Climate & Climatic Variation (Chapter 2). CLIMATE =. 1. Statistics of Weather. Daily Precipitation - Iowa/Nebraska. CLIMATE =. 1. Statistics of Weather. The expected weather + departures from expected weather. CLIMATE. Reflects the geophysical processes active at a location….
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Climate & Climatic Variation (Chapter 2)
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CLIMATE • Implies samples over a period of time. How long? How frequent? 2. WMO standard: 30 years • which 30? • paleoclimate? 3. There is no universal standard, but must define the interval for the topic at hand
Climatic Variation and Change Additional Factors • Abrupt change • external conditions (e.g., solar output) • internal feedbacks • passing a threshold (e.g. ice caps melting) 2. Multiple climate states from the same external conditions
The Climate System Three important controling factors: • Latitude - insolation • Elevation - temp. decrease with height • Closeness to oceans - heat reservoir
The Climate System Subsystems • Atmosphere - rapid changes • - links other subsystems • - greenhouse gases • Ocean • slow evolution (“memory”, “flywheel”) • chemical role, esp. CO2 • Land • - range of time scales • - cryosphere & biosphere roles • - location of continents
Solar Constant At photosphere surface, solar flux ~ 6.2.107 W-m-2
Solar Constant At photosphere surface, solar flux ~ 6.2.107 W-m-2 At Earth’s orbit, solar flux ~ 1360 W-m-2
Planetary Albedo Scattering: air molecules, aerosols Reflection: clouds Surface albedo
What is Earth’s temperature? Balance: Radiation in = Radiation out a Incoming = 1360 W-m-2 x (1-albedo) x (area facing sun) = 1360 x (1-0.3) x pa2 = 1.2.10+17 W
What is Earth’s temperature? Balance: Radiation in = Radiation out a Incoming = 1360 W-m-2 x (1-albedo) x (area facing sun) = 1360 x (1-0.3) x pa2 = 1.2.10+17 W Outgoing = sT4 x (area emitting) ; i.e., black body = sT4 x 4 pa2
What is Earth’s temperature? Balance: Radiation in = Radiation out a Incoming = 1360 W-m-2 x (1-albedo) x (area facing sun) = 1360 x (1-0.3) x pa2 = 1.2.10+17 W Outgoing = sT4 x (area emitting) ; (i.e., black body) = sT4 x 4 pa2 Balance implies T = {0.7(1360 W-m-2)/4s}1/4 = 255 K = -18 oC
What is Earth’s temperature? Balance: Radiation in = Radiation out a Balance implies T = -18 oC Observed surface T = +15 oC Difference? Must account for atmosphere (greenhouse effect).
What if temperature decreases? a These are the same: Incoming = 1.2.10+17 W Outgoing = sT4 x (area emitting) = sT4 x 4 pa2 • But for T < 255 K: • imbalance • Incoming solar exceeds outgoing IR • net energy input • T increases ~ Negative Feedback ~
Negative Feedback Perturb climate system Negative feedback moves climate back toward starting point A stabilizing factor
Greenhouse Effect IR radiation absorbed & re-emitted, partially toward surface Solar radiation penetrates
Greenhouse Effect IR radiation absorbed & re-emitted, partially toward surface Net IR: ~25-100 W-m Emitted IR: ~200-500 W-m
Greenhouse Effect Cooler atmosphere: - Less water vapor - Less IR radiation absorbed & re-emitted Solar radiation penetrates
Greenhouse Effect Cooler atmosphere: - thus less surface warming - cooler surface temperature Solar radiation penetrates
Positive Feedback Perturb climate system Positive feedback moves climate away from starting point A destabilizing factor Other examples (textbook): - ice-albedo feedback - CO2-ocean temperature feedback
Feedbacks Distinguish between: 1. external forcing change - e.g., insolation, volcanism - often predictable 2. Internal feedback mechanisms - nonlinear, coupled interactions - generally less predictable (stochastic)
Radiation Spectrum Black Body Curves Emission 255 K 6,000 K Wavelength [m] Solar (shortwave, visible) Terrestrial (longwave, infrared)