The Role of Mathematics in Understanding the Earth s Climate. Andrew Roberts

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Transcription:

The Role of Mathematics in Understanding the Earth s Climate Andrew Roberts

Outline What is climate (change)? History of mathematics in climate science How do we study the climate? Dynamical systems Large-scale (Atlantic) ocean circulation Ice ages and the mid-pleistocene transition Winter is coming?

Weather vs. Climate Conditions of the atmosphere over a short period of time (minutes - months) Temp, humidity, precip, cloud coverage (today) Snowfall on November 14, 2014 Heat wave in 2010 Hurricane How the atmosphere behaves over a long period of time Average of weather over time and space (usually 30-yr avg) Historical average November precipitation Record high temperature Average number and strength of tropical cyclones, annually

Weather vs. Climate Climate is what you expect, weather is what you get 0.4 0.3 Climate Weather 0.2 Can view climate as a probability distribution of possible weather 0.1-4 -2 2 4

What is Climate Change? 0.4 0.3 0.2 0.1-4 -2 2 4

What is Climate Change? 0.4 0.3 0.2 0.1-4 -2 2 4

What is Climate Change? 0.4 0.3 0.2 0.1-4 -2 2 4

What is Climate Change? 0.4 0.3 0.2 0.1-4 -2 2 4

Precipitation Dry areas get dryer, wet areas get wetter Climate scientists predict more floods and more droughts!

Mathematics and Climate Change T = Q(1 (T )) T 4 Energy balance equation Q : incoming solar radiation (1 (T )) : proportion absorbed by the Earth T 4 :heat re-radiated back to space

Energy Balance T =0) Q(1 (T )) = T 4 Radiation 400 350 300 250 200 150 100 200 220 240 260 280 300 T

Greenhouse Effect Joseph Fourier attempted to calculate the average temperature of the Earth (c. 1820) Hypothesized what has come to be known as the greenhouse effect something is trapping heat in the Earth s atmosphere 50 years before Stefan-Boltzmann energy balance equation 75 years before Arrhenius quantified how much colder the Earth should be

Greenhouse Effect Radiation 400 350 300 250 200 150 100 T = Q(1 (T )) " T 4 50 220 240 260 280 300 T

Energy Balance Cartoon

Ice Ages Mid-1700s: speculation that ice ages exists 1830s: A few geologists claim ice-ages happend, ideas rejected 1842: Joseph Adhémar (mathematician) is first to propose ice-ages caused by variation in solar radiation

Ice Ages 1870s: Geologists reach consensus that ice-ages occurred (James Croll) 1912-1924: Milutin Milankovic Eccentriciy (100 kyr) Kepler 1609 Obliquity/Axial tilt (41 kyr) Milankovic 1912 Precession (23 kyr) Hipparchus 130 B.C.

Milankovic Cycles

Snowball Earth @T(y) @t = Qs(y)(1 (y, )) (A + BT(y)) C(T (y) T ( )) Budyko and Sellers (1969) describe spatially dependent energy balance model Assume Northern and Southern hemisphere symmetric Assume temperature is the same for fixed latitude (y) Includes energy transport term

Snowball Earth 2 stable states of ice coverage: Warm climate (like now - and even ice ages) Snowball climate (entire Earth covered in ice) Dismissed as mathematical artifact until 1990s New consensus: 3 snowball events (all over 600 myr ago)

How do we study the climate?

How do we study the climate?

How do we study the climate?

How do we study the climate? Models!

Model Hierarchies

Conceptual Models Examples: Energy balance models Typically model 1 or 2 processes/phenomena Large-scale average behavior Help explain climate to nonexperts Motivate large experiments Pros: Simple enough to be analyzed by a person Can explore all possibilities Intuition Cons: Too simple to prove scientific results definitively Adding more processes could destroy phenomenon

Intermediate Complexity and Process Models Some spatial resolution More processes (but not too many) Simple enough for some interpretation Too complex to analyze by hand

GCMs and ESMs Too complicated to interpret causality Too complicated to explore all possibilities (where do we look?) Millions of lines of code (bugs?) Expensive (financially and computationally) Treated as experimental Earths Useful for prediction*

Weather Prediction Observation of Current State Model

Weather Prediction Observation of Current State Model Prediction (1 hour)

Weather prediction Observation of Current State Model Model Prediction (1 hour) Prediction (2 hour)

Observations have error Observed state Actual (initial) state

Error grows Observed state State after 1 hr Model Actual (initial) state 1 hour prediction

and grows Observed state State after 1 hr State after 2 hr Actual (initial) state Model 1 hour prediction Model 2 hour prediction

Lorenz Butterly

Climate Prediction

Climate Prediction

Climate Prediction

Climate Prediction Where do observations come in?

Confronting Models with Data

Confronting Models with Data Model 1st IC Data

Confronting Models with Data Model 1st IC Data

Data Assimilation Model 1st IC Data 2nd IC

Data Assimilation 1st IC Model Data 2nd IC Model (w/o DA) Model (w/ DA) Data

Data Assimilation Model 1st IC Data 2nd IC Data

The Role of Mathematics in Climate Science Field Lab Observation Data Theory Simulations as Experiments ESMs GCMs Conceptual Models Math

Dynamical Systems Derivative (from Calculus) dx dt = f(t) Example dx dt = t3 x(t) = t4 4 t + k t 2 2 + kt + C

Dynamical Systems Derivative (from Calculus) dx dt = f(t) Example dx dt = t3 t + k What if dx dt = f(x)?

More than one variable? System of Differential Equations ẋ = f(x, y) ẏ = g(x, y) Defines a Vector Field

Vector Fields System of Differential Equations 3 ẋ = y ẏ = x x 3 + x 2y + k 2 1 0-1 Defines a Vector Field -2-3 -3-2 -1 0 1 2 3

Equilibrium Points ẋ = y ẏ = x x 3 + x 2y + k 3 2 Equilibrium points occur when ẋ =0 ẏ =0 1 0-1 -2-3 -3-2 -1 0 1 2 3

Solutions ẋ = y ẏ = x x 3 + x 2y + k 3 2 1 Even if equations can t be solved, we can understand 0-1 -2-3 Qualitative Behavior -3-2 -1 0 1 2 3

Varying k ẋ = y x 3 + x ẏ = x 2y +0 ẋ = y x 3 + x ẏ = x 2y 2 3 3 2 2 1 1 0 0-1 -1-2 -2-3 -3-3 -2-1 0 1 2 3-3 -2-1 0 1 2 3

Quadratic equation ax 2 + bx + c =0 Bifurcation in Algebra I

Quadratic equation Bifurcation in Algebra I ax 2 + bx + c =0 Bifurcation parameter: Discriminant b 2 4ac > 0 2 Real Roots 10 5-4 -2 2 4

Bifurcation in Algebra I Quadratic equation ax 2 + bx + c =0 Bifurcation parameter: Discriminant b 2 4ac > 0 2 Real Roots No qualitative change for small change in equation 15 10 5-4 -2 2 4-5

Bifurcation in Algebra I Quadratic equation ax 2 + bx + c =0 Bifurcation parameter: Discriminant b 2 4ac < 0 0 Real Roots Big enough change in system leads to qualitatively different solutions 15 10 5-4 -2 2 4-5

Bifurcation in Algebra I Quadratic equation ax 2 + bx + c =0 Bifurcation parameter: Discriminant b 2 4ac =0 1 Real Root Bifurcation occurs when solutions collide 20 15 10 5-4 -2 2 4

Bifurcations as Tipping Points

Bifurcations as Tipping Points

Bifurcations as Tipping Points

Bifurcations as Tipping Points

Hysteresis

Bifurcation vs. Intrinsic Dynamics Idea of bifurcations assumes modeler has control over how parameters change i.e., do NOT depend on state of system Snowball Earth: bifurcation parameter depends on GHGs (which in turn depend on temperature and ice) How does behavior change?

Fast/Slow Dynamics Fast variable is like state of system as before Slow variable is acts partly like parameter, partly like state variable Example of parameter: Milankovic cycles depend only on time (influence climate, but not influenced by climate) Examples of slow variable: GHGs, Ice coverage ẋ = f(x; ) (t) = g(t) ẋ = f(x, y) ẏ = "g(x, y) " 1

Picturing the difference ẋ = f(x; ) (t) = g(t) ẋ = f(x, y) ẏ = "g(x, y) " 1 λ 2 y 2 1 1-4 -2 2 4 x -4-2 2 4 x -1-1 -2-2

Example in Ocean Circulation

Stommel s Circulation Model Circulation variable:

Stommel s Circulation Model Model Reduces: x T e Tp! 1 Get one state variable: y S e S p Bifurcation parameter: µ SA T A ẏ = µ y A 1 y y

µ! slow variable ẏ = µ y A 1 y y µ = 0 ( y)

Mixed-mode Oscillations 2D dynamical systems can have up to 3 end states: Fixed equilibrium Periodic equilibrium (with fixed amplitude and period) Run-away behavior MMOs have big and small oscillations need 3D system! 3D dynamics much more complicated (chaos)

Ice Ages over the last 400 kyr ẋ = y x 3 +3x k ẏ = "[p(x a) 2 b my ( + y z)] ż = "r( + y z)

Ice Ages over the last 400 kyr ẋ = y x 3 +3x k ẏ = "[p(x a) 2 b my ( + y z)] ż = "r( + y z) x ice volume z oceanic carbon y atmospheric carbon

Ice Ages over the last 400 kyr ẋ = y x 3 +3x k ẏ = "[p(x a) 2 b my ( + y z)] ż = "r( + y z) Fast Slow

Ice Ages over the last 400 kyr ẋ = y x 3 +3x k ẏ = "[p(x a) 2 b my ( + y z)] ż = "r( + y z) Change in ice volume depends on temperature, but temperature depends on the amount of ice and how much GHGs are in the atmosphere

Ice Ages over the last 400 kyr ẋ = y x 3 +3x k ẏ = "[p(x a) 2 b my ( + y z)] ż = "r( + y z) Land-atmosphere carbon flux

Ice Ages over the last 400 kyr ẋ = y x 3 +3x k ẏ = "[p(x a) 2 b my ( + y z)] ż = "r( + y z) Ocean-atmosphere carbon flux

Ice Ages over the last 400 kyr

Ice Ages over the last 400 kyr

Ice Ages over the last 400 kyr

Ice Ages over the last 400 kyr

Ice Ages over the last 400 kyr

El Niño-Southern Oscillation

How does ENSO work?

The Data

Predicting ENSO August predictions

Predicting ENSO August Prediction? September prediction Probability of ENSO: low October Prediction Probability of ENSO: 0.68 November Prediction 58% chance of ENSO Normal to weak ENSO

ENSO ẋ = "(x 2 ax)+x apple x + y nz + d c x x 3 3 ẏ = "(ay + x 2 ) x ż = m k z 2

ENSO ẋ = "(x 2 ax)+x apple x + y nz + d c x x 3 3 ẏ = "(ay + x 2 ) x ż = m k z 2 x temperature gradient y z temp of W Pacific thermocline dept in W Pacific

ENSO ẋ = "(x 2 ax)+x apple x + y nz + d c x x 3 3 ẏ = "(ay + x 2 ) x ż = m k z 2 Upwelling feedback

ENSO ẋ = "(x 2 ax)+x apple x + y nz + d c x x 3 3 ẏ = "(ay + x 2 ) x ż = m k z 2 Thermocline adjustment

ENSO ẋ = "(x 2 ax) + x apple x + y nz + d c x x 3 3 ẏ = "(ay + x 2 ) x ż = m k z 2 Advection

ENSO

Simulation 1

Simulation 1

Simulation 2

Simulation 2

Model Output

Winter?