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Glossary Annex III
AIII
transport is converging, mass conservation requires a vertical flow away
from the surface. This is called Ekman pumping. The opposite effect, in case
of divergence, is called Ekman suction. The effect is important in both the
atmosphere and the ocean.
Ekman transport The total transport resulting from a balance between
the Coriolis force and the frictional stress due to the action of the wind on
the ocean surface. See also Ekman pumping.
Electromagnetic spectrum Wavelength or energy range of all elec-
tromagnetic radiation. In terms of solar radiation, the spectral irradiance is
the power arriving at the Earth per unit area, per unit wavelength.
El Niño-Southern Oscillation (ENSO) The term El Niño was initially
used to describe a warm-water current that periodically flows along the
coast of Ecuador and Peru, disrupting the local fishery. It has since become
identified with a basin-wide warming of the tropical Pacific Ocean east of
the dateline. This oceanic event is associated with a fluctuation of a global-
scale tropical and subtropical surface pressure pattern called the Southern
Oscillation. This coupled atmosphere–ocean phenomenon, with preferred
time scales of two to about seven years, is known as the El Niño-Southern
Oscillation (ENSO). It is often measured by the surface pressure anomaly
difference between Tahiti and Darwin or the sea surface temperatures in
the central and eastern equatorial Pacific. During an ENSO event, the pre-
vailing trade winds weaken, reducing upwelling and altering ocean cur-
rents such that the sea surface temperatures warm, further weakening the
trade winds. This event has a great impact on the wind, sea surface tem-
perature and precipitation patterns in the tropical Pacific. It has climatic
effects throughout the Pacific region and in many other parts of the world,
through global teleconnections. The cold phase of ENSO is called La Niña.
For the corresponding indices, see Box 2.5.
Emission scenario A plausible representation of the future develop-
ment of emissions of substances that are potentially radiatively active
(e.g., greenhouse gases, aerosols) based on a coherent and internally con-
sistent set of assumptions about driving forces (such as demographic and
socioeconomic development, technological change) and their key relation-
ships. Concentration scenarios, derived from emission scenarios, are used
as input to a climate model to compute climate projections. In IPCC (1992)
a set of emission scenarios was presented which were used as a basis
for the climate projections in IPCC (1996). These emission scenarios are
referred to as the IS92 scenarios. In the IPCC Special Report on Emission
Scenarios (Nakićenović and Swart, 2000) emission scenarios, the so-called
SRES scenarios, were published, some of which were used, among others,
as a basis for the climate projections presented in Chapters 9 to 11 of IPCC
(2001) and Chapters 10 and 11 of IPCC (2007). New emission scenarios
for climate change, the four Representative Concentration Pathways, were
developed for, but independently of, the present IPCC assessment. See also
Climate scenario and Scenario.
Energy balance The difference between the total incoming and total
outgoing energy. If this balance is positive, warming occurs; if it is nega-
tive, cooling occurs. Averaged over the globe and over long time periods,
this balance must be zero. Because the climate system derives virtually all
its energy from the Sun, zero balance implies that, globally, the absorbed
solar radiation, that is, incoming solar radiation minus reflected solar radi-
ation at the top of the atmosphere and outgoing longwave radiation emit-
ted by the climate system are equal. See also Energy budget.
Energy Balance Model (EBM) An energy balance model is a sim-
plified model that analyses the energy budget of the Earth to compute
changes in the climate. In its simplest form, there is no explicit spatial
dimension and the model then provides an estimate of the changes in
globally averaged temperature computed from the changes in radiation.
This zero-dimensional energy balance model can be extended to a one-
dimensional or two-dimensional model if changes to the energy budget
with respect to latitude, or both latitude and longitude, are explicitly con-
sidered. See also Climate model.
Energy budget (of the Earth) The Earth is a physical system with
an energy budget that includes all gains of incoming energy and all losses
of outgoing energy. The Earth’s energy budget is determined by measur-
ing how much energy comes into the Earth system from the Sun, how
much energy is lost to space, and accounting for the remainder on Earth
and its atmosphere. Solar radiation is the dominant source of energy into
the Earth system. Incoming solar energy may be scattered and reflected
by clouds and aerosols or absorbed in the atmosphere. The transmitted
radiation is then either absorbed or reflected at the Earth’s surface. The
average albedo of the Earth is about 0.3, which means that 30% of the
incident solar energy is reflected into space, while 70% is absorbed by
the Earth. Radiant solar or shortwave energy is transformed into sensible
heat, latent energy (involving different water states), potential energy, and
kinetic energy before being emitted as infrared radiation. With the average
surface temperature of the Earth of about 15°C (288 K), the main outgoing
energy flux is in the infrared part of the spectrum. See also Energy balance,
Latent heat flux, Sensible heat flux.
Ensemble A collection of model simulations characterizing a climate
prediction or projection. Differences in initial conditions and model formu-
lation result in different evolutions of the modelled system and may give
information on uncertainty associated with model error and error in initial
conditions in the case of climate forecasts and on uncertainty associated
with model error and with internally generated climate variability in the
case of climate projections.
Equilibrium and transient climate experiment An equilibrium
climate experiment is a climate model experiment in which the model is
allowed to fully adjust to a change in radiative forcing. Such experiments
provide information on the difference between the initial and final states
of the model, but not on the time-dependent response. If the forcing is
allowed to evolve gradually according to a prescribed emission scenario,
the time-dependent response of a climate model may be analysed. Such
an experiment is called a transient climate experiment. See also Climate
projection.
Equilibrium climate sensitivity See Climate sensitivity.
Equilibrium line The spatially averaged boundary at a given moment,
usually chosen as the seasonal mass budget minimum at the end of
summer, between the region on a glacier where there is a net annual loss
of ice mass (ablation area) and that where there is a net annual gain (accu-
mulation area). The altitude of this boundary is referred to as equilibrium
line altitude (ELA).
Equivalent carbon dioxide (CO
2
) concentration The concentra-
tion of carbon dioxide that would cause the same radiative forcing as
a given mixture of carbon dioxide and other forcing components. Those
values may consider only greenhouse gases, or a combination of green-
house gases and aerosols. Equivalent carbon dioxide concentration is a
metric for comparing radiative forcing of a mix of different greenhouse
gases at a particular time but does not imply equivalence of the corre-
sponding climate change responses nor future forcing. There is generally
no connection between equivalent carbon dioxide emissions and resulting
equivalent carbon dioxide concentrations.
Equivalent carbon dioxide (CO
2
) emission The amount of carbon
dioxide emission that would cause the same integrated radiative forcing,
over a given time horizon, as an emitted amount of a greenhouse gas or
a mixture of greenhouse gases. The equivalent carbon dioxide emission is
obtained by multiplying the emission of a greenhouse gas by its Global
Warming Potential for the given time horizon. For a mix of greenhouse