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Ch04
1.
Chapter 4: Insolation
and Temperature McKnight’s Physical Geography: A Landscape Appreciation, Tenth Edition, Hess
2.
© 2011 Pearson
Education, Inc. Insolation and Temperature • The Impact of Temperature on the Landscape • Energy, Heat, and Temperature • Basic Heating and Cooling Processes in the Atmosphere • The Heating of the Atmosphere • Variations in Heating by Latitude and Season • Land and Water Contrasts 2© 2011 Pearson Education, Inc.
3.
© 2011 Pearson
Education, Inc. Insolation and Temperature • Mechanisms of Heat Transfer • Vertical Temperature Patterns • Global Temperature Patterns • Global Warming and the Greenhouse Effect 3
4.
© 2011 Pearson
Education, Inc. The Impact of Temperature on the Landscape • All living things influenced by temperature • Adaptation to temperature extremes • Affects soil and bedrock exposure 4 Figure 4-1b Figure 4-1a
5.
© 2011 Pearson
Education, Inc. Energy, Heat, and Temperature • Definition of energy • Forms of energy – Chemical – Kinetic – Potential – Nuclear – Others • Kinetic energy—energy of movement 5
6.
© 2011 Pearson
Education, Inc. Energy, Heat, and Temperature • Definition of temperature • Measuring temperature • Temperature scales – Celsius – Fahrenheit – Kelvin – Conversions between scales 6 Figure 4-2
7.
© 2011 Pearson
Education, Inc. Energy, Heat, and Temperature • The Sun • Primary source of energy for Earth’s atmosphere • Properties of Sun – Average size star – Nuclear fusion – Magnitude of Sun’s energy • Energy spreads as it leaves the Sun 7 Figure 4-3
8.
© 2011 Pearson
Education, Inc. Energy, Heat, and Temperature • Electromagnetic energy • Electromagnetic spectrum • Wavelengths • Three important areas on the spectrum – Visible radiation – Ultraviolet radiation – Infrared radiation • Shortwave solar radiation, insolation 8 Figure 4-5
9.
© 2011 Pearson
Education, Inc. Basic Heating and Cooling Processes in the Atmosphere • Radiation – Definition – Warmer objects radiate more effectively – Warmer objects emit at shorter wavelengths – Sun ultimate “hot” body in Solar System – Blackbody radiators 9
10.
© 2011 Pearson
Education, Inc. Basic Heating and Cooling Processes in the Atmosphere • Radiative processes • Absorption – Body absorbs radiation – Good radiator, good absorber • Reflection – Objects repel electromagnetic waves – Opposite of absorption 10 Figure 4-7
11.
© 2011 Pearson
Education, Inc. Basic Heating and Cooling Processes in the Atmosphere • Scattering – Deflection of light waves by molecules and particles • Transmission – Electromagnetic waves pass completely through a medium – Sunsets 11 Figure 4-9
12.
© 2011 Pearson
Education, Inc. Basic Heating and Cooling Processes in the Atmosphere • Greenhouse effect • Some atmospheric gases transmit shortwave radiation, but not Earth’s longwave radiation • Earth radiation held in by atmosphere • Atmospheric blanket 12 Figure 4-12
13.
© 2011 Pearson
Education, Inc. Basic Heating and Cooling Processes in the Atmosphere • Other heating types • Conduction – Transfer of heat energy across a medium – Results from molecular collision – Air is a poor conductor 13 Figure 4-13
14.
© 2011 Pearson
Education, Inc. Basic Heating and Cooling Processes in the Atmosphere • Convection – Heat transfer by vertical circulation – Molecules move in tandem – Convection cell • Advection – Horizontal transfer of heat in a moving fluid 14 Figure 4-14
15.
© 2011 Pearson
Education, Inc. Basic Heating and Cooling Processes in the Atmosphere • Adiabatic cooling – Air rises and expands, molecular collisions decrease, so temperature decreases • Adiabatic warming – Air sinks and compresses, collisions increase so temperatures increase 15 Figure 4-15
16.
© 2011 Pearson
Education, Inc. Basic Heating and Cooling Processes in the Atmosphere • Latent heat – Heat released or absorbed during a phase change – “Latent” since heat is not felt – Most common phase changes: • Evaporation • Condensation 16
17.
© 2011 Pearson
Education, Inc. The Heating of the Atmosphere • Balance between shortwave incoming solar radiation and outgoing longwave solar radiation • Some shortwave radiation reflected by atmosphere or surface • Albedo 17 Figure 4-16
18.
© 2011 Pearson
Education, Inc. The Heating of the Atmosphere • Global energy budget 18 Figure 4-17
19.
© 2011 Pearson
Education, Inc. Variations in Heating by Latitude and Season • Angle of incidence • Atmospheric obstructions • Day length • Latitudinal radiation balance 19 Figure 4-18
20.
© 2011 Pearson
Education, Inc. Variations in Heating by Latitude and Season • World distribution of insolation 20 Figure 4-21
21.
© 2011 Pearson
Education, Inc. Land and Water Contrasts • Land heats and cools more rapidly than water due to: – Specific heat – Transmission – Mobility – Evaporative cooling 21 Figure 4-23
22.
© 2011 Pearson
Education, Inc. Land and Water Contrasts • Implications 22 Figure 4-24
23.
© 2011 Pearson
Education, Inc. Mechanisms of Heat Transfer • Need heat transfer to prevent constant warming at tropics and cooling at poles • Circulation patterns in atmosphere and oceans transfer heat 23
24.
© 2011 Pearson
Education, Inc. Mechanisms of Heat Transfer • Atmospheric circulation – General circulation Ch. 5 • Oceanic circulation – Respond to average wind conditions over long time scales – Subtropical gyres 24 Figure 4-25
25.
© 2011 Pearson
Education, Inc. Mechanisms of Heat Transfer • Northern and southern variations – Near Northern Hemisphere pole, landmasses lie so close that little flow can enter the Arctic Ocean – Effect more pronounced in northern Pacific than northern Atlantic – In Southern Hemisphere, little land mass allows for constant westward belt of ocean circulation, the West Wind Drift 25
26.
© 2011 Pearson
Education, Inc. Mechanisms of Heat Transfer • Temperature patterns – Low-latitude currents are warm – Poleward currents transfer warm water poleward – High-latitude currents transfer warm water to the east in Northern Hemisphere; cool water east in Southern Hemisphere – Equatorial currents transfer cool water equatorward • Westward intensification 26
27.
© 2011 Pearson
Education, Inc. Mechanisms of Heat Transfer • Rounding out the pattern – Northwestern portions of Northern Hemisphere receive cool water from Arctic Ocean – Water pulled away from western coasts of continents results in upwelling – Deep ocean circulation 27 Figure 4-26
28.
© 2011 Pearson
Education, Inc. Vertical Temperature Patterns • Definition of lapse rate • Environmental lapse rate • Average lapse rate (about 6.5°C/km) • Temperature inversions – Surface inversions – Upper air inversions 28 Figure 4-27
29.
© 2011 Pearson
Education, Inc. Global Temperature Patterns • Primary controls on global temperature – Altitude – Latitude – Land–Water contrasts – Ocean currents 29 Figure 4-29 – average January temperature Figure 4-30 – average July temperature
30.
© 2011 Pearson
Education, Inc. Global Temperature Patterns • Seasonal patterns – Latitudinal shift in isotherms from one season to another – More pronounced over continents than water and over high latitudes than low latitudes 30 Figure 4-31
31.
© 2011 Pearson
Education, Inc. Global Temperature Patterns • Annual temperature range – Difference in average temperature of warmest and coldest months 31 Figure 4-32
32.
© 2011 Pearson
Education, Inc. Global Warming and the Greenhouse Effect • Climate of Earth is becoming warmer, known as global warming • Human-enhanced greenhouse effect • Carbon dioxide main culprit • Also methane, nitrous oxide • Intergovermental Panel on Climate Change 32 Figure 4-33
33.
© 2011 Pearson
Education, Inc. Global Warming and the Greenhouse Effect • Relationship between carbon dioxide and temperature 33 Figure 4-35
34.
© 2011 Pearson
Education, Inc. Summary • Temperature affects both living and nonliving aspects of Earth’s landscape • Energy exists in many different forms, but cannot be created or destroyed • Temperature is a measure of the amount of kinetic energy in the molecules of a substance • Temperature is measured on three primary scales • The Sun is the primary source of energy for Earth’s atmosphere • Electromagnetic radiation is classified by wavelength 34
35.
© 2011 Pearson
Education, Inc. Summary • The Sun emits three important types of electromagnetic radiation: visible, infrared, and ultraviolet • Insolation refers to incoming solar radiation • Radiation is the process by which electromagnetic radiation is emitted by an object • Radiation can undergo several processes, including absorption, reflection, transmission, and scattering • The greenhouse effect makes Earth able to support life 35
36.
© 2011 Pearson
Education, Inc. Summary • Conduction is the transfer of heat through molecular collision • Convection is a vertical transport of heat in a fluid • Advection is the horizontal transport of heat • Adiabatic cooling and warming processes do not release or absorb heat • The global radiation budget describes the latitudinal distribution of temperature • Land surfaces heat and cool faster than water surfaces 36
37.
© 2011 Pearson
Education, Inc. Summary • Heat is transferred globally through atmospheric and oceanic circulations • The vertical temperature patterns in the atmosphere help describe vertical circulations • Global warming is the observed warming of the atmosphere • Temperature and carbon dioxide show a close relationship 37
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