TEA Banner
TEA Navbar

Ozone and Temperature Data Analysis, South Pole Antarctica

data | hook | main | background & resources | student

Author Contact Information

Elke Bergholz, UNIT, 24 - FDR Drive, New York, N.Y. 10034 
ebergholz@unis.org

Teachers Experiencing Antarctica (TEA) parcticipant, National 
Science Foundation (NSF), in collaboration with Climate 
Monitoring and Diagnostic Laboratory, National Oceanographic 
and Atmospheric Administration (NOAA), Boulder Colorado, D. 
Hofmann, Principal Investigator.

Overview
Overview

  • Students will analyze and plot ozone and temperature data collected at the Amundsen - Scott South Pole Station during January and February, 1999 , October 1998, October 1967

  • Students will make annual and seasonal comparison of ozone data

  • Students will become familiar with the distribution and correlation of ozone and temperature in the atmosphere from 0 to 35 kilometers

  • Students will study the chemistry of the ozone layer and its depletion, and became familiar with the nature of the ozone hole over Antarctica.

    Objectives

  • Discuss the layers of the atmosphere
  • Discuss the history of the ozone hole
  • Discuss the chemistry of ozone formation
  • Discuss the different methods of collecting ozone data (TOMS satellite, Dobson, airborne Ozonesonde) - Compare different solutions used in ozonesondes
  • Compare seasonal data collected with ozonesondes
  • Compare annual data collected with ozonesondes
  • Discuss the reason of ozone hole formation and closing
  • Compare Antarctic and Arctic ozone hole formation ( see web sites)
  • Discuss international regulations for ozone protection

    Grade Level/Discipline
    Grades 5 - 12 and beyond, Ecology, Environmental Science, Chemistry, Earth Science

    National Standards
    Grades 9-12 Content Standard A: Scientific Inquiery Content Standard B: Physical Science: Chemical Reactions Content Standard D: Earth and Space Science Content Standard E: Science and technology Content Standard F: Environmental quality Content Standard G: History and Nature of Science

    Grades 5 - 8 Content Standard A: Scientific Inquiery Content Standard D: Earth and Space Science Content Standard E: Science and technology Content Standard F: Science in Personal and Social Perspectives Content Standard G: History and Nature of Science

    Pre-activity set-up

  • be familiar with the ozone topics covered in the journals of Elke Bergholz (../../)

  • be familiar with the chemistry of ozone ( see this website which includes science about the ozone, with an excellent map explaining the vortex formation in the polar air: http://www.atm.ch.cam.ac.uk/tour/ )

  • make graphing paper or graphing computer programs available

  • copy ozone data sets attached to this activity, each data set could be plotted by different groups within the class.

    Materials

  • Ozone Data October 1967/71, October 1998, January 1999
  • Graphing paper or computer graphing programs
  • internet access (optional)
  • overhead with paper and marker
  • for an ozone model: tooth picks and Styrofoam balls.
  • order video: "Ozone - Cancer of the sky", 45 min, $ NZ 30, available from the International Antarctic Center, Christchurch, New Zealand 4 -6 weeks delivery time.

    http://www.iceberg.co.nz/eduresou.htm

    Time Frame
    Time spend on the topic will depend on the depth of study.

  • Pre-discussion time: 2 x 45 min per ozone background topic
  • Plotting time: one set of data 40 min
  • Post discussion time: 2 x 45 min

    This activity was also conducted in a 120 min time period which included the discussion time without pre discussion time

    Engagement and Exploration (Student Inquiry Activity)
    1. Step: Tell your students to imagine the following scenario: Imagine you are an ozone scientist who is about to go to the Antarctic to conduct your seasonal research. You are walking down the streets in Christchurch, New Zealand, during the month of October. It is a beautiful summer day. ( October in New Zealand is the beginning of the summer season). You forgot to put on sun lotion and you contracted a sun burn within an hour. Why, you are asking yourself? This did not happen to you in October in upstate New York! You advise the members of your research team to take sun lotion along to Antarctica.

    2. Step: Discuss with your students:

  • the difference between seasons in the Northern and Southern hemisphere. (Use a globe!!) The Austrian spring ( which is the spring of the Southern Hemisphere) starts in September whereas in the Northern hemisphere the fall starts in September.

  • that the Antarctic has 24 hour daylight during the summer

  • that there is an ozone whole over the Antarctic and that we will find out when and how it is formed.

    3. Step: Read Elke Bergholz’s journals of January 2,3,and 4 about the stay in New Zealand Go to : ../../ Go to: meet the TEA’s Go to: Elke Bergholz Go to: Elke’s Daily Journal Click on January 2, 3, and 4 individually and read journals . ( Note: if not enough computers with internet access is available, it might be useful to have copies of the journals for students).

    4. Step: Tell your student to continue to imagine the ozone scientist scenario and his/her arrival in Antarctica Imagine that you will be at the South Pole for the whole summer season, October until February. (I was at the South pole for 4 weeks in January/ February.) This is your first time for you to go to the Antarctic and you will be going all the way to the South Pole. How exciting!! You will be at the bottom of the world. Have students read my journal from January 9th and 10th : Arrival in McMurdo and at the South Pole.

    5. Step: Discuss with your student: what is actually ozone? a) Definition: ( Journal excerpt entry 1/22) What is ozone?

    Ozone derives from ordinary oxygen (O2). It is the most important trace constituent in the stratosphere. Although it is present in relative concentrations of no more than a few parts per million, it is such an efficient absorber of ultra violet light (UV light) that it is the largest source of heat in the atmosphere at altitudes between about 10 km and 50 km. UV absorption by ozone causes the temperature inversion that is responsible for the existence of the stratosphere. (see your plots of temperature and altitude, see also CMDL's web page at wwwcmdl.noaa.gov ). Ozone is also an important radiator, with strong emission bands in the 9.6 mm infrared region. In the UV-B region (290 - 315 nm) it absorbs with an efficiency that increases exponentially with decreasing wavelength, and so strongly that at 290 nm the radiation at the ground is reduced by more than a factor of 10 to the 4th from that above the ozone layer. This strong variation of absorption efficiency with wavelength in the UV-B region is the basis of the Dobson operational method (see journal 1/14) Ozone is the main source of the highly reactive OH radical, which causes the removal of many organic molecules from the atmosphere. In the troposphere, it is also a pollutant, which means that its natural concentration is increased by human activity. Because its extra oxygen bond can be easily broken, ozone is a strong oxidant that is both corrosive to materials and toxic to plants and animals. A principal of human smog, it is produced in and downwind of urban centers by photochemical reactions involving organic hydrocarbons and oxides of nitrogen. Some intrusions of stratospheric air are also a significant source of ozone in the troposphere.

    b) make a model of 1. an Ozone molecule:

    Material

  • tooth picks
  • Styrofoam balls

    Procedure: connect 3 balls with each ball representing one oxygen molecule.

    2. the layers of the atmosphere Material

  • different colored poster paper

    Procedure

  • cut and paste the different layers of the atmosphere
  • Atmospheric layers:
      - Troposphere: 7 - 15 km - Stratosphere: to about 50 km - Mesosphere: to about 80 km - Thermosphere: to about 500 km - Outer Space: > 500km

    4. Step: To understand the launching of ozone balloons: have students read the journals: It is time to get to work and collect ozone data. Read the journals about how ozone detectors work and how the ozone balloons are launched.

  • Picture of an ozone sonde: journal of Jan 13th August 6th

  • Description of the ozone sonde ( journal entry excerpt : January 12th)

  • Picture sequence of ozone balloon launching: journal 1/15

    Principle of an ozonesonde: As I have described in my journals from the summer, these sonds are two electro-chemical cells . One is an anode and the other a cathode. Both cells contain potassium iodide solutions. While the balloonrises, a small piston pump pumps air through the solution. The ozone in the pumped air reacts with the iodine solution and produces ions that create a current, which is proportional to the ozone concentration in the air. The piston pump operates by a buttery. An electronic interface board translates all the data points to the radiosonde. The radiosonde submits the data to a converter. The radio signals are converted into the computer language and the measurements appear as a graph plotted with rising altitude.

    5. Step: Plotting of ozone data: During my time on the ice, we had to launche balloons in temperatures below minus 21 Celsius. The coldest day was minus 40 Celsius. Imagine how well planned everything had to go. The plotting, however, was done by the computer.

    a) Divide the class in different groups and use three different sets of data, see Appendix for data and results. Groups: 1. Ozone Data, October 1967/71 2. Ozone Data, October 1998 3. Ozone Data, January 1999

    b) Have students follow the instructions of General Activity Description (see Student Reproducible Masters)

    c) One representative of the group should transfer the plot onto a transparent overhead paper

    d) Present all data to class using an overhead by overlaying the group data

    Explanation (Discussing)
    The following questions can be discussed:

    1. Where do we find the most ozone concentration in January? In the Stratosphere, from about 15 to 25 kilometers. See graph.

    2. Are there seasonal ozone concentration differences? ( Compare the ozone data collected in October 1998 and Jan 1999)

    Ozone concentration in the stratosphere is almost "0" in October 1998 compared to January of 1999. This indicates the depletion of ozone during the Antarctic Spring time in September and October. This is called the Antarctic ozone hole: the Antarctic ozone hole is seasonal.

    It is often misunderstood that the ozone hole over the Antarctic exists all year around, which is not true: the Antarctic ozone hole is seasonal. See also Background information journal entires:

  • 1/23: history of the ozone hole
  • 1/25: pollutants in the stratosphere

    3. Where in the atmosphere is the ozone whole? The ozone hole is located in the stratosphere and it is not a solid hole throughout the atmosphere. ( See graph: October 1998). However, there is an overall depletion of ozone up to 10% throughout the world

    Total ozone loss: excerpt journal entry 1/26, emailo interview with Dr. Bryan Johnson, CMDL, Boulder, Colorado

    " The question about ozone loss is hard to answer - since ozone is always being produced and destroyed. The average rate of decline in total ozone is about 4 to 6% per decade (10 years). I think the number the students are asking about may be that the total ozone destroyed over Antarctica in one season represents about 3% of the ozone in the atmosphere. The main idea to have the students understand is that ozone is not a limited quantity in the atmosphere that we are running out of - it is a balance of destruction and production processes, and when we have excess chlorine in the stratosphere then we reach a lower level of balance - because chlorine adds an extra (very effective) destruction process. Ozone is produced mostly in the equator regions, but the dynamics of wind and currents transport ozone out of the tropics and to the mid-latitudes where it tends to build up."

    4. Can we observe annual differences in ozone concentrations? Compare the ozone data collected in October 1967 with those collected in October 1998.

    Data plots will reveal that the ozone hole did not exist in the late 60ties. (See Graphs)

    The first CFC’s produced and used took several decades to make it to the Stratosphere. Therefore, not enough CFC’s were available yet in the late 60ties (see October 1967 data) to deplete the stratosphere compared to the October 1998 ozone data which shows the stratospheric ozone depletion.

    Elaboration (Polar Applications)
    Extensions 1. Graphing of the Temperature depending on the altitude: Plot the temperature depending on the Altitude

    Questions: 1. How does the temperature change in the atmosphere?

    2. Research on Total Ozone: a) Compare total ozone data (compared to the ozone profile you plotted) collected with the ozonesonde with total ozone collected with the DOBSON. Go to total ozone archives. (Total ozone collected at the South Pole is listed in the heading of each data set.) http://www.cmdl.noaa.gov/owv

    Questions: 1. What are typical ground levels of ozone and total ozone levels? About 300

    2. What is a DOBSON unit? See Journal entry:

    b) Comparison of Satellite TOMS ozone data using TOMS data archives: http://jwocky.gsfc.nasa.gov/eptoms/toda.html

    Exchange (Students Draw Conclusions)
    Student's Conclusions:

    1. Ozone is mostly abundant in the stratosphere.

    2. The Ozone depletions happens seasonal : in the Antarctic springtime: September/ October.

    3. The depletion of the stratospheric ozone during the Antarctic spring has decreased since the 60ties to almost zero.

    4. Ozone depletion happens because of CFC’s brought down to the Antarctic via atmospheric circulation where it combines with a single ozone molecule which is then not available anymore for ozone formation.

    5. The seasonal Antarctic stratospheric ozone hole will close again during the month of November and December with ozone produced in the equator reagion and circulated to the Pole.

    6. There is an overall loss of ozone of about 5 -10%

    Evaluation (Assessing Student Performance)
    1. Modeling skills

  • is the student able to produce an ozone and atmosphere model

    1. Graphing skills assessment:

  • Can the student choose the correct axis?
  • Is the student able to plot data points.?

    2. Drawing conclusions about the data:

  • is the student able to ‘read the story’ of the graph? Example: the October 1998 data express the depletion of ozone in the stratosphere.

    3. Incorporating and synthesizing written information with the plotting information:

  • is the student able to draw conclusions from the journal reading and find explanations to the ozone depletion?

    data | hook | main | background & resources | student