ATMO 551a Moist Adiabat Fall Change in internal energy: ΔU

Similar documents
ATMO 551a Fall 08. Equivalent Potential Temperature

1. Water Vapor in Air

df dz = dp dt Essentially, this is just a statement of the first law in one of the forms we derived earlier (expressed here in W m 3 ) dq p dt dp

Thermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic]

ATMO/OPTI 656b Spring 09. Physical properties of the atmosphere

Outline. Aim. Gas law. Pressure. Scale height Mixing Column density. Temperature Lapse rate Stability. Condensation Humidity.

Atmospheric Thermodynamics

Radiative equilibrium Some thermodynamics review Radiative-convective equilibrium. Goal: Develop a 1D description of the [tropical] atmosphere

Quasi-equilibrium transitions

P sat = A exp [B( 1/ /T)] B= 5308K. A=6.11 mbar=vapor press. 0C.

2σ e s (r,t) = e s (T)exp( rr v ρ l T ) = exp( ) 2σ R v ρ l Tln(e/e s (T)) e s (f H2 O,r,T) = f H2 O

Exam 1 (Chaps. 1-6 of the notes)

Chapter 4 Water Vapor

First Law of Thermodynamics

Lecture Ch. 6. Condensed (Liquid) Water. Cloud in a Jar Demonstration. How does saturation occur? Saturation of Moist Air. Saturation of Moist Air

Parcel Model. Meteorology September 3, 2008

Meteorology 6150 Cloud System Modeling

ATMO/OPTI 656b Spring 08. Physical Properties of the Atmosphere

Today s Lecture: Atmosphere finish primitive equations, mostly thermodynamics

Parcel Model. Atmospheric Sciences September 30, 2012

Clouds associated with cold and warm fronts. Whiteman (2000)

ρ x + fv f 'w + F x ρ y fu + F y Fundamental Equation in z coordinate p = ρrt or pα = RT Du uv tanφ Dv Dt + u2 tanφ + vw a a = 1 p Dw Dt u2 + v 2

2 Equations of Motion

Clouds and turbulent moist convection

Buoyancy and Coriolis forces

1. Static Stability. (ρ V ) d2 z (1) d 2 z. = g (2) = g (3) T T = g T (4)

Simplified Microphysics. condensation evaporation. evaporation

References: Parcel Theory. Vertical Force Balance. ESCI Cloud Physics and Precipitation Processes Lesson 3 - Stability and Buoyancy Dr.

Atsc final Equations: page 1/6

1/18/2011. Conservation of Momentum Conservation of Mass Conservation of Energy Scaling Analysis ESS227 Prof. Jin-Yi Yu

Measuring State Parameters of the Atmosphere

Naraine Persaud, Entry Code ME-11 1

Hence. The second law describes the direction of energy transfer in spontaneous processes

The Clausius-Clapeyron and the Kelvin Equations

Introduction. Lecture 6: Water in Atmosphere. How Much Heat Is Brought Upward By Water Vapor?

Atmospheric Dynamics: lecture 2

Dynamic Meteorology: lecture 2

ATMOS 5130 Lecture 9. Enthalpy Conservation Property The Second Law and Its Consequences Entropy

Measuring State Parameters of the Atmosphere

Rocket propulsion Prof. K. Ramamurthi Department of Mechanical Engineering Indian Institute of Technology, Madras. Lecture 09 Theory of Nozzles

Project 3 Convection and Atmospheric Thermodynamics

1. The vertical structure of the atmosphere. Temperature profile.

GEF2200 Atmosfærefysikk 2012

First-Order Differential Equations

GEF2200 atmospheric physics 2018

Conservation of Mass Conservation of Energy Scaling Analysis. ESS227 Prof. Jin-Yi Yu

Physics Nov Cooling by Expansion

Atmospheric Physics. August 10, 2017

Kelvin Effect. Covers Reading Material in Chapter 10.3 Atmospheric Sciences 5200 Physical Meteorology III: Cloud Physics

Temperature and Thermodynamics, Part II. Topics to be Covered

ATMO551a Fall Vertical Structure of Earth s Atmosphere

First Law of Thermodyamics U = Q + W. We can rewrite this by introducing two physical. Enthalpy, H, is the quantity U + pv, as this

Thermodynamic Energy Equation

Classical Thermodynamics. Dr. Massimo Mella School of Chemistry Cardiff University

Applied Thermodynamics for Marine Systems Prof. P. K. Das Department of Mechanical Engineering Indian Institute of Technology, Kharagpur

What is thermodynamics? and what can it do for us?

4.1 LAWS OF MECHANICS - Review

Entropy and the Second Law of Thermodynamics

Lecture 9: Climate Sensitivity and Feedback Mechanisms

Convective Heat and Mass Transfer Prof. A.W. Date Department of Mechanical Engineering Indian Institute of Technology, Bombay

4. Atmospheric transport. Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017

Lecture 7. Science A-30 February 21, 2008 Air may be forced to move up or down in the atmosphere by mechanical forces (wind blowing over an obstacle,

ESCI 485 Air/Sea Interaction Lesson 1 Stresses and Fluxes Dr. DeCaria

EART164: PLANETARY ATMOSPHERES

Liquid water static energy page 1/8

Planetary Atmospheres

Global Energy Balance: Greenhouse Effect

2.1 Effects of a cumulus ensemble upon the large scale temperature and moisture fields by induced subsidence and detrainment

An alternative, less empirical approach (though still full of brazen assumptions) is the following:

ATMO 551a Fall The Carnot Cycle

Numerical Example An air parcel with mass of 1 kg rises adiabatically from sea level to an altitude of 3 km. What is its temperature change?

Thermodynamics Introduction and Basic Concepts

Chapter 5 - Atmospheric Moisture

w = -nrt hot ln(v 2 /V 1 ) nrt cold ln(v 1 /V 2 )[sincev/v 4 3 = V 1 /V 2 ]

Needs work : define boundary conditions and fluxes before, change slides Useful definitions and conservation equations

LECTURE 5 THE CONTENTS OF THIS LECTURE ARE AS FOLLOWS: 1.0 SOME OF THE THEORETICAL CONCEPTS INVOLVED IN HEAT FLOW. 1.1 Sensible Heat Flow

Köhler Curve. Covers Reading Material in Chapter 10.3 Atmospheric Sciences 5200 Physical Meteorology III: Cloud Physics

Atmospheric Sciences 321. Science of Climate. Lecture 13: Surface Energy Balance Chapter 4

CHEMICAL ENGINEERING THERMODYNAMICS. Andrew S. Rosen

Composition, Structure and Energy. ATS 351 Lecture 2 September 14, 2009

Lecture 3: Convection

Step 1. Step 2. g l = g v. dg = 0 We have shown that over a plane surface of water. g v g l = ρ v R v T ln e/e sat. this can be rewritten

Diffusional Growth of Liquid Phase Hydrometeros.

Lecture 10: Climate Sensitivity and Feedback

Basic Thermodynamics Prof. S.K Som Department of Mechanical Engineering Indian Institute of Technology, Kharagpur

Chapter 4. Energy Analysis of Closed Systems

First Law CML 100, IIT Delhi SS. The total energy of the system. Contribution from translation + rotation + vibrations.

1 One-dimensional analysis

Radiative-Convective Models. The Hydrological Cycle Hadley Circulation. Manabe and Strickler (1964) Course Notes chapter 5.1

Theory. Humidity h of an air-vapor mixture is defined as the mass ratio of water vapor and dry air,

Isobaric Coordinates

MME 2010 METALLURGICAL THERMODYNAMICS II. Fundamentals of Thermodynamics for Systems of Constant Composition

Name... Class... Date... Specific heat capacity and specific latent heat

Thermodynamics part III.

Atmospheric Composition הרכב האטמוספירה

1 Introduction to Governing Equations 2 1a Methodology... 2

1. Heterogeneous Systems and Chemical Equilibrium

Physics 53. Thermal Physics 1. Statistics are like a bikini. What they reveal is suggestive; what they conceal is vital.

Chapter 5. On-line resource

GEF2200 vår 2017 Løsningsforslag sett 1

Transcription:

Enthalpy and the Moist Adiabat We have described the dry adiabat where an air parcel is lifted rapidly causing the air parcel to expand as the environmental pressure decreases and the air parcel does work on the environment but no heat is exchanged with the environment. As a result some of the air parcel s internal energy is converted to doing work on the environment. The result is the dry adiabatic temperature gradient dt dz = g (1) C p Now we discuss the effect of transferring the latent of water vapor to increase the temperature of the air. This includes discussion about various measures of energy or heat, and highlight what the concept of enthalpy is. Recall that when heat enters or is added to a parcel, this heat can go to the internal energy of the parcel, as well as to work the parcel does on the environment. Remember that energy added to the system goes into some combination of the bulk energy of the system, E B, (which is large scale mechanical energy: kinetic plus potential energy) plus the internal energy of the system, U. We write this as Δ( U + E B ) = ΔQ + ΔW (2) Heat added: ΔQ SYSTEM Work done by surroundings: ΔW Change in internal energy: ΔU Change in bulk energy: ΔE B where ΔW is defined as positive when the environment does work on the parcel (not when the parcel does work on the environment). Remember also that ΔW =-p ΔV. Now we ignore changes in bulk energy and express the properties of the parcel in specific units (i.e. per unit mass), yielding dq = du dw = du + p d(1/ρ) Note that q here is the heat per unit mass, not the specific humidity. Remember that when heat is added to the system (=air parcel) when volume (i.e. density) is kept constant, the only place for the energy to go is into the kinetic energy of the molecules: dq v = du = c v dt. If we consider heating up the gas from some absolute zero temperature, we can define the total specific internal energy as 1 Kursinski 10/18/10

u = c v T where we have assumed c v is independent of T and that no phase changes have occurred. We ll address the effects of phase changes shortly. Now, when heat is added to the air parcel when it is held at constant pressure (which is the typical situation in the atmosphere) we can rewrite d(1/ρ) = d(r*t/p m A ), and end up with dq p = c v dt + (R*/m a ) dt = c p dt Here, there is a work term, because as the gas heats up at constant pressure, it expands and does work on the environment. To keep track of this process, we define the enthalpy, h h = u + p/ρ = c p T Note that Enthalpy is not a measure of the energy contained in a parcel. It is a hybrid that contains both the internal energy and some of the energy that the air parcel transferred to the environment that the environment stores to make room for the parcel. In a hydrostatic atmosphere, this second form of energy is stored as the extra gravitational potential of the overriding air that has been lifted to make room for the expanded parcel. Now consider the most general form of dq again, where we take advantage of our expression for enthalpy dq = du dw = du + pd(1/ρ) = du + p d(r*t/pm a ) = dh ρ -1 dp In hydrostatic equilibrium, we have dq = dh + gdz = dh + dφ We call the term h + Φ the dry static energy, and keep track of it with the potential temperature θ = T + Φ/c p = T + Γ d z What goes into the dry static energy is the gravitational potential energy of the parcel, the internal energy of the parcel, and the gravitational potential of the air overlying the parcel caused by the parcel s presence (volume). We keep track of dry static energy because it is constant 2 Kursinski 10/18/10

during adiabatic processes, when dq = 0. Dry static energy goes to zero as a parcel is adiabatically dropped to the ground and then cooled at constant pressure to zero. Moist static energy This has all been review, but I m now using the notation and terms in W+H to be consistent. Now let s consider what happens when we throw phase changes into the mix. Water vapor releases heat when it condenses. This is called the latent heat of vaporization in W+H, although you will also see it called the latent heat of condensation. The amount of heat released is a weak function of temperature, with a value of about 2.5x10 6 J/kg at 0 C, and 2.25 x 10 6 J/kg at 100 C. The amount of heat released depends on the amount of mass of water vapor condensed or in units of specific heat, we have dq = -L v dm v dq = -L v dq v Note that there s a minus sign because vapor content goes down when condensation occurs. Relating this to the heating of our parcel, we have dq = dh + dφ = -L v dq v If there is no heat exchange besides this latent process, we can write 0 = dh + dφ + L v dq v This is called a moist adiabatic process the only heat exchange is the conversion of latent heat of vapor into sensible heat as the vapor condenses. Since no heat or mass actually crosses the boundary of our parcel, this is really considered an interconversion of internal enrgy. We can even consider the un-condensed vapor as a form of internal energy, not as a form of heat. In this case, we define the moist static energy of a parcel as, h + Φ + L v q v To keep track of moist static energy, we define the equivalent potential temperature θ e = θ + (L v /c p )q v θ e is always larger than θ, as it includes the internal potential energy of the vapor. It is also conserved when cloud water condenses or evaporates. You can think of equivalent potential temperature as the temperature a parcel would have if you first condensed all the vapor out, and then dropped it to surface pressure adiabatically. Exercise: What is the potential temperature outside right now? (T = 34.7; Td = 1.6; p = 926 mb) In the general adiabatic case for a rising air parcel, dz > 0, dt < 0 and dq < 0. We need an additional constraint on the problem and this is provided by the assertion that dq = dq s (T), which is the same thing as saying that RH will max out at 100%. (We will learn later that this is merely an approximation, but it is a good one for coarse purposes). For RH to equal 100% as 3 Kursinski 10/18/10

temperature is decreasing, there must be a corresponding decrease in saturation vapor pressure, which is achieved by condensation. The saturation specific humidity is the ratio of the saturation density to air density. q s = ρ s /ρ a The saturation density is obtained from the saturation vapor pressure using the ideal gas law. ρ s = n sv M w n sv = e s (T)/(R*T) Using the ideal gas law to relate air density to air pressure, we get ρ a = pm w /(R*T) These lead to the following simplification for q s q s = (M w /M A )(e s (T)/p) Now our goal is to find dq s, which is more easily manipulated through its log dq s = q s dlnq s = q s (dlne s dlnp) [Note that we have conveniently neglected the sensitivity of molecular weight of air to vapor pressure, which will contribute a very minor term.] The first term shows that saturation mixing ratio will increase if saturation vapor pressure increases. Note the second term that shows that saturation specific humidity will increase with a decrease in ambient pressure. This might seem counterintuitive, since we know that q doesn t change with changes in pressure. However, q s is a different beast than q. Whereas q keeps track of the mass of vapor in a given mass of air, q s tracks the mass of water vapor that would be in equilibrium with a flat surface of water per unit mass of air. As pressure goes up and down, saturation vapor pressure doesn t notice. It is only sensitive to temperature. However, the dry air mass is fluctuating with pressure, causing the constant saturation vapor pressure to be a relatively larger fraction of the air pressure as pressure goes down. To explore this further, consider a chamber that is partially filled with water and is held at temperature T. In equilibrium, the total pressure will be p d + e s (T), where p d is the pressure due to the dry air. Now we evacuate the chamber of half the air. At this very instant the pressure will be p d /2 + e s (T)/2, and q will be the same as before since there has been no condensation or evaporation (yet). But the water surface will still have a vapor pressure of e s (T). So over time, water will evaporate and q will increase to a new, higher equilibrium value, qs(t,p f ). Now we go back to the moist parcel that is ascending adiabatically. From Clausius-Clapyron, we have dlne s = L c M w /(R*T 2 ) dt And hydrostatic pressure for ideal gases can be written as: dlnp = -dz/h 4 Kursinski 10/18/10

Where H is the scale height of the atmosphere = R*T/(M A g). Thus our expression for dq s can be written in terms of dt and dz, which are the same independent variables used in our dry adiabatic equation. dq s = q s (L c M w /(R*T 2 ) dt + dz/h) Subbing all this into the energy conservation equation yields, 0 = c p dt + gdz + L c q s [L c M w /(R*T 2 ) dt + dz/h] Now we can solve for dt/dz = -Γ M, which is called the moist adiabatic lapse rate dt/dz = - (g + L c q s /H) / [c p + L c q s (L c M w /(R*T 2 ))] At this point, it is useful to note the g/c p is the dry adiabatic lapse rate, Γ D, and that H is a function of gravity. After some algebra, we get, Γ M = Γ D qsm A 1+ R * T qs M 1+ c R * T p W 2 When all is said and done, we see that there are two terms that make the moist adiabatic lapse rate different from the dry value. The numerator contains a term that came from the pressure dependence of saturation specific humidity (as discussed above). The denominator has a term that came from the temperature dependence of saturation specific humidity through the Clausius Clapyron relation, and this is the dominant term. While both terms are important to getting the right value, the CC term dominates. At 0 C and mean sea level pressure (MSL) the denominator is 1.68 and the numerator is 1.12, with that the moist lapse rate is (6.5 K/km), about 2/3 the value of the dry lapse rate. At 15 C, the numerator is 1.312 and the denominator increases to 2.630, for a moist lapse rate of 4.9 half the value of the dry lapse rate. This addition of the 2 nd term in the denominator signifies that that both kinetic and latent energy sources are used to do work on the environment as it expands, thus slowing the cooling relative to the case when only kinetic energy is used. The modifier in the numerator accounts for the evaporation (and hence cooling) that happens independently of temperature as air depressurizes, due to the drop in vapor pressure at fixed specific humidity. Because it represents a cooling with height, it increases the magnitude of the lapse rate, but only slightly relative to the CC effect. 5 Kursinski 10/18/10