Atmospheric Thermodynamics
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3-1 Adiabatic Compression
Solution Physics 213 Problem 1 Week 3 Adiabatic Compression a) Last week, we considered the problem of isothermal compression: 1.5 moles of an ideal diatomic gas at temperature 35oC were compressed isothermally from a volume of 0.015 m3 to a volume of 0.0015 m3. The pV-diagram for the isothermal process is shown below. Now we consider an adiabatic process, with the same starting conditions and the same final volume. Is the final temperature higher, lower, or the same as the in isothermal case? Sketch the adiabatic processes on the p-V diagram below and compute the final temperature. (Ignore vibrations of the molecules.) α α For an adiabatic process ViTi = VfTf , where α = 5/2 for the diatomic gas. In this case Ti = 273 o 1/α 2/5 K + 35 C = 308 K. We find Tf = Ti (Vi/Vf) = (308 K) (10) = 774 K. b) According to your diagram, is the final pressure greater, lesser, or the same as in the isothermal case? Explain why (i.e., what is the energy flow in each case?). Calculate the final pressure. We argued above that the final temperature is greater for the adiabatic process. Recall that p = nRT/ V for an ideal gas. We are given that the final volume is the same for the two processes. Since the final temperature is greater for the adiabatic process, the final pressure is also greater. We can do the problem numerically if we assume an idea gas with constant α. γ In an adiabatic processes, pV = constant, where γ = (α + 1) / α. -
Thermodynamics Formulation of Economics Burin Gumjudpai A
Thermodynamics Formulation of Economics 306706052 NIDA E-THESIS 5710313001 thesis / recv: 09012563 15:07:41 seq: 16 Burin Gumjudpai A Thesis Submitted in Partial Fulfillment of the Requirements for the Degree of Master of Economics (Financial Economics) School of Development Economics National Institute of Development Administration 2019 Thermodynamics Formulation of Economics Burin Gumjudpai School of Development Economics Major Advisor (Associate Professor Yuthana Sethapramote, Ph.D.) The Examining Committee Approved This Thesis Submitted in Partial 306706052 Fulfillment of the Requirements for the Degree of Master of Economics (Financial Economics). Committee Chairperson NIDA E-THESIS 5710313001 thesis / recv: 09012563 15:07:41 seq: 16 (Assistant Professor Pongsak Luangaram, Ph.D.) Committee (Assistant Professor Athakrit Thepmongkol, Ph.D.) Committee (Associate Professor Yuthana Sethapramote, Ph.D.) Dean (Associate Professor Amornrat Apinunmahakul, Ph.D.) ______/______/______ ABST RACT ABSTRACT Title of Thesis Thermodynamics Formulation of Economics Author Burin Gumjudpai Degree Master of Economics (Financial Economics) Year 2019 306706052 We consider a group of information-symmetric consumers with one type of commodity in an efficient market. The commodity is fixed asset and is non-disposable. We are interested in seeing if there is some connection of thermodynamics formulation NIDA E-THESIS 5710313001 thesis / recv: 09012563 15:07:41 seq: 16 to microeconomics. We follow Carathéodory approach which requires empirical existence of equation of state (EoS) and coordinates before performing maximization of variables. In investigating EoS of various system for constructing the economics EoS, unexpectedly new insights of thermodynamics are discovered. With definition of truly endogenous function, criteria rules and diagrams are proposed in identifying the status of EoS for an empirical equation. -
Thermodynamics of Power Generation
THERMAL MACHINES AND HEAT ENGINES Thermal machines ......................................................................................................................................... 1 The heat engine ......................................................................................................................................... 2 What it is ............................................................................................................................................... 2 What it is for ......................................................................................................................................... 2 Thermal aspects of heat engines ........................................................................................................... 3 Carnot cycle .............................................................................................................................................. 3 Gas power cycles ...................................................................................................................................... 4 Otto cycle .............................................................................................................................................. 5 Diesel cycle ........................................................................................................................................... 8 Brayton cycle ..................................................................................................................................... -
ESCI 241 – Meteorology Lesson 8 - Thermodynamic Diagrams Dr
ESCI 241 – Meteorology Lesson 8 - Thermodynamic Diagrams Dr. DeCaria References: The Use of the Skew T, Log P Diagram in Analysis And Forecasting, AWS/TR-79/006, U.S. Air Force, Revised 1979 An Introduction to Theoretical Meteorology, Hess GENERAL Thermodynamic diagrams are used to display lines representing the major processes that air can undergo (adiabatic, isobaric, isothermal, pseudo- adiabatic). The simplest thermodynamic diagram would be to use pressure as the y-axis and temperature as the x-axis. The ideal thermodynamic diagram has three important properties The area enclosed by a cyclic process on the diagram is proportional to the work done in that process As many of the process lines as possible be straight (or nearly straight) A large angle (90 ideally) between adiabats and isotherms There are several different types of thermodynamic diagrams, all meeting the above criteria to a greater or lesser extent. They are the Stuve diagram, the emagram, the tephigram, and the skew-T/log p diagram The most commonly used diagram in the U.S. is the Skew-T/log p diagram. The Skew-T diagram is the diagram of choice among the National Weather Service and the military. The Stuve diagram is also sometimes used, though area on a Stuve diagram is not proportional to work. SKEW-T/LOG P DIAGRAM Uses natural log of pressure as the vertical coordinate Since pressure decreases exponentially with height, this means that the vertical coordinate roughly represents altitude. Isotherms, instead of being vertical, are slanted upward to the right. Adiabats are lines that are semi-straight, and slope upward to the left. -
The First Law of Thermodynamics Continued Pre-Reading: §19.5 Where We Are
Lecture 7 The first law of thermodynamics continued Pre-reading: §19.5 Where we are The pressure p, volume V, and temperature T are related by an equation of state. For an ideal gas, pV = nRT = NkT For an ideal gas, the temperature T is is a direct measure of the average kinetic energy of its 3 3 molecules: KE = nRT = NkT tr 2 2 2 3kT 3RT and vrms = (v )av = = r m r M p Where we are We define the internal energy of a system: UKEPE=+∑∑ interaction Random chaotic between atoms motion & molecules For an ideal gas, f UNkT= 2 i.e. the internal energy depends only on its temperature Where we are By considering adding heat to a fixed volume of an ideal gas, we showed f f Q = Nk∆T = nR∆T 2 2 and so, from the definition of heat capacity Q = nC∆T f we have that C = R for any ideal gas. V 2 Change in internal energy: ∆U = nCV ∆T Heat capacity of an ideal gas Now consider adding heat to an ideal gas at constant pressure. By definition, Q = nCp∆T and W = p∆V = nR∆T So from ∆U = Q W − we get nCV ∆T = nCp∆T nR∆T − or Cp = CV + R It takes greater heat input to raise the temperature of a gas a given amount at constant pressure than constant volume YF §19.4 Ratio of heat capacities Look at the ratio of these heat capacities: we have f C = R V 2 and f + 2 C = C + R = R p V 2 so C p γ = > 1 CV 3 For a monatomic gas, CV = R 3 5 2 so Cp = R + R = R 2 2 C 5 R 5 and γ = p = 2 = =1.67 C 3 R 3 YF §19.4 V 2 Problem An ideal gas is enclosed in a cylinder which has a movable piston. -
Steam Tables and Charts Page 4-1
CHE 2012 Steam Tables and Charts Page 4-1 SECTION 4 STEAM TABLES AND CHARTS WATER AND STEAM Consider the heating of water at constant pressure. If various properties are to be measured, an experiment can be set up where water is heated in a vertical cylinder closed by a piston on which there is a weight. The weight acting down under gravity on a piston of fixed size ensures that the fluid in the cylinder is always subject to the same pressure. Initially the cylinder contains only water at ambient temperature. As this is heated the water changes into steam and certain characteristics may be noted. Initially the water at ambient temperature is subcooled. As heat is added its temperature rises steadily until it reaches the saturation temperature corresponding with the pressure in the cylinder. The volume of the water hardly changes during this process. At this point the water is saturated. As more heat is added, steam is generated and the volume increases dramatically since the steam occupies a greater space than the water from which it was generated. The temperature however remains the same until all the water has been converted into steam. At this point the steam is saturated. As additional heat is added, the temperature of the steam increases but at a faster rate than when the water only was being heated. The Page 4-2 Steam Tables and Charts CHE 2012 volume of the steam also increases. Steam at temperatures above the saturation temperature is superheated. If the temperature T is plotted against the heat added q the three regions namely subcooled water, saturated mixture and superheated steam are clearly indicated. -
Adiabatic Bulk Moduli
8.03 at ESG Supplemental Notes Adiabatic Bulk Moduli To find the speed of sound in a gas, or any property of a gas involving elasticity (see the discussion of the Helmholtz oscillator, B&B page 22, or B&B problem 1.6, or French Pages 57-59.), we need the “bulk modulus” of the fluid. This will correspond to the “spring constant” of a spring, and will give the magnitude of the restoring agency (pressure for a gas, force for a spring) in terms of the change in physical dimension (volume for a gas, length for a spring). It turns out to be more useful to use an intensive quantity for the bulk modulus of a gas, so what we want is the change in pressure per fractional change in volume, so the bulk modulus, denoted as κ (the Greek “kappa” which, when written, has a great tendency to look like k, and in fact French uses “K”), is ∆p dp κ = − , or κ = −V . ∆V/V dV The minus sign indicates that for normal fluids (not all are!), a negative change in volume results in an increase in pressure. To find the bulk modulus, we need to know something about the gas and how it behaves. For our purposes, we will need three basic principles (actually 2 1/2) which we get from thermodynamics, or the kinetic theory of gasses. You might well have encountered these in previous classes, such as chemistry. A) The ideal gas law; pV = nRT , with the standard terminology. B) The first law of thermodynamics; dU = dQ − pdV,whereUis internal energy and Q is heat. -
Session 15 Thermodynamics
Session 15 Thermodynamics Cheryl Hurkett Physics Innovations Centre for Excellence in Learning and Teaching CETL (Leicester) Department of Physics and Astronomy University of Leicester 1 Contents Welcome .................................................................................................................................. 4 Session Authors .................................................................................................................. 4 Learning Objectives .............................................................................................................. 5 The Problem ........................................................................................................................... 6 Issues .................................................................................................................................... 6 Energy, Heat and Work ........................................................................................................ 7 The First Law of thermodynamics................................................................................... 8 Work..................................................................................................................................... 9 Heat .................................................................................................................................... 11 Principal Specific heats of a gas ..................................................................................... 12 Summary .......................................................................................................................... -
1 Microphysics
ASTR 501 Stellar Physics 1 1 Microphysics • equation of state, density: ρ(P, T, X) • radiative absorption coefficient, opacity: κ(P, T, X) • rate of energy production: (P, T, X) (nuclear physics) Nuclear physics also responsible for composition changes dXj = Fˆj · Xj (1) dt burn while the total composition change also includes a mixing term: dX ∂ dX i = 4πr2ρ D i (2) dt mix ∂m dm 1.1 Equation of state For the fluid to have an EOS it must be collisional: lregion λ (3) where λ is the mean free path. P from equation of state, consider three cases: ASTR 501 Stellar Physics 2 (a) ideal gas equation of state: p = R ρT (b) barotropic equation of state: pressure p depends only on ρ, as for example • isothermal: p ∼ ρ • adiabatic: p = Kργ Plus non-ideal effects, e.g. electron degeneracy. 1.2 Ideal gas equation of state Assumption: internal energy entirely in kinetic energy according to kinetic theory: = CVT , where CV is the specific heat at constant volume. This can be seen from the first law of thermodynamics dQ = d + pdV , where V is the specific volume, d if we express d = dT dT . d Similarly, the specific heat at constant pressure Cp = dT + R where R is the gas constant. This follows from the ideal gas equation of state. [†13] It also follows that Cp − CV = R [†14], and the ratio of specific heats is defined as C γ = p . (4) CV ASTR 501 Stellar Physics 3 α CV can be related to R as CV = 2 R , where α is the number of degrees of freedom 1 per particle, since the energy per particle per degree of freedom is 2kT where k is 2+α the Boltzmann constant, and R = nk. -
Heat Capacity Ratio of Gases
Heat Capacity Ratio of Gases Carson Hasselbrink [email protected] Office Hours: Mon 10-11am, Beaupre 360 1 Purpose • To determine the heat capacity ratio for a monatomic and a diatomic gas. • To understand and mathematically model reversible & irreversible adiabatic processes for ideal gases. • To practice error propagation for complex functions. 2 Key Physical Concepts • Heat capacity is the amount of heat required to raise the temperature of an object or substance one degree 풅풒 푪 = 풅푻 • Heat Capacity Ratio is the ratio of specific heats at constant pressure and constant volume 퐶푝 훾 = 퐶푣 휕퐻 휕퐸 Where 퐶 = ( ) and 퐶 = ( ) 푝 휕푇 푝 푣 휕푇 푣 • An adiabatic process occurs when no heat is exchanged between the system and the surroundings 3 Theory: Heat Capacity 휕퐸 • Heat Capacity (Const. Volume): 퐶 = ( ) /푛 푣,푚 휕푇 푣 3푅푇 3푅 – Monatomic: 퐸 = , so 퐶 = 푚표푛푎푡표푚푖푐 2 푣,푚 2 5푅푇 5푅 – Diatomic: 퐸 = , so 퐶 = 푑푖푎푡표푚푖푐 2 푣,푚 2 • Heat Capacity Ratio: 퐶푝,푚 = 퐶푣,푚 + 푅 퐶푝,푚 푅 훾 = = 1 + 퐶푣,푚 퐶푣,푚 푃 [ln 1 ] 푃2 – Reversible: 훾 = 푃 [ln 1 ] 푃3 푃 [ 1 −1] 푃2 – Irreversible: 훾 = 푃 [ 1 −1] 푃3 • Diatomic heat capacity > Monatomic Heat Capacity 4 Theory: Determination of Heat Capacity Ratio • We will subject a gas to an adiabatic expansion and then allow the gas to return to its original temperature via an isochoric process, during which time it will cool. • This expansion and warming can be modeled in two different ways. 5 Reversible Expansion (Textbook) • Assume that pressure in carboy (P1) and exterior pressure (P2) are always close enough that entire process is always in equilibrium • Since system is in equilibrium, each step must be reversible 6 Irreversible Expansion (Lab Syllabus) • Assume that pressure in carboy (P1) and exterior pressure (P2) are not close enough; there is sudden deviation in pressure; the system is not in equilibrium • Since system is not in equilibrium, the process becomes irreversible. -
Analysis of Thermodynamic Processes with Full Consideration of Real Gas Behaviour
Analysis of thermodynamic processes with full consideration of real gas behaviour Version 2.12. - (July 2020) engineering your visions © by B&B-AGEMA, No. 1 Contents • What is TDT ? • How does it look like ? • How does it work ? • Examples engineering your visions © by B&B-AGEMA, No. 2 Introduction What is TDT ? TDT is a Thermodynamic Design Tool, that supports the design and calculation of energetic processes on a 1D thermodynamic approach. The software TDT can be run on Windows operating systems (Windows 7 and higher) or on different LINUX-platforms. engineering your visions © by B&B-AGEMA, No. 3 TDT - Features TDT - Features 1. High calculation accuracy: • real gas properties are considered on thermodynamic calculations • change of state in each component is divided into 100 steps 2. Superior user interface: • ease of input: dialogs on graphic screen • visualized output: graphic system overview, thermodynamic graphs, digital data in tables 3. Applicable various kinds of fluids: • liquid, gas, steam (incl. superheated, super critical point), two-phase state • currently 29 different fluids • user defined fluid mixtures engineering your visions © by B&B-AGEMA, No. 4 How does TDT look like ? engineering your visions © by B&B-AGEMA, No. 5 TDT - User Interface Initial window after program start: start a “New project”, “Open” an existing project, open one of the “Examples”, which are part of the installation, or open the “Manual”. engineering your visions © by B&B-AGEMA, No. 6 TDT - Main Window Structure tree structure action toolbar notebook containing overview and graphs calculation output On the left hand side of the window the entire project information is listed in a tree structure. -
Thermodynamic/Aerological Charts/Diagrams
THERMODYNAMIC/AEROLOGICAL CHARTS/DIAGRAMS 1 /31 • Thermodynamic charts are used to represent the vertical structure of the atmosphere, as well as major thermodynamic processes to which moist air can be subjected. • Thermodynamic charts can be used to obtain easily different thermodynamic properties, e.g. q (potential temperature) and moisture quantities (such as the specific humidity), from a given radiosonde ascent. • Even though today it is possible to compute many quantities directly, thermodynamic diagrams are still very useful and remain videly used. 2 /31 • Each diagram has lines of constant: – p, pressure, – T, temperature, – q, potential temperature, – q, saturation specific humidity. – saturated adiabats. • One difficulty of all diagrams is that they are two dimensional, and the most compact description of the state of the atmosphere encompasses three dimensions, for instance, {T,p,q}. 3 /31 • The simplest and most common form of the aerological diagram has pressure as the ordinate and temperature as the abscissa – the temperature scale is linear – it is usually desirable to have the ordinate approximately representative of height above the surface, thus The ordinate may be proportional to –ln p (the Emagram) or to pR/cp (the Stuve diagram). • The Emagram has the advantage over the Stuve diagram in that area on the diagram is proportional to energy: dw = pdυ = RdT −υdp dp dw = R dT − RT RdT is an exact differential which integrates to zero !∫ !∫ !∫ p !∫ dw = −R!∫ Td(ln p) • A chart with coordinates of T versus ln p has the property of a true thermodynamic diagram, i.e. the area is proportional to energy.