summary of lecture 1

29
Summary of Lecture 1 • Introduction to Earth’s atmosphere – origin – composition – structure – comparison with other planets • Stefan’s law 4 4 1 s T S

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Summary of Lecture 1. Introduction to Earth’s atmosphere origin composition structure comparison with other planets Stefan’s law. Solar and Terrestrial Radiation. Sun ~ 6000 K UV/vis λ max ~0.6 μ m Solar flux =1370 Wm -2 S (1- α )/4= σ T E 4 Earth ~ 255 K IR λ max ~ 12 μ m. - PowerPoint PPT Presentation

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Page 1: Summary of Lecture 1

Summary of Lecture 1

• Introduction to Earth’s atmosphere– origin– composition– structure– comparison with other planets

• Stefan’s law

44 1sT S

Page 2: Summary of Lecture 1

Solar and Terrestrial Radiation

Sun ~ 6000 K

UV/vis max~0.6m

Solar flux =1370 Wm-2

S (1-)/4=TE4

Earth ~ 255 K

IR max~ 12m

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UV absorptionInfraRed

UVa /Visible

UVb

UVc

DUV

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Absorption by atmospheric gases

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Radiation Balance

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Notes:• Surface has Ts=288 K and radiates Ts

4 = 400 Wm-2 (117 units).

• Atmosphere at 250 K radiates 220 Wm-2 (64 units), both up and down.

• 30% of surface radiation is reflected by the atmosphere (32 units), giving a total downward flux of 96 units.

• Non-radiative flux of 100 Wm-2 (30 units) drives the atmospheric circulation and weather

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Seasonal net IR radiation

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Global Climate

Net short, long and global radiation entering and leaving the top of our atmosphere measured by satellite.

Data are from the Earth Radiation Budget Experiment (ERBE)

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Global Warming

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Global temperatures 1880-2015

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Change in extent of Arctic sea ice

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Rising CO2 levels

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0

50

100

150

200

250

300

350

1990 2000 2010 2020 2030 2040 2050 2060 2070 2080 2090 2100

700

600

500

400

350

CO

2 c

on

cen

trati

on

p

pm

Carbon dioxide concentrationin the atmosphere, due to three emissions scenarios

Business as usual emissionsConstant 1990 emissions50% reduction in emissions

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Global temperature riseG

lob

al t

em

pe

ratu

re r

ise,

deg

ree

s C IPCC A1FI emissions

A2 emissionsB2 emissionsB1 emissions

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Components of sea-level rise

Hadley Centre

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Pattern of annual temperature changes

2080s relative to present dayA1FI emissions scenario

0 1 2 3 4 5 6

Met Office / Hadley Centre

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Temperature riseMedium-high emissions scenario, 2080s

winter summer

°C

Hadley Centre Hadley Centre

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Pattern of annual precipitation changes

2080s relative to present day

–3 –2 –1 1 2 3–0.5 0.5–0.25 0.250

A1FI emissions scenarioMet Office / Hadley Centre

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Change in precipitation

%

winter summer

Medium-high emissions scenario, 2080s

Hadley Centre Hadley Centre

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Change in surface temperature with forced THC collapse, but without change in greenhouse

gases

Deg C

Hadley Centre