenced by long-term temperature conditions and surface landscape attributes. Air temperature has a direct impact on how much water may evaporate, or transition, from a liquid to a vapor state. We will see in the next section that warmer air carries greater amounts of energy, on average, than cooler air. When water is exposed to warmer air (as opposed to cooler air), larger numbers of water molecules acquire energy to evaporate. The greatest evaporation rates therefore occur in warm environments over the world's oceans. The warmest conditions on Earth are found near the Equator, or the approximate mid-point between the North and South Poles. Within the Equatorial region, ocean waters typically have higher mean sea level temperatures, and this is illustrated in Fig. 1 below:
Which of the following is the likeliest location for atmospheric water vapor content to be near 4% concentration levels?
The Sahara Desert
The lower Atlantic Ocean near the Caribbean Islands
The North Pole
The northern Pacific Ocean near Alaska
number of variable gases (water vapor, carbon dioxide, methane) are also
considered greenhouse gases, or gases that have the ability to absorb outgoing
radiative energy from the earth. This absorption of energy then causes a warming effect in the earth’s
atmosphere. Without this dynamic known
as the “Greenhouse Effect”, the Earth would drastically cool and life as we know it would not
be sustainable. Since the dawn of the
Industrial Revolution, however, atmospheric greenhouse gas concentrations have
been steadily increasing. Fig. 2 is an
image of atmospheric carbon dioxide (CO2) concentrations that have been measured at the
Mauna Loa Observatory (Mauna Loa, Hawaii) at 3,397 meters above sea
level since 1958. The red line is
indicative of running carbon dioxide data, and the black line is indicative of
seasonally corrected data (the overall trend for a given year). You will note that atmospheric carbon dioxide levels vary within a given year (the reason for this is explored in question 9), although concentrations over the five-decade period have steadily increased overall.
What would account for the seasonal variations (the red line) of atmospheric carbon dioxide concentrations displayed in Fig. 2 above? (Hint: Photosynthesis plays a key role).
Seasonal variations in vegetation or plant flourishment
Seasonal variations of urban industrial activity
Seasonal temperature swings of a given year
Seasonal variations in atmospheric pressure
Parts per million (or ‘ppm,’ as labeled in the y-axis of Fig. 2 above), is the mathematical equivalent of dividing a given value by one million, and then multiplying the result with 100%. For instance, 5 ppm is the equivalent of the following mathematical formula:
In the above example, the answer of 5.0 x 10-4 is an expression requiring the decimal next to the '5' digit to be moved four places to the left. This gives us an answer of 0.0005, and the two answers are therefore equal.
When measurements were first taken at the Mauna Loa Observatory in 1958, the overall atmospheric concentration of carbon dioxide was estimated at 315.28 ppm. What is the equivalent expression of 315.28 ppm?
By December 2016, atmospheric carbon dioxide concentrations at the Mauna Loa Observatory were measured at 404.48 ppm. What is the equivalent expression of 404.48 ppm?
We can also calculate the percentage increase in carbon dioxide concentrations observed at Mauna Loa between 1958 and 2016. To calculate the overall percentage increase, we use the following formula:
In the first step of our formula, we find the difference in ppm values between 1958 and 2016 and take the absolute value of our answer (this is represented by the vertical bars in the first step of the formula). Therefore, if the difference in our values is a negative number, we retain the numerical value and make this value positive. In the second step, we take this absolute value and divide it by our 1958 ppm value. We lastly take this resulting value and multiply it by 100%.
Given that 315.28 ppm of carbon dioxide was observed at Mauna Loa in 1958 and 404.48 ppm of carbon dioxide was observed in 2016, what is the overall percentage increase in atmospheric CO2 concentrations over this time frame?
As indicated in Table 3, some of the other important variable gases found in the atmosphere include methane and ozone. Methane concentrations, like carbon dioxide, have also been increasing in the earth's atmosphere due to anthropogenic industrialization. Atmospheric ozone concentrations, however, vary based on one's location from the Equator. Ozone consists of three atoms (or units) of oxygen, and is produced from solar radiation interactions. The greatest concentrations of atmospheric ozone typically lie approximately 25-30 km into the atmosphere. Most of the earth's atmospheric ozone is created near the Equator where the Earth receives its greatest solar concentrations, although global planetary circulations transport much of the ozone towards planetary locations found closer to the Poles. The Poles, meanwhile, correspond to where atmospheric ozone levels are significantly lower. In 1985, a large ozone "hole" was discovered over Antarctica, which resulted in a ban for a number of household products that release CFCs (cholorfluorocarbons), or gas compounds that can destroy ozone.
Based on surface landscape attributes, which of the following would likely result in greatest atmospheric concentrations of methane?
There are some locations around the globe which experience 24 hours of darkness for weeks at a time. Would this result in GREATER or LESSER atmospheric ozone concentrations?
Section 3: The Four Layers of the Atmosphere
Fig. 3 is a visual of the four layers comprising the earth’s atmosphere, which consists of the Troposphere, Stratosphere, Mesosphere, and Thermosphere. These atmospheric layers are identified based on their temperature properties, which is represented by the yellow line in Fig. 3 below. Temperature is the average kinetic energy, or energy of motion, possessed by the atoms and molecules that comprise a substance. In other words, if the air temperature is measured at 25°C (77°F), this reflects the average amount of movement energy emitted by atoms and molecules comprising the air sample. A higher air temperature (i.e. 30°C) reflects faster atomic and molecular motion, and it therefore reflects a higher mean kinetic energy content of the air.
Most of the world's weather occurs in the Troposphere, or the lowest layer of the atmosphere. This is also the layer of the atmosphere as to where most of the world's atmospheric gases are found (remember the 5.6 km rule discussed in Section 1). As one increases with altitude into the atmosphere, the temperatures of atmospheric gases found in each layer will vary. Within the Troposphere, most of the sun's heating occurs near the earth's surface, and this is why temperatures initially decrease with height. This is illustrated by the yellow line shown in Fig. 3 above. Note in Fig. 3 the average temperature values listed along the x-axis and the height values listed along the y-axis.
When viewing Fig. 3 above, which atmospheric layer consists of the hottest gases found in the Earth's atmosphere?
Based on the information provided to you at the end of Section 2 in this chapter, which atmospheric layer is where one would find an Ozone maximum (or the Ozone Layer)?
define the rate of change in temperature relative to the change in atmospheric height as a lapse rate. If, for instance, the temperature decreases
by 10 degrees Celsius over a 2 km distance in height, the lapse rate would be
calculated as (10 degrees Celsius / 2 km), or a lapse rate of 5 degrees
Celsius km-1 (note that although temperatures decrease over this distance, lapse rate values are positive). When viewing the temperature profile of the atmosphere in Fig. 3, note the orientation of the temperature line for each atmospheric layer. For some atmospheric layers, we see a decrease in temperature with height, but for others, we actually see an increase in temperature with height. A warming of the atmosphere that occurs with increasing altitude is referred to as an inversion.
Given the orientation of the yellow line graph with respect to the temperature values listed along the x-axis in Fig. 3, which atmospheric layers consist of a temperature INVERSION? Select ALL that apply:
To calculate a lapse rate, use the following equation:
You must first subtract the difference of two provided temperature values (make sure you subtract the final value from the initial value, and note that we are NOT taking the absolute value this time). The second and final step consists of taking the difference and dividing it by a vertical distance of the atmosphere.
Starting at the Troposphere, the average sea level temperature is approximately 15° C, but it drops to approximately -55° C at the Tropopause (the upper limit of the Troposphere). The location of the Tropopause varies depending on the long-term temperature conditions for a given region, but we will assume for Question 18 that the Tropopause is located approximately 11 km above sea level.
What is the approximate lapse rate of the Troposphere as a whole?
6.5 degrees C / km
0.15 km / 1 degree C
-6.5 degrees C / km
102 degrees C / km
The Stratosphere is where one finds the Ozone Layer, or a layer of gases which protects us from harmful ultraviolet solar radiation. The Ozone Layer absorbs this harmful radiation, which results in higher temperatures for atmospheric gases found within this second atmospheric layer. Due to the presence of ozone, the approximate temperature in the lower Stratosphere is -51°C, whereas the approximate temperature located at the Stratopause (or the upper limit of the Stratosphere) is -15°C. The stratospheric layer of the atmosphere spans a vertical distance of approximately 32 km from its lower to upper boundaries.
Use the lapse rate formula and the information supplied in the previous paragraph to calculate the approximate Stratospheric lapse rate:
-1.13 deg C / km
1.13 deg C / km
-6.67 deg C / km
1.51 deg C / km
Lapse rates play a crucial role in determining whether atmospheric conditions are favorable for thunderstorm development. We will therefore examine lapse rates in further detail when we explore instability in Chapter 5.
The last two layers of the atmosphere consist of the Mesosphere and the Thermosphere. In the Mesosphere, temperatures cool with height, although meteors often burn up within this atmospheric layer. Objects such as meteors travel at very high rates of speed (in tens of thousands of km hr-1), and therefore possess large amounts of kinetic energy. As meteors enter the Mesosphere, they enter a more dense segment of the earth's atmosphere with greater numbers of gas molecules. Meteors that encounter large numbers of gas molecules at high rates of speed generate large amounts of friction in the process, and this produces an enormous build-up of heat. This heat build-up ultimately is what causes fast-traveling meteors to burn up in the atmosphere.
The Thermosphere, which borders outer space, is the last of the earth's four atmospheric layers. Very few of the earth's gases are found in the Thermosphere, which translates into very low atmospheric pressure and density values found in this region of the earth's atmosphere. Gases found in the Thermosphere, however, can become quite hot, as they are among the first of the earth's gases to be exposed to incoming energy emitted by the sun. This is why temperatures increase with altitude in the Thermosphere, as shown in Fig. 3.
A passenger jet flying at cruising altitude is often traveling in the upper Troposphere at approximately 725 km per hour (or 450 mph). Why don't passenger jets burn up as meteors do?
Atmospheric temperatures found in the Troposphere are cooler than temperatures found in the Mesosphere.
Speeds of passenger jets are far slower than those of streaking meteors, and therefore do not generate as much of a heat build up as incoming meteors.
Atmospheric densities in the Troposphere are less than in the Mesosphere.
The Ozone Layer prevents ultraviolet radiation from burning up passenger jets in the Troposphere.
(WARM or COLD?) While temperature measures the AVERAGE amount of kinetic energy generated by molecules, HEAT measures the TOTAL amount of kinetic energy emitted by gas molecules. It is the concept of HEAT (our exposure to the total energy emitted by all gas molecules) that provides us a sense of warmth or cold.
Based on this concept and given the total amount of gas molecules found in the Thermosphere, would one feel WARM or COLD if exposed to conditions found in the Thermosphere?
In this chapter, we examined the basic structure of the earth's atmosphere. Atmospheric pressure and density values both decrease approximately 50% for every 5.6 km above the earth's surface. Most of the earth's atmosphere is comprised of permanent gases (nitrogen and oxygen), although it is also comprised of variable gases (carbon, water vapor, methane, ozone) which are also very important to life on earth. The earth's atmosphere is separated into four layers (Troposphere, Stratosphere, Mesosphere, Thermosphere), which each consist of unique atmospheric temperature characteristics. Most of the world's weather is confined to the Troposphere, which borders the earth's surface. The Stratosphere is where one would find the Ozone Layer, and is where the atmosphere temporarily warms with height. The Mesosphere is the third atmospheric layer, and is where streaking meteors typically burn up in the sky. The fourth and final layer is the Thermosphere, and it is where the earth's hottest atmospheric gases are found.
Now that you've mastered the basic concepts pertaining to the earth's atmospheric structure, we will next examine the earth's orientation relative to the sun in Chapter 2. We will see that this orientation is why we have seasons (fall, spring, winter, summer) on earth. In later chapters, we will further examine the earth's uneven heating patterns, and we will see that they are ultimately responsible for causing the world's weather!
Based on what was discussed in Section 1 and your answers for Tables 1 and 2, which of the following altitude segments is where one would find the greatest atmospheric pressure decrease?
0 - 5.6 km
16.8 - 22.4 km
33.6 - 39.2 km
Somewhere above 39.2 km
Given the concept of photosynthesis, what type of a surface landscape would result in relatively LOWER atmospheric Carbon Dioxide levels?
Which of the following is the correct order of atmospheric layers with lowest to highest pressure values?
Troposphere, Stratosphere, Mesosphere, Thermosphere
Mesosphere, Thermosphere, Stratosphere, Troposphere
Thermosphere, Mesosphere, Stratosphere, Troposphere
Thermosphere, Troposphere, Mesosphere, Stratosphere
 Image courtesy of the NASA Earth Observatory under public domain.
 Image courtesy of the NOAA ESRL Global Monitoring Division, Boulder, Colorado, USA, under public domain.
 Image courtesy of the U.S. National Weather Service via Wikimedia Commons under public domain.