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Title: Basic definitions, terms, e.g., Climate, climatology, anomaly, teleconnection,


1
Mid-course overview(NB overview a guide but not
necessarily everything)
Chapter 1. Intro. Review elements include
  • Basic definitions, terms, e.g., Climate,
    climatology, anomaly, teleconnection,
  • Trace gases, anthropogenic increase
  • Perspective from paleoclimate on where fossil
    fuels come from, some idea of time scales,
    natural variability, are recent changes
    unusual,..
  • ENSO material, mostly as comes back in chpt 4.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
2
1.1 Climate dynamics, climate change and climate
prediction
  • Climate average condition of the atmosphere,
    ocean, land surfaces and the ecosystems in them
    (includes average measures of weather-related
    variability, e.g. storm frequency)
  • Weather state of atmosphere and ocean at given
    moment.
  • Average taken over January of many different
    years to obtain a climatological value for
    January, etc.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
3
  • Climate change
  • occurring on many time scales, including those
    that affect human activities.
  • time period used in the average will affect the
    climate that one defines.
  • e.g., 1950-1970 will differ from the average from
    1980-2000.
  • Climate variability
  • essentially all the variability that is not just
    weather.
  • e.g., ice ages, warm climate at the time of
    dinosaurs, drought in African Sahel region, and
    El Niño.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
4
  • Global warming predicted warming, associated
    changes in the climate system in response to
    increases in "greenhouse gases" emitted into
    atmosphere by human activities.
  • Greenhouse gases e.g., carbon dioxide, methane
    and chlorofluorocarbons trace gases that absorb
    infrared radiation, affect the Earth's energy
    budget.
  • warming tendency, known as the greenhouse effect
  • Climate prediction endeavor to predict not only
    human-induced changes but the natural variations.
    e.g., El Niño
  • Climate models
  • Mathematical representations
  • of the climate system
  • typically equations for temperature,
  • winds, ocean currents and other climate
  • variables solved numerically on computers.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
5
  • El Niño
  • largest interannual (year-to-year) climate
    variation interaction between the tropical
    Pacific ocean and the atmosphere above it.
  • a prime example of natural climate variability.
  • first phenomenon for which the essential role of
    dynamical interaction between atmosphere and
    ocean was demonstrated.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
6
  • Teleconnections remote effects of El Niño (or
    other regional climate variations).
  • Anomaly departure from normal climatological
    conditions.
  • calculated by difference between value of a
    variable at a given time, e.g., pressure or
    temperature for a particular month, and
    subtracting the climatology of that variable.
  • Climatology includes the normal seasonal cycle.
  • e.g., anomaly of summer rainfall for June, July
    and August 1997, average of rainfall over that
    period minus averages of all June, July and
    August values over a much longer period, such as
    1950-1998.
  • To be precise, the averaging time period for the
    anomaly and the averaging time period for the
    climatology should be specified.
  • e.g., monthly averaged SST anomalies relative to
    1950-2000 mean.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
7
Table 1.1
1.4 Global change in recent history
Air main constituents Formula Concentration
Nitrogen N2 78.08
Oxygen O2 20.95
Water H2O 0.1 to 2
Trace gas name Concentration (in 2004)
Carbon dioxide CO2 377 (parts per million) ppm, 0.038
Methane CH4 1.75 ppm
Nitrous oxide N2O 0.32 ppm
Ozone O3 0.000251 ppm (atm. average) (10 ppm max in stratosphere)
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
8
Carbon dioxide concentrations since
1958,measured at Mauna Loa, Hawaii.
Figure 1.1
  • Annual, interannual variations
  • biological impacts on carbon cycle
  • Trend due to fossil fuel emissions.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
9
Figure 1.2
Concentration of various trace gasesestimated
since 1850
  • Methane Cattle, sheep, rice paddies, fossil fuel
    by-product wetlands, termites (parts per
    billion).
  • Nitrous Oxide biomass burning, fertilizers?
  • Chlorofluorocarbons man-made, zero before 1950
    (parts per trillion).

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
10
Figure 1.3
Global mean surface temperatures estimated since
preindustrial times
  • Anomalies relative to 1961-1990 mean
  • Annual average values of combined near-surface
    air temperature over continents and sea surface
    temperature over ocean.
  • Curve smoothing similar to a decadal running
    average.
  • From University of East Anglia Climatic Research
    Unit, Brohan et al. (2006).

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
11
1.5 El Niño An example of natural climate
variability
  • ENSO El Niño/Southern Oscillation.
  • Contd in Chpt 4
  • El Niño is associated with warm phase of a
    phenomenon that is largely cyclic.
  • La Niña for the cold phase.
  • El Niño arises in tropical Pacific along the
    equator.
  • Changes in sea surface temperature, ocean
    subsurface temperatures down to a few hundred
    meters depth, rainfall, and winds ocean-atmos.
    interaction!
  • Variations in the Pacific basin within about
    10-15 degrees latitude of the equator are the
    primary variables.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
12
Paleoclimate A few climate notes with Geological
time scale
Figure 1.12
  • Very distant past--- Myrmillions of years
  • Key points
  • Climate can vary substantially, on all timescales
  • Long periods in deep past with warmer climate
    than present ( higher est. CO2 )
  • deposition over 100s of millions of years
    sequesters carbon dioxide as fossil fuels (oil,
    coal, natural gas)
  • return of this CO2 to atmosphere occurring over
    very short period.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
13
Antarctic ice core records of CO2, deuterium
isotope ratio variations (dD), and Antarctic air
temperature inferred from dD
Figure 1.13
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
14
Chapter 2 Basics of Global Climate
  • Review elements include
  • Basic concepts and terminology that tend to recur
    later
  • E.g., albedo, moist convection, easterly winds

2.1 Components and phenomena in the climate system
  • Climate processes
  • solar radiation tends to get through the
    atmosphere ocean heated from above Þ stable to
    vertical motions.
  • warm surface layer, colder deep waters
  • mixing near ocean surface Þ upper mixed layer
    50 m
  • mixing carries surface warming down as far as
    thermocline, layer of rapid transition of
    temperature to the colder abyssal waters below

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
15
Satellite image based on visible light with 5x5
grid overlay
Figure 2.2
Courtesy of NASA
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
16
The parameterization problem
  • For each grid box in a climate model, only the
    average across the grid box of wind, temperature,
    etc. is represented.
  • The average of smaller scale effects has
    important impacts on large-scale climate.
  • e.g., clouds primarily occur at small scales, yet
    the average amount of sunlight reflected by
    clouds affects the average solar heating of a
    whole grid box.
  • Parameterization representing average effects of
    scales smaller than the grid scale (e.g., clouds)
    as a function of the grid scale variables (e.g.
    temperature and moisture) in a climate model.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
17
2.2 Basics of radiative forcing
  • Solar radiation input Infrared radiation (IR) is
    the only way this heat input can be balanced by
    heat loss to space
  • Since IR emissions depend on the Earth's
    temperature, the planet tends to adjust to a
    temperature where IR energy loss balances solar
    input
  • Blackbody radiation approximation for how
    radiation depends on temperature
  • Total energy flux integrated across all
    wavelengths of light
  • R sT4
  • Full climate models do detailed computation as a
    function of wavelength, for every level in the
    atmosphere,
  • Trace gases absorb IR at wavelengths where O2,
    N2 ineffective.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
18
Pathways of energy transfer in a global average
2.3 Globally averaged energy budget
Figure 2.8
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
19
  • Greenhouse effect
  • The upward IR from the surface is mostly trapped
    in the atmosphere, rather than escaping directly
    to space, so it tends to heat the atmosphere.
  • The atmosphere warms to a temperature where it
    emits sufficient radiation to balance the heat
    budget, but it emits both upward and downward, so
    part of the energy is returned back down to the
    surface where it is absorbed.
  • This results in additional warming of the
    surface, compared to a case with no atmospheric
    absorption of IR.
  • Atmosphere emits IR downward Þ absorbed at
    surface.
  • Both gases and clouds contribute to absorption of
    IR and thus to the greenhouse effect.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
20
Pathways of energy transfer in a global average
(cont.)
  • At the top of the atmosphere, in the global
    average and for a steady climate
  • IR emitted balances incoming solar.
  • Global warming involves a slight imbalance
  • a change in the greenhouse effect Þ slightly less
    IR emitted from the top (chap. 6).
  • small imbalance Þ slow warming.
  • Three roles for clouds and convection
  • heating of the atmosphere (through a deep layer)
  • reflection of solar radiation (contributing to
    albedo)
  • trapping of infrared radiation (contributing to
    the greenhouse effect)

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
21
2.4 Gradients of rad. forcing and energy
transport by atm.
  • Differences in input of solar energy between
    latitudes Þ temperature gradients.
  • These gradients would be huge if it were not for
    heat transport in ocean atmosphere and heat
    storage in ocean.

Figure 2.9
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
22
Latitude structure of the circulation (cont.)
  • Hadley cell thermally driven, overturning
    circulation, rising in the tropics and sinking at
    slightly higher latitudes (the subtropics).
  • Explanations of this in chpt. 3
  • Relation to observations
  • rising branch assoc. with convective heating and
    heavy rainfall subtropical descent regions,
    little rain.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
23
Figure 2.13
  • Intertropical convergence zones (ITZCs) or
    tropical convection zones heavy precipitation
    features deep in the tropics, (convergence refers
    to the low level winds that converge into these
    regions).
  • Monsoons tropical convection zones move
    northward in northern summer, southward in
    southern summer, especially over continents.
  • Not just a function of latitude, e.g., strong
    convection over tropical western Pacific, little
    over cold eastern Pacific Walker circulation
    along equator

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
24
Figure 2.16
  • Equatorial cold tongue along the equator in the
    Pacific.
  • maintained by upwelling of cold water from below.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
25
Equatorial Walker circulation
Figure 2.14
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
26
Ocean vertical structure
Figure 2.18
  • Ocean surface is warmed from above Þ lighter
    water over denser water (stable
    stratification).
  • Deep waters tend to remain cold
  • on long time scales, import of cold waters from a
    few sinking regions near the poles maintains cold
    temperatures.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
27
The thermohaline circulation
Figure 2.19
  • Salinity (concentration of salt) affects ocean
    density in addition to temperature.
  • Waters dense enough to sink cold and salty
  • Thermohaline circulation deep overturning
    circulation is termed the (thermal for the
    temperature, haline from the greek word for salt,
    hals).

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
28
The carbon cycle
Figure 2.21b
Values from Denman et al. , IPCC (2007) format
follows Sarmiento and Gruber , Physics Today
(2002).
  • Fossil fuels 6.4 PgC/yr (1990s) (incl. 0.1 PgC/yr
    cement production)
  • 40 coal, 40 from oil and derivatives such as
    gasoline, 20 from natural gas
  • 1.6 PgC/yr land-use change e.g., deforestation
    to agricultural (smaller C storage)
  • 1990s anthropogenic emissions 8 PgC/yr (6.4
    fossil fuels 1.6 land use change)
  • Fortunately, less than half remains in the
    atmosphere
  • 2.2 PgC/yr increased flux into ocean 2.5
    PgC/yr taken up by land vegetation

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
29
Fossil fuel emissions and increases in
atmospheric CO2 concentrations
Figure 2.22
Values are from Denman et al., IPCC (2007)
format follows Sarmiento and Gruber , Physics
Today (2002).
  • Fossil fuel emissions converted to CO2
    concentration change if all remained in the
    atmosphere (1 ppm for each 2.1 PgC) rising
  • Actual rate of accumulation (change in
    concentration each year all positive rising
    concentration, but variable rate of increase)
  • Variations primarily due to land biosphere, e.g.,
    droughts assoc with ENSO
  • Accumulation rate 55 of fossil fuel emissions
    on average

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
30
Chapter 3 Physical Processes in the Climate
System
Review elements include
  • Where do we get the equations in climate models
    (conservation of momentum, energy, mass,eq of
    state)
  • Main balances from these equations especially as
    we apply them to explain important climate
    features
  • PGF vs Coriolis
  • Thermal circulation, thermal expansion
  • Upwelling,

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
31
3.1 Conservation of Momentum
Only in vertical
  • Coriolis force due to rotation of earth
    (apparent force).
  • PGF pressure gradient force. Tends to move air
    from high to low pressure.
  • Fdrag friction-like forces due to turbulent or
    surface drag.

Use force per unit mass for atm/oc.
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
32
Coriolis force (cont.)
  • Turns a body or air/water parcel to the right in
    the northern hemisphere to the left in the
    southern hemisphere.
  • Exactly on the equator, the horizontal component
    of the Coriolis force is zero
  • Acts only for bodies moving relative to the
    surface of the Earths equator and is
    proportional to velocity.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
33
Schematic of geostrophic wind and wind with
frictional effects
Figure 3.4
Geostrophic balance At large scales at
mid-latitudes and approaching the tropics the
Coriolis force and the pressure gradient force
are the dominant forces (for horizontal motions)
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
34
Section 3.1 Overview
  • An approximate balance between the Coriolis force
    and the pressure gradient force holds for winds
    and currents in many applications (geostrophic
    balance) (Fig. 3.4).
  • The Coriolis force tends to turn a flow to the
    right of its motion in the Northern Hemisphere
    (left in the Southern Hemisphere) the pressure
    gradient force acts from high toward low
    pressure.
  • The Coriolis parameter f varies with latitude
    (zero at the equator, increasing to the north,
    negative to the south) this is called the
    beta-effect (?? rate of change of f with
    latitude).
  • In the vertical direction, the pressure gradient
    force balances gravity (hydrostatic balance).
    This allows us to use pressure as a vertical
    coordinate. Pressure is proportional to the mass
    above in the atmospheric or oceanic column.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
35
Figure 3.5
Application thermal circulation
  • Tropics (Hadley circ) subtropics
  • West Pacific (Walker circ.) East Pacific
  • relatively low pressure (at given height) at
    low levels in warm region PGF toward warm region
    (near surface)

e.g.
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
36
Section 3.2 Overview
  • Atmos relationship of density to pressure and
    temperature from ideal gas law
  • Ocean density depends on temperature (warmer
    less dense, e.g. sea level rise by warming)
    salinity (saltier more dense).
  • Thermal circulations (Fig. 3.5) warm atmospheric
    column has low pressure near the surface and
    high pressure aloft relative to pressure at same
    height in a neighboring cold region. Reason see
    Fig. 3.5
  • PGF near surface toward warm region Coriolis
    force may affect circulation but warm region
    tends to have convergence rising. e.g. Walker,
    Hadley circulations
  • sea level rise by thermal expansion density
    changes by given fraction (thermal expansion
    coefficient) so sea level rise proportional to
    depth of column that warmsdT e.g., deep vs
    upper ocean

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
37
Section 3.3 Overview
  • Ocean time rate of change of temperature of
    water parcel given by heating
  • for a surface layer net surface heat flux from
    the atm. minus the flux out the bottom by mixing
  • Atmosphere Temperature eqn. similar to ocean
    but
  • when an air parcel rises, temperature decreases
    as parcel expands towards lower pressure.
  • Quickly rising air parcel (e.g. in thermals)
    little heat is exchanged
  • temperature decreases at 10 C/km (the dry
    adiabatic lapse rate).

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
38
Section 3.3 Overview (cont.)
  • Time derivatives following parcel hide
    complexity of the system the parcels themselves
    tend to deform in complex ways if followed for a
    long time.
  • Results in the loss of predictability for
    weather.
  • The time derivative for temperature at a fixed
    point is obtained by expanding the time
    derivative for the parcel in terms of velocity
    times the gradients of temperature (advection).
  • Similar procedure applies in other equations.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
39
Coastal upwelling e.g., Peru northward wind
component along a north-south coast
Figure 3.9
  • Drag of wind stress tends to accelerate currents
    northward
  • Coriolis force turns current to left in S. Hem
  • momentum eqn.
  • u away from coast horizontal divergence
    upwelling from below thru bottom of surface
    layer 50m
  • Continuity eqn.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
40
Processes leading to equatorial upwelling
Figure 1.7
  • Wind stress accelerates currents westward
  • wind speed fast relative to currents, so
    frictional drag at surface slows the wind but
    accelerates the currents
  • Just north of Equator small Coriolis force turns
    current slightly to right (south of Equator to
    the left) divergence in surface layer
    balanced by upwelling from below

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
41
Figure 3.11
3.4e Conservation of warm water mass in idealized
layer above thermocline
warm less dense
cold dense
  • Warm light water above thermocline at depth h
  • Horizontal divergence/convergence in upper layer
    movement of thermocline

approx. H mean
thermocline depth,
D vertical avg. thru layer

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
42
Section 3.5 Overview
  • Conservation of mass gives equations for water
    vapor (atmosphere) and salinity (ocean) and
    other things, e.g. ice/snow
  • water vapor main sinks moist convection
    precipitation source surface evaporation
    (transport in between)
  • Salinity at the ocean surface is increased by
    evaporation and decreased by precipitation.
  • latent heat of condensation water vapor sink
    gives heating in clouds (connecting mass and
    energy equations)
  • Latent heat of melting important to surface mass
    balance of ice (or snow), e.g., application to
    time needed to melt an ice sheet by surface heat
    flux imbalance W/m2 vs kg/m2 J/kg

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
43
Section 3.6 Overview
  • Saturation of moist air depends on temperature
    according to Figure 3.12. Relative humidity gives
    the water vapor relative to the saturation value.
  • A rising parcel in moist convection decreases in
    temperate according to the dry adiabatic lapse
    rate until it saturates, then has a smaller moist
    adiabatic lapse rate. The temperature curve in
    Figure 3.13 (the moist adiabat) depends on only
    the surface temperature and humidity where the
    parcel started.
  • If this curve is warmer than the temperature at
    upper levels, convection typically occurs.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
44
3.7 Wave Processes in the Atmosphere and Ocean
Overview
Skim for qualitative background for chpt 4.
  • Waves play an important role in communicating
    effects from one part of the atmosphere to
    another.
  • Rossby waves depend on the beta-effect change
    of coriolis force with latitude. Their inherent
    phase speed is westward. In a westerly mean flow,
    stationary Rossby waves can occur in which the
    eastward motion of the flow balances the westward
    propagation. Stationary perturbations, such as
    convective heating anomalies during El Nino, tend
    to excite wavetrains of stationary Rossby waves.

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
45
Chapter 4El Nino
Review elements include
  • Tropical Pacific climatology as it sets the stage
    for ENSO
  • Schematics of ENSO (but with sense of how these
    connect to observations seen earlier)
  • Feedbacks that strengthen El Nino/La Nina
    (Bjerknes hypothesis feedbacks)
  • Linkage between sea surface height, thermocline
    depth, and pressure gradients in the upper ocean

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
46
December 1997 Anomalies of sea surface
temperatureduring the fully developed warm phase
of ENSO
Figure 1.7
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
47
Figure 4.2 (Chapter 4 preview)
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
48
The Bjerknes feedbacks (warm phase)
Figure 4.3
  • Positive feedback loop reinforces initial anomaly

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
49
Commonly used index regions for ENSO SST anomalies
Figure 1.5
  • When SST in the Niño-3 region is warm during El
    Niño, the SOI tends to be negative, i.e.,
    pressure is low in the eastern Pacific relative
    to the west.
  • Pressure gradient tends to produce anomalous
    winds blowing from west to east along the
    equator.
  • Reverse during periods of cold equatorial Pacific
    SST (La Niña).

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
50
Nino-3 index of equatorial Pacific sea surface
temperature anomalies and the Southern
Oscillation Index of atmospheric pressure
anomalies
Figure 1.6
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
51
December 1997 Anomalies of sea level
heightduring the fully developed warm phase of
ENSO
Figure 1.10
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
52
Idealized upper ocean layer
4.4 Pressure gradients in an idealized upper layer
Figure 4.4
  • Sea surface height ? thermocline depth cm vs.
    m
  • PGF from regions of deep thermocline (high sea
    surfacehigh pressure above thermocline) toward
    regions of shallower thermocline

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
53
Response of the ocean to a westerly wind anomaly
Re Onset and demise of El Niño warm phase
Figure 4.13
Wind anoms currents
  • To east of the wind anomalies, equatorial jet
    (Kelvin wave) extends east, deepening thermocline
    (H)
  • (recall warms SST)
  • To west, inflow of water to jet (in oc. upper
    layer) comes from off the equator (but little
    effect on SST)
  • shallow thermocline in west extends westward
    (Rossby wave), as mass transferred to east by jet
  • when reaches western boundary, can no longer
    supply mass by extending shallow region
  • Weakening of jet extends eastward, ending warm
    phase
  • As wind anomalies weaken, shallow thermocline
    extends eastward transition to cold phase

Deep Thermocline anoms
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
54
Two positions of the thermocline,
indicatingregion of thermocline anomalies
Figure 4.5
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
55
The transition into the 1997-98 El Niño warm
phase (Apr. 1997)
Figure 4.8b
Slowly evolving thermocline depth anomalies (
subsurface temperature anoms) affect eastern
Pacific SST later. Key to predictability.
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
56
The transition into the 1997-98 El Niño warm
phase (Sep. 1997)
Figure 4.8c
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
57
The transition into the 1997-98 El Niño warm
phase (Jan. 1998)
Figure 4.8d
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
58
Basis for ENSO forecasts and Limits to skill
  • weather unpredictable beyond two weeks
  • But interaction with the slowly evolving ocean
    (both in Bjerknes feedbacks and delayed effects
    of Western Pacific thermocline anomalies)
  • permits prediction of ENSO Eastern Pacific
    SST anomalies (and associated atmospheric
    anomalies) up to 9 months ahead
  • Forecast skill tends to degrade with longer lead
    time for forecast
  • Loss of skill in ENSO forecasts
  • Imperfections in the forecast system
  • -e.g., model errors, scarcity of input data (can
    be improved, if )
  • Fundamental limits to predictability
  • - weather noise acts like a random forcing
    on slow ocean-atmosphere interaction
  • e.g., SST gradient determines average strength
    of Tradewinds. But in a particular month,
    transient weather events can cause equatorial
    Easterlies to differ from this

Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
59
An ensemble of forecasts duringthe onset of the
1998-99 La Niña
  • Start coupled model from different ocean initial
    conditions (leading also to changes in atm. )
  • Initial differences grow Þ ensemble of prediction
    runs
  • Ensemble spread gives estimate of uncertainty
  • Spread tends to grow with time (due to weather
    noise coupled feedbacks)
  • Ensemble mean gives best estimate

Figure 4.18
Courtesy of the European Centre for Medium-range
Weather Forecasting.
Neelin, 2011. Climate Change and Climate
Modeling, Cambridge UP
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