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Transcript
Global warming
Global mean surface temperature change from 1880 to 2015, relative to the 1951–1980 mean.
The black line is the annual mean and the red line is the 5-year running mean. Source: NASA
GISS.
World map showing surface temperature trends (°C per decade) between 1950 and 2014. Source:
NASA GISS.
Fossil fuel related carbon dioxide (CO2) emissions compared to five of the IPCC's "SRES"
emissions scenarios, published in 2000. The dips are related to global recessions. Image source:
Skeptical Science.
Fossil fuel related carbon dioxide emissions over the 20th century. Image source: EPA.
Global warming and climate change are terms for the observed century-scale rise in the
average temperature of the Earth's climate system and its related effects. Multiple lines of
scientific evidence show that the climate system is warming. Although the increase of nearsurface atmospheric temperature is the measure of global warming often reported in the popular
press, most of the additional energy stored in the climate system since 1970 has gone into ocean
warming. The remainder has melted ice and warmed the continents and atmosphere. Many of the
observed changes since the 1950s are unprecedented over tens to thousands of years. On 12
November 2015, NASA scientists reported that human-made carbon dioxide (CO2) continues to
increase above levels not seen in hundreds of thousands of years: currently, about half of the
carbon dioxide released from the burning of fossil fuels is not absorbed by vegetation and the
oceans and remains in the atmosphere.
Scientific understanding of global warming is increasing. The Intergovernmental Panel on
Climate Change (IPCC) reported in 2014 that scientists were more than 95% certain that global
warming is mostly being caused by increasing concentrations of greenhouse gases (GHG) and
other human (anthropogenic) activities. Climate model projections summarized in the report
indicated that during the 21st century the global surface temperature is likely to rise a further 0.3
to 1.7 °C (0.5 to 3.1 °F) for their lowest emissions scenario using stringent mitigation and 2.6 to
4.8 °C (4.7 to 8.6 °F) for their highest. These findings have been recognized by the national
science academies of the major industrialized nation and are not disputed by any scientific body
of national or international standing.
Warmest years
15 of the top 16 warmest years have occurred since 2000. While record-breaking years can
attract considerable public interest, individual years are less significant than the overall trend. So
some climatologists have criticized the attention that the popular press gives to "warmest year"
statistics; for example, Gavin Schmidt stated "the long-term trends or the expected sequence of
records are far more important than whether any single year is a record or not."
2015 was not only the warmest year on record, it broke the record by the largest margin by
which the record has been broken. 2015 was the 39th consecutive year with above-average
temperatures. Ocean oscillations like El Niño Southern Oscillation (ENSO) can affect global
average temperatures, for example, 1998 temperatures were significantly enhanced by strong El
Niño conditions. 1998 remained the warmest year until 2005 and 2010 and the temperature of
both of these years was enhanced by El Niño periods. The large margin by which 2015 is the
warmest year is also attributed to another strong El Niño. However, 2014 was ENSO neutral.
According to NOAA and NASA, 2015 had the warmest respective months on record for 10 out
of the 12 months. The average temperature around the globe was 1.62˚F (0.90˚C) or 20% above
the twentieth century average. In a first, December 2015 was also the first month to ever reach a
temperature 2 degrees Fahrenheit above normal for the planet.
Greenhouse gases
The greenhouse effect is the process by which absorption and emission of infrared radiation by
gases in a planet's atmosphere warm its lower atmosphere and surface. It was proposed by
Joseph Fourier in 1824, discovered in 1860 by John Tyndall, was first investigated quantitatively
by Svante Arrhenius in 1896, and was developed in the 1930s through 1960s by Guy Stewart
Callendar.
On Earth, naturally occurring amounts of greenhouse gases have a mean warming effect of about
33 °C (59 °F). Without the Earth's atmosphere, the Earth's average temperature would be well
below the freezing temperature of water. The major greenhouse gases are water vapor, which
causes about 36–70% of the greenhouse effect; carbon dioxide (CO2), which causes 9–26%;
methane (CH4), which causes 4–9%; and ozone (O3), which causes 3–7%. Clouds also affect the
radiation balance through cloud forcing similar to greenhouse gases.
Human activity since the Industrial Revolution has increased the amount of greenhouse gases in
the atmosphere, leading to increased radiative forcing from CO2, methane, tropospheric ozone,
CFCs and nitrous oxide. According to work published in 2007, the concentrations of CO2 and
methane have increased by 36% and 148% respectively since 1750. These levels are much
higher than at any time during the last 800,000 years, the period for which reliable data has been
extracted from ice cores. Less direct geological evidence indicates that CO2 values higher than
this were last seen about 20 million years ago.
Fossil fuel burning has produced about three-quarters of the increase in CO2 from human activity
over the past 20 years. The rest of this increase is caused mostly by changes in land-use,
particularly deforestation. Estimates of global CO2 emissions in 2011 from fossil fuel
combustion, including cement production and gas flaring, was 34.8 billion tonnes (9.5 ± 0.5
PgC), an increase of 54% above emissions in 1990. Coal burning was responsible for 43% of the
total emissions, oil 34%, gas 18%, cement 4.9% and gas flaring 0.7%.
The ozone layer and it’s depletion
The ozone layer or ozone shield refers to a region of Earth's stratosphere that absorbs most of
the Sun's ultraviolet (UV) radiation. It contains high concentrations of ozone (O3) relative to
other parts of the atmosphere, although still very small relative to other gases in the stratosphere.
The ozone layer contains less than 10 parts per million of ozone, while the average ozone
concentration in Earth's atmosphere as a whole is only about 0.3 parts per million.
The photochemical mechanisms that give rise to the ozone layer were discovered by the British
physicist Sydney Chapman in 1930. Ozone in the Earth's stratosphere is created by ultraviolet
light striking ordinary oxygen molecules containing two oxygen atoms (O2), splitting them into
individual oxygen atoms (atomic oxygen); the atomic oxygen then combines with unbroken O2
to create ozone, O3. The ozone molecule is unstable (although, in the stratosphere, long-lived)
and when ultraviolet light hits ozone it splits into a molecule of O2 and an individual atom of
oxygen, a continuing process called the ozone-oxygen cycle. Chemically, this can be described
as:
O2 + ℎνuv → 2O
O + O2 ↔ O3
Alternatively,
2 O3 → 3 O2
O + O2 = O3
This is a continuing process that terminates when an oxygen atom "recombines" with an ozone
molecule to make two O2 molecules.
O + O3 = 2O2
About 90% of the ozone in our atmosphere is contained in the stratosphere.
Ozone depletion describes two distinct but related phenomena observed since the late 1970s: a
steady decline of about 4% in the total amount of ozone in Earth's stratosphere (the ozone layer),
and a much larger springtime decrease in stratospheric ozone around Earth's polar regions.
CFCs and other contributory substances are referred to as ozone-depleting substances (ODS).
Since the ozone layer prevents most harmful UVB wavelengths (280–315 nm) of ultraviolet light
(UV light) from passing through the Earth's atmosphere, observed and projected decreases in
ozone generated worldwide concern, leading to adoption of the Montreal Protocol that bans the
production of CFCs, halons, and other ozone-depleting chemicals such as carbon tetrachloride
and trichloroethane.
Ozone can be destroyed by a number of free radical catalysts, the most important of which are
the hydroxyl radical (OH·), nitric oxide radical (NO·), chlorine radical (Cl·) and bromine radical
(Br·). The dot is a common notation to indicate that all of these species have an unpaired electron
and are thus extremely reactive. All of these have both natural and man-made sources; at the
present time, most of the OH· and NO· in the stratosphere is of natural origin, but human activity
has dramatically increased the levels of chlorine and bromine. These elements are found in
certain stable organic compounds, especially chlorofluorocarbons (CFCs), which may find their
way to the stratosphere without being destroyed in the troposphere due to their low reactivity.
Once in the stratosphere, the Cl and Br atoms are liberated from the parent compounds by the
action of ultraviolet light, e.g.
CFCl3 + electromagnetic radiation → Cl· + ·CFCl2
The Cl and Br atoms can then destroy ozone molecules through a variety of catalytic cycles. In
the simplest example of such a cycle,[4] a chlorine atom reacts with an ozone molecule, taking an
oxygen atom with it (forming ClO) and leaving a normal oxygen molecule. The chlorine
monoxide (i.e., the ClO) can react with a second molecule of ozone (i.e., O3) to yield another
chlorine atom and two molecules of oxygen. The chemical shorthand for these gas-phase
reactions is:


Cl· + O3 → ClO + O2: The chlorine atom changes an ozone molecule to ordinary oxygen
ClO + O3 → Cl· + 2 O2: The ClO from the previous reaction destroys a second ozone
molecule and recreates the original chlorine atom, which can repeat the first reaction and
continue to destroy ozone.