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AMS Weather Studies Introduction to Atmospheric Science, 5 th Edition Chapter 4 Heat, Temperature, & Atmospheric Circulation © AMS
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What are the causes and consequences of heat transfer within the Earth-atmosphere system? This chapter covers: Distinguishing temperature and heat Heat transfer processes Thermal response and specific heat Heat imbalances How does heat affect atmospheric circulation? © AMS2 Driving Question
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Case-in-Point Extreme Heat of Death Valley, CA © AMS3 Death Valley – Hottest and driest place in North America 134°F in 1913 2nd highest temperature ever recorded on Earth Summer 1996 40 successive days over 120°F 105 successive days over 110°F Causes: Topographic setting Atmospheric circulation Intense solar radiation Cooperative Weather observing station at Furnace Creek Ranch
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© AMS4 All matter is composed of molecules or particles in continual vibrational, rotational, and/or translational motion. Energy represented by this motion is called kinetic energy. Temperature Directly proportional to the average kinetic energy of atoms or molecules composing a substance Internal energy Encompasses all the energy in a substance Includes kinetic energy Includes potential energy, arising from forces between atoms/molecules Heat is energy in transit When two substances are brought together with different kinetic energy, energy is always transferred from warmer object to colder Distinguishing Temperature & Heat
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© AMS5 Temperature Scales Absolute zero Temperature at which theoretically all molecular motion ceases No electromagnetic radiation is emitted Absolute zero = -459.67°F = 273.15°C = 0 K Distinguishing Temperature & Heat
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© AMS6 Temperature scales measure degree of hotness or coldness Calorie Amount of heat required to raise temperature of 1 gram of water 1 Celsius degree Different from “food” calorie, which is actually 1 kilocalorie Joule More common in meteorology today 1 calorie = 4.1868 joules British Thermal Units (BTU) Amount of energy required to raise 1 pound of water 1 Fahrenheit degree 1 BTU = 252 cal = 1055 J Distinguishing Temperature & Heat
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© AMS 7 Thermometer Liquid-in-glass thermometer Uses mercury or alcohol Bimetallic thermometer Two strips of metal with different expansion/contraction rates Electrical resistance thermometer Thermograph Measures and records temperature Bilmetallic thermometer The change of temperature during the passage of a cold front as determined by an electronic thermometer. Distinguishing Temperature & Heat Liquid-in-glass thermometer
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© AMS8 Shielding temperature sensors Important properties Accuracy Response time Location is important Ventilated Shielded from weather Enclosure for the NWS electronic temperature sensor Distinguishing Temperature & Heat
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© AMS9 Temperature gradient Change in temperature over distance Example: the hot equator and cold poles Heat flows in response to a temperature gradient This is the 2 nd law of thermodynamics Heat flows toward lower temperature so as to eliminate the gradient Heat flows/transfers in the atmosphere Radiation Conduction Convection Latent heat – phase changes in water Heat Transfer Processes
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© AMS10 Heat Transfer Processes Radiation Both a form of energy and a means of energy transfer Occurs even in a vacuum, such as space Absorption of radiation by an object causes the temperature of object to rise Converts electromagnetic energy to heat Radiational heating Absorption at greater rate than emission Radiational cooling Emission at greater rate than absorption
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© AMS11 Conduction Transfer of kinetic energy of atoms or molecules by collision between neighboring atoms or molecules Heat conductivity Rate of heat transport across an area to a temperature gradient Some materials have a higher heat conductivity than others Solids (metal) are better conductors than liquids Liquids are better than gases (air) Conductivity impaired by trapped air Examples: fiberglass insulation, thick layer of fresh snow Heat Transfer Processes
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© AMS12 A thick layer of snow is a good insulator because of air trapped between individual snowflakes. As snow settles, the snow cover’s insulating property diminishes. Heat Transfer Processes
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© AMS13 Convection Consequence of differences in air density Transport of heat within a substance via movement of substance itself Substance must liquid or gas Very important process for transferring heat in atmosphere The convection cycle Ascending warm air expands, cools and eventually sinks back to ground Heat Transfer Processes
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Latent heating Movement of heat from one location to another due to phase changes of water Example: evaporation of water, movement of vapor by winds, condensation elsewhere © AMS14 Heat Transfer Processes
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Temperature change caused by input/output of a quantity of heat varies among substances Specific heat The amount of heat required to raise 1 gram of a substance 1 Celsius degree Thermal Response and Specific Heat © AMS15 The contrast in specific heat is one reason why the sand is hotter than the water.
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© AMS16 Thermal inertia Resistance to a change in temperature Large body of water exhibits greater resistance to temperature change than land because of difference in specific heat Maritime climate Immediately downwind of the ocean experience much less annual temperature change Continental climate Locations well inland experience greater annual temperature change Thermal Response and Specific Heat San Francisco, CA, has a maritime climate while St. Louis, MO, has a continental climate.
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© AMS17 Heat Imbalance: Atmosphere vs. Earth’s Surface At Earth’s surface Absorption of solar radiation is greater than emission of IR In atmosphere Emission of IR radiation to space is greater than absorption of solar radiation Therefore, Earth’s surface has net radiational heating Atmosphere has net radiational cooling. So, Earth’s surface transfers heat to the atmosphere, making up difference
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© AMS18 Heat Imbalance: Atmosphere vs. Earth’s Surface
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© AMS19
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© AMS20 Heat Imbalance: Atmosphere vs. Earth’s Surface Latent Heating Some absorbed solar radiation used to vaporize water at Earth’s surface. Energy released to the atmosphere when clouds form Comparatively, large amounts of heat needed for phase changes of water Sensible Heating Heat transfer via conduction and convection that can be sensed by temperature change and measured by a thermometer
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© AMS21 Heat Imbalance: Atmosphere vs. Earth’s Surface
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© AMS22 Sensible heating, in the form of convectional uplifts, can combine with latent heating, through condensation, to channel heat from Earth’s surface into the troposphere Produces cumulus clouds If it continues vertically, cumulonimbus clouds form Heat Imbalance: Atmosphere vs. Earth’s Surface
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Bowen Ratio Describes how energy received at the Earth’s surface is partitioned between sensible heating and latent heating Bowen ratio = [(sensible heating)/(latent heating)] At the global scale, this is [(7 units)/(23 units)] = 0.3 © AMS23 Heat Imbalance: Atmosphere vs. Earth’s Surface
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© AMS24 Surface energy budget through the course of a year at Yuma, AZ and Madison, WI. R = net radiation absorbed H = sensible heating LE = latent heating G = storage
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Heat Imbalance: Tropics vs. Middle and High Latitudes Earth’s surface unevenly heated due to higher solar altitudes in the tropics than higher latitudes Causes a temperature gradient, resulting in heat transfer Poleward heat transport Air mass exchange Storms Ocean currents © AMS25
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© AMS26 Heat Imbalance: Tropics vs. Middle and High Latitudes Heat transport by air mass exchange North-south exchange of air masses transports sensible heat from the tropics into middle and high latitudes Air mass properties of depend on source region Modify as they move Heat transport by storms Tropical storms and hurricanes are greater contributors to poleward heat transport than middle latitude cyclones
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© AMS27 The Gulf Stream flows along the East Coast from Florida to the Delaware coast. Heat transport by ocean circulation Contributes via wind-driven surface currents and thermohaline circulation Thermohaline circulation is density- driven movement of water masses Transports heat energy, salt, and dissolved gases over great distances and depths Meridional overturning circulation (MOC) At high latitudes, surface waters cool and sink, then flow southward as cold bottom water Heat Imbalance: Tropics vs. Middle and High Latitudes
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© AMS28 Imbalances in radiational heating/cooling create temperature gradients Earth’s surface the troposphere Low and high latitudes Heat transported in the Earth-atmosphere system to reduce temperature differences Cause-and-effect chain starts with the Sun, ends with weather Some solar radiation is absorbed (converted to heat), some to converted to kinetic energy Causes winds, convection currents, and north-south exchange of air masses Rate of heat redistribution varies by season Causes seasonal weather and air circulation changes Why Weather?
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© AMS29 Radiational controls Factors that affect local radiation budget and air temperature Time of day and time of the year Solar altitude and duration of radiation Cloud cover Surface characteristics Annual temperature cycle represents these variations Annual temperature maximums and minimums do not occur at exact max/min of solar radiation, especially in middle and high latitudes The atmosphere takes time to heat and cool Average lag time in US = 27 days Up to 36 days with the maritime influence Variation of Air Temperature
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© AMS30 Variation of Air Temperature
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© AMS31 Daily temperature cycle Lowest temperature usually occurs just after sunrise Based on radiation alone, minimum temperature would occur after sunrise when incoming radiation becomes dominant Highest temperature usually occurs in the early to middle afternoon Even though peak of solar radiation is around noon, imbalance in favor of incoming vs. outgoing radiation continues so the atmosphere also continues to warm Variation of Air Temperature
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© AMS32 Variation of Air Temperature Daily Temperature Cycle
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© AMS33 Surface cover Dry soil heats more rapidly than moist Less energy used to evaporate water Especially in drought, energy used only to heat soil, soil becomes hotter Relative humidity also affects evaporation Snow High albedo Less energy absorbed by the surface or converted to heat Snow reduces sensible heating of overlying air Some of the available heat is used to vaporize snow Snow is an excellent infrared radiation emitter Nocturnal radiational cooling is extreme When skies are clear, or light winds or calm conditions Variation of Air Temperature
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© AMS 34 Variation of Air Temperature Air mass advection Horizontal movement of an air mass from one location to another Cold air advection (A) Horizontal movement of colder air into a warmer area Warm air advection (B) Horizontal movement of warmer air into a colder area Significance of air mass advection to local temperature Initial temperature of the air new mass Degree of modification the air mass as travels over the Earth’s surface
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© AMS35 Variation of Air Temperature Urban heat island effect City of warmth surrounded by cooler air In a city: Relative lack of moisture Absorbed heat raises temperature (not for evaporation) Greater concentration of heat sources (cars, air conditioners, etc) Multiple reflections and lower albedo Building materials conduct heat more readily than soil and vegetation Develops best on nights when air is calm and sky is clear
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© AMS36 Variation of Air Temperature Satellite-produced maps of Providence, RI (top) and Buffalo, NY (bott0m) highlighting the role that differences in development patterns/vegetation cover can have on a city’s urban heat island. Providence has a significantly stronger heat island signature. Buffalo, NY Providence, RI
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