EAS270, The Atmosphere 2 nd Mid-term Exam 2 Nov. 2016

Similar documents
EAS270, The Atmosphere Mid-term Exam 27 Oct, 2006

EAS270, The Atmosphere Mid-term Exam 28 Oct. 2011

Solar Radiation and Environmental Biophysics Geo 827, MSU Jiquan Chen Oct. 6, 2015

Lecture 4: Radiation Transfer

1) The energy balance at the TOA is: 4 (1 α) = σt (1 0.3) = ( ) 4. (1 α) 4σ = ( S 0 = 255 T 1

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?

Lecture 2: Global Energy Cycle

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun

AT350 EXAM #1 September 23, 2003

Lecture 5: Greenhouse Effect

Lecture 9: Climate Sensitivity and Feedback Mechanisms

Earth s Energy Balance and the Atmosphere

Project 3 Convection and Atmospheric Thermodynamics

Hand in Question sheets with answer booklets Calculators allowed Mobile telephones or other devices not allowed

Spectrum of Radiation. Importance of Radiation Transfer. Radiation Intensity and Wavelength. Lecture 3: Atmospheric Radiative Transfer and Climate

Lecture 3: Atmospheric Radiative Transfer and Climate

Radiative Equilibrium Models. Solar radiation reflected by the earth back to space. Solar radiation absorbed by the earth

ATMOSPHERIC ENERGY and GLOBAL TEMPERATURES. Physical Geography (Geog. 300) Prof. Hugh Howard American River College

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics Problem Solving 10: The Greenhouse Effect. Section Table and Group

Lecture 5: Greenhouse Effect

MAPH & & & & & & 02 LECTURE

Radiation, Sensible Heat Flux and Evapotranspiration

Boundary layer equilibrium [2005] over tropical oceans

1. Weather and climate.

Lecture 2: Global Energy Cycle

Solar Flux and Flux Density. Lecture 2: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth

G109 Midterm Exam (Version A) October 10, 2006 Instructor: Dr C.M. Brown 1. Time allowed 50 mins. Total possible points: 40 number of pages: 5

( ) = 1005 J kg 1 K 1 ;

Glaciology HEAT BUDGET AND RADIATION

Lecture 3: Global Energy Cycle

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

The Planck Blackbody Equation and Atmospheric Radiative Transfer

Chapter 4 Water Vapor

Radiation in the atmosphere

Mon Oct 20. Today: radiation and temperature (cont) sun-earth geometry energy balance >> conceptual model of climate change Tues:

Energy. Kinetic and Potential Energy. Kinetic Energy. Kinetic energy the energy of motion

G109 Alternate Midterm Exam October, 2004 Instructor: Dr C.M. Brown

Blackbody Radiation. A substance that absorbs all incident wavelengths completely is called a blackbody.

ATMS 321 Problem Set 1 30 March 2012 due Friday 6 April. 1. Using the radii of Earth and Sun, calculate the ratio of Sun s volume to Earth s volume.

Earth: the Goldilocks Planet

Lecture 2 Global and Zonal-mean Energy Balance

ATMS 321: Sci. of Climate Final Examination Study Guide Page 1 of 4

Mon April 17 Announcements: bring calculator to class from now on (in-class activities, tests) HW#2 due Thursday

Remote Sensing C. Rank: Points: Science Olympiad North Regional Tournament at the University of Florida. Name(s): Team Name: School Name:

Temperature (T) degrees Celsius ( o C) arbitrary scale from 0 o C at melting point of ice to 100 o C at boiling point of water Also (Kelvin, K) = o C

Final Examination. Part A Answer ONLY TWELVE QUESTIONS in Part A. (Each question is 3 points)

Radiation in climate models.

- global radiative energy balance

Exercises. Exercises 145

Understanding the Greenhouse Effect

Lecture 4: Heat, and Radiation

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

The Structure and Motion of the Atmosphere OCEA 101

( 1 d 2 ) (Inverse Square law);

Lecture 4: Global Energy Balance

Lecture 4: Global Energy Balance. Global Energy Balance. Solar Flux and Flux Density. Blackbody Radiation Layer Model.

Data and formulas at the end. Exam would be Weds. May 8, 2008

Snow II: Snowmelt and energy balance

The Earth s Radiation Balance

Key Feedbacks in the Climate System

Chapter 2. Heating Earth's Surface & Atmosphere

The Atmospheric Boundary Layer. The Surface Energy Balance (9.2)

ATMOS 5140 Lecture 1 Chapter 1

COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION

Earth Systems Science Chapter 3

Course Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2. Changing climate. 3. Future climate change

The inputs and outputs of energy within the earth-atmosphere system that determines the net energy available for surface processes is the Energy

- matter-energy interactions. - global radiation balance. Further Reading: Chapter 04 of the text book. Outline. - shortwave radiation balance

Let s make a simple climate model for Earth.

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,

Next quiz: this Friday, questions. Plus more on Wednesday.

Global Climate Change

The Atmosphere. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems

ATMOS 5140 Lecture 7 Chapter 6

Energy: Warming the earth and Atmosphere. air temperature. Overview of the Earth s Atmosphere 9/10/2012. Composition. Chapter 3.

Lecture # 04 January 27, 2010, Wednesday Energy & Radiation

1., annual precipitation is greater than annual evapotranspiration. a. On the ocean *b. On the continents

Energy Balance and Temperature. Ch. 3: Energy Balance. Ch. 3: Temperature. Controls of Temperature

Energy Balance and Temperature

Monday 9 September, :30-11:30 Class#03

Torben Königk Rossby Centre/ SMHI

Chapter 02 Energy and Matter in the Atmosphere

Temperature Change. Heat (Q) Latent Heat. Latent Heat. Heat Fluxes Transfer of heat in/out of the ocean Flux = Quantity/(Area Time) Latent heat

di λ ds = ρk λi λ B λ (T ) + ρk λ dz' )= B λ (T(z'))e I λ (z TOA + k λ Longwave radiative transfer Longwave radiative transfer

Greenhouse Steady State Energy Balance Model

Energy, Temperature, & Heat. Energy, Temperature, & Heat. Temperature Scales 1/17/11

Questions you should be able to answer after reading the material

Modeling of Environmental Systems

GEO1010 tirsdag

Clouds and atmospheric convection

Chapter 11 Lecture Outline. Heating the Atmosphere

Emission Temperature of Planets. Emission Temperature of Earth

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

Lecture 10: Climate Sensitivity and Feedback

Course Outline. About Me. Today s Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2.

Meteorology Pretest on Chapter 2

5) The amount of heat needed to raise the temperature of 1 gram of a substance by 1 C is called: Page Ref: 69

Which picture shows the larger flux of blue circles?

Temperature Pressure Wind Moisture

Lecture 3a: Surface Energy Balance

Transcription:

EAS270, The Atmosphere 2 nd Mid-term Exam 2 Nov. 2016 Professor: J.D. Wilson Time available: 50 mins Value: 25% No formula sheets; no use of tablet computers etc. or cell phones. Formulae/data at back. Multi-choice (25 x 1 25 %) 1. Referring to Figure (1), which statement is false? (a) A,B,C lie in the shortwave radiation band (b) D,E lie in the longwave radiation band (c) The atmosphere is almost completely transparent at C (d) Waveband C would be ideal for nocturnal viewing of earth from satellites (e) The high absorbtivity at λ > 20µm is due to greenhouse gases 2. Referring to Figure (2), select the correct pair of values for the temperature lapse rate ( T/ z) in respectively the lower and the upper layers. (Note: a temperature change of 1 o C is the same as a change of 1 K). (a) 0.01 Km 1, 0.005 Km 1 (b) 0.01 Km 1, 0.002 Km 1 (c) 0.02 Km 1, 0.002 Km 1 (d) 0.02 Km 1, 0.005 Km 1 (e) 0.05 Km 1, 0.005 Km 1 Read T/ z off graph. 3. Referring to Figure 3, which option gives correct units for the vertical axis (spectral emission ratefromablackbody)andfortheareaunderthecurve(emittedradiantenergyfluxdensity)? (a) Wm 2, Wm 2 (b) Wm 2 µm 1, W (c) Wm 2 µm 1, Wm 2 (d) Wm 2 µm 1, Wµm 1 (e) Wµm 1, Wµm 4. If a certain body has longwave emissivity ǫ = 0.96 and its temperature is T = 18 o C, which option most closely states the wavelength λ max of the peak in its thermal emission spectrum and its full-spectrum rate of emission E of longwave radiation? (a) 10µm, 390Wm 2 (b) 10µm, 6 10 3 Wm 2 (c) 100µm, 390Wm 2 (d) 1µm, 410Wm 2 (e) 0.1µm, 410Wm 2 1

5. Which statement in regard to Figure (4) is false? (a) each of Q,Q H,Q E quantifies an energy flux density oriented along the vertical axis (b) it is implicit (assumed) horizontal energy flows are irrelevant (c) above the laminar sublayer on ground surfaces, the transport mechanism for sensible & latent heat (Q H,Q E ) is convection (d) Q G (sometimes symbolized Q S ) is the rate at which energy is stored/released below the reference plane (e) times of sunrise & sunset coincide with sign changes in net radiation (Q ) 6. Suppose on a sunny summer afternoon the net radiation over a flat field of bare soil were Q = 500 W m 2, and the sensible and latent heat fluxes were Q H = 180, Q E = 300 W m 2. What was the soil heat flux Q G? (a) 980 W m 2 (b) 480 W m 2 (c) 120 W m 2 (d) 20 W m 2 (e) 980 W m 2 7. Compute absolute humidity ρ v if vapour pressure e = 1.1 kpa and temperature T = 23 o C. (a) 8 10 3 kgm 3 (b) 8 10 6 kgm 3 (c) 0.1 kgm 3 (d) 1 10 4 kgm 3 (e) 8 gkg 1 8. What is the RH of air with temperature T = 6 o C and vapour pressure e = 7 hpa? (a) 95% (b) 75% (c) 65% (d) 55% (e) 45% 9. Which property is not constant, for an air parcel undergoing unsaturated, adiabatic vertical motion? (a) mixing ratio r (b) specific humidity q (c) potential temperature θ (d) vapour pressure e 2

10. Suppose planet A at distance r A from its star (or sun) has solar constant S A. What is the solar constant ( S B ) for planet B, orbiting the same star at distance r B = 4r A? (a) 4S A (b) 16S A (c) S A /4 (d) S A /16 (e) S A /64 11. A hypothetical radiative equilibrium temperature T E can be calculated as the mean temperature of an isothermal earth (of radius r E ) that has no atmosphere, based on an energy balance of form dt E dt πr 2 E (1 r s)s 0 4πr 2 E σt4 E I II III where the term on the left is the rate of warming or cooling (change in T E per unit change in time t), r s is the albedo (shortwave reflectivity), S 0 the solar constant, σ the Stefan- Boltzmann constant, and means is proportional to. Which term(s) is/are set to zero in order to compute the radiative equilibrium temperature? (a) I (b) I, II (c) I, III (d) I, II, III (e) III 12. Supposeapilot, flying atmiddaythroughthemiddleofadeepcloudlayer, observes abrighter region towards the sun. Which best describes the colour of this sunlight? (a) reddish light (b) bluish light (c) milky white light (d) yellow-brown light 13. At the time of the southern hemisphere summer solstice (solar declination δ = 23.5 o ), what is the noon solar elevation at latitude φ = +23.5 o (which is in the northern hemisphere)? (See given equation) (a) 90 o (b) 66.5 o (c) 43 o (d) 23.5 o (e) 0 o 3

14. Based on Figure (5), at what time did the daily maximum in surface temperature occur? (Note: Local Standard Time was UTC - 7). (a) 0/24 UTC (b) 21 UTC (c) between 19 and 20 UTC (d) 13 UTC (e) 3 UTC 15. Assuming Figure (6) applies during a period of cloudless summer weather, which interpretive statement is false? (a) the layer identified as free air also classifies as being an inversion (b) the Residual Layer is well-mixed (i.e. neutral) with respect to unsaturated adiabatic motion (c) this diagram is characteristic of mid-afternoon conditions (d) the free air is unconditionally stable (e) the sensible heat flux Q H is negative in the surface inversion, and zero in the Residual Layer 16. Referring to Figure (7), over what interval of time was the atmospheric surface layer unstably stratified? (a) midnight to 07:00 (b) 17:30 to midnight (c) midnight to 07:00 and 17:30 to midnight (d) 07:00 to 17:30 (e) 05:30 to 20:00 17. Referring to Figure (8), what is the temperature T if the vapour pressure is e = 4 kpa? (a) 20 C (b) 0 C (c) 20 C (d) 29 C (e) T cannot be determined from the given information 4

18. Referring to Figure (9), which statement is true? (a) the middle layer is neutral with respect to unsaturated adiabatic motion (b) until it rose above level z, an unsaturated parcel rising from the surface would be subject to a downward buoyancy force F B (c) in middle layer, potential temperature decreases with increasing height (d) the uppermost layer is absolutely unstable (e) the surface layer is an inversion 19. Using Figure (10), deduce an approximate value for the potential temperature of air with (P,T) = (400hPa, 60 C), taking the reference pressure as 1000 hpa. (a) 22 C (b) 22K (c) 2 C (d) +4 C (e) +22 C 20. Again referring to Figure (10), suppose the surface pressure, temperature and dewpoint were respectively (1000hPa, 10 C, 20 C). Using Normand s Rule, estimate the pressure at the Lifting Condensation Level. (a) 510 hpa (b) 630 hpa (c) 680 hpa (d) 850 hpa (e) 1000 hpa 21. If the Level of Free Convection is at height z LCL = 500m AGL (above ground level) and the surface temperature is T = 23 C, what is the surface dewpoint T d? (a) 4 C (b) 4 C (c) 11.5 C (d) 19 C (e) 27 C 5

22. What is signified by the heavy dashed line on Figure (11) that has been added by the instructor? (a) ridge in the 500 hpa height field (b) trough in the 500 hpa height field (c) thermal (thickness) ridge (d) thermal trough (e) possibility of freezing rain 23. What is signified by the pattern of stippling on Figure (11)? (a) possibility of freezing rain (b) thickness lies in the interval 534 Z 540 dam (c) temperature-dewpoint spread T dd 2 K (d) temperature below freezing (e) probable path for the upper low to follow 24. Based on Figure (11), which statement regarding the short term (say, 1 hour) weather trend at the point denoted X (north of SASK. ) is most plausible? (a) advective warming (b) advective cooling (c) radiative cooling (d) frost (e) rain 25. Referring to Figure (12), which statement correctly distinguishes the expected 1-hour advective temperature trends at the points (A,B,C)? (a) A warming, B cooling, C cooling (b) A cooling, B warming, C cooling (c) A unchanging, B warming, C warming (d) A unchanging, B cooling, C warming (e) A warming, B warming, C warming 6

Equations and Data. E = ǫ σ T 4. Stefan-Boltzmann law. E [W m 2 ], the emitted longwave energy flux density; ǫ, the emissivity of the surface (dimensionless); σ = 5.67 10 8 [W m 2 K 4 ], the Stefan- Boltzmann constant; T [K], the surface temperature. λ max = 2897 T. Wien s displacement law. λ max [µm], the wavelength at which the peak in the emission spectrum occurs; T [K], the temperature of the emitting surface. α = 90 o φ δ. Solar elevation α at local solar noon time, at a location having latitude φ (negative in the S. hemisphere), at the time of year when solar declination is δ (δ is negative during northern hemisphere winter, and at the time of the solstices its magnitude is 23.5 o ). Q = Q H + Q E + Q S. Surface energy balance on a reference plane at the base of the atmosphere. Q the net radiation, positive if directed towards the surface; Q H,Q E the sensible and latent heat fluxes, positive if directed from the surface towards the atmosphere; Q S (sometimes denoted Q G ) the storage term, positive if directed from the surface into ground/lake/ocean. e = ρ v R v T. The ideal gas law for water vapor. e [Pa], vapour pressure; ρ v, [kg m 3 ] the absolute humidity (ie. vapor density); T [Kelvin], the temperature; and R v = 462 [J kg 1 K 1 ], the specific gas constant for water vapor. F B = g Tp T = g θp θ. The buoyancy force on a parcel whose temperature is T T θ p (and potential tempertaure is θ p ) at a level where the environmental temperature and potential temperature are T,θ. The denominator must be in Kelvin unit. F B is positive for an upward force. z LCL = 125 (T sfc T d,sfc ). Gives the height of the LCL in metres AGL, given the difference between surface temperature and surface dewpoint. Table 1: Equilibrium vapour pressure e s (T) [hpa] versus temperature T [ o C]. Figure cited applies to equilibrium over a plane surface of water where T 0 o C, or of ice where T < 0 o C. T e s (T) T e s (T) T e s (T) T e s (T) T e s (T) T e s (T) T e s (T) T e s (T) -10 2.60-5 4.02 0 6.11 5 8.72 10 12.27 15 17.04 20 23.37 25 31.67-9 2.84-4 4.37 1 6.57 6 9.35 11 13.12 16 18.17 21 24.86 26 33.61-8 3.10-3 4.76 2 7.05 7 10.01 12 14.02 17 19.37 22 26.43 27 35.65-7 3.38-2 5.17 3 7.58 8 10.72 13 14.97 18 20.63 23 28.09 28 37.80-6 3.69-1 5.62 4 8.13 9 11.47 14 15.98 19 21.96 24 29.83 29 40.06 7

Figure 1: Radiative absorptivity of the earth s atmosphere, versus wavelength ( λ ): if, at a given wavelength, the absorptivity is 100%, then light of that wavelength is absorbed completely on a vertical path through the (whole) atmosphere. Labels (A,B,...E) each denote a characteristic region of the absorption spectrum. 1500 1000 Height [m] 500 0 13 14 15 16 17 18 19 20 Temperature o C Figure 2: Idealized profile of temperature in the lowest 1500 m of the atmosphere. The elbow is at (z,t) = (500m,15 o C). (Note: a temperature change of 1 o C is the same as a change of 1 K.) 8

E λ (λ) 0 0 10 20 30 40 50 60 λ, μ m Figure 3: Planck curve for the spectral emission rate from a blackbody with temperature 300 K. Figure 4: Idealized daily cycle in the components of the surface energy balance for a moist, vegetated surface on a clear day in summer (Figure 6.19 from Ross s Weather & Climate). Symbols are Q the net radiation (= K +L, sum of net shortwave plus net longwave radiation), positive for downward flow towards the surface; Q H,Q E the sensible and latent heat fluxes, positive for upward flow away from the surface; and Q G the energy flux into storage, sometimes labelled Q s. 9

Figure 5: Variation with time of the components of the near-surface radiation budget, measured in Nevada. Figure 6: Idealised profile of potential temperature θ(z). 10

W m -2 600 400 200 Q* Q H Q E Q G 0 200 0 6 12 18 24 Hour Figure 7: Variation with time of the components of the surface energy budget over grassland in Alberta (1 July 2003; courtesy of L. Flanagan). Figure 8: Curve giving equilibrium vapour pressure versus temperature. (Ross, Fig 7.4.) 11

Figure 9: Idealized three-layer summer, daytime temperature profile. (Ross s Figure 8.21). Figure 10: Blank skew-t/log-p diagram. Heavy solid curves are dry adiabats, lighter solid curves are moist adiabats, dashed lines are isohumes, and straight lines are isobars or isotherms.. 12

Figure 11: CMC 500 hpa analysis (cropped) for 12Z on 27 Sept. 2016. Secondary field is the 1000-500 hpa thickness, and the contour on the warm side of the stippled zone is the 540 dam thickness contour. Figure 12: CMC 850 hpa analysis (cropped) for 00Z on 10 Oct. 2016. 13