Greenhouse Steady State Energy Balance Model

Similar documents
Radiation, Sensible Heat Flux and Evapotranspiration

Glaciology HEAT BUDGET AND RADIATION

Lecture 3a: Surface Energy Balance

Lecture 9: Climate Sensitivity and Feedback Mechanisms

Lecture 3a: Surface Energy Balance

Modeling of Environmental Systems

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

Chapter 1 INTRODUCTION AND BASIC CONCEPTS

METR 130: Lecture 2 - Surface Energy Balance - Surface Moisture Balance. Spring Semester 2011 February 8, 10 & 14, 2011

Effect of moisture transfer on heat energy storage in simple layer walls

PERFORMANCE EVALUATION OF REFLECTIVE COATINGS ON ROOFTOP UNITS

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

Outline. Stock Flow and temperature. Earth as a black body. Equation models for earth s temperature. Balancing earth s energy flows.

Level 7 Post Graduate Diploma in Engineering Heat and mass transfer

ERT 460 CONTROLLED ENVIRONMENT DESIGN II HEAT TRANSFER. En Mohd Khairul Rabani Bin Hashim

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

Lecture notes: Interception and evapotranspiration

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

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

Snow II: Snowmelt and energy balance

Lecture 10. Surface Energy Balance (Garratt )

Earth s Energy Balance and the Atmosphere

Boundary layer equilibrium [2005] over tropical oceans

Lecture 4: Global Energy Balance

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

Temperature and light as ecological factors for plants

Heat budget and thermodynamics at a free surface:

SEM-2017(03HI MECHANICAL ENGINEERING. Paper II. Please read each of the following instructions carefully before attempting questions.

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

Radiation Effects On Exterior Surfaces

Lecture 7: The Monash Simple Climate

1. Weather and climate.

Chapter 3. Basic Principles. Contents

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

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

GEOG415 Mid-term Exam 110 minute February 27, 2003

Lecture 4: Heat, and Radiation

Principles of Solar Thermal Conversion

ME 476 Solar Energy UNIT TWO THERMAL RADIATION

Earth s Energy Budget: How Is the Temperature of Earth Controlled?

Name(s) Period Date. Earth s Energy Budget: How Is the Temperature of Earth Controlled?

Lecture 5: Greenhouse Effect

WUFI Workshop NBI / SINTEF 2008 Radiation Effects On Exterior Surfaces

Thermal Energy Final Exam Fall 2002

Energy and Radiation. GEOG/ENST 2331 Lecture 3 Ahrens: Chapter 2

Simplified Collector Performance Model

Teaching the Greenhouse Effect. Brian Hornbuckle and Ray Arritt

Physics 111. Lecture 42 (Walker: 18.9) Entropy & Disorder Final Review. May 15, 2009

Lecture 5: Greenhouse Effect

CZECH TECHNICAL UNIVERSITY IN PRAGUE FACULTY OF MECHANICAL ENGINEERING DEPARTMENT OF ENVIRONMENTAL ENGINEERING

( ) = 1005 J kg 1 K 1 ;

ET Theory 101. USCID Workshop. CUP, SIMETAW (DWR link)

S.E. (Chemical) (Second Semester) EXAMINATION, 2011 HEAT TRANSFER (2008 PATTERN) Time : Three Hours Maximum Marks : 100

Block 6 Heat transport in rivers

Thermodynamics Introduction and Basic Concepts

CAE 331/513 Building Science Fall 2017

The Numerical Psychrometric Analysis

Climate Roles of Land Surface

Thermal behavior and Energetic Dispersals of the Human Body under Various Indoor Air Temperatures at 50% Relative Humidity

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

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

CAE 331/513 Building Science Fall 2015

Land Surface Processes and Their Impact in Weather Forecasting

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

Lecture 10: Climate Sensitivity and Feedback

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

ONE DIMENSIONAL CLIMATE MODEL

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

Section 3.5 Thermal Comfort and Heat Stress

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

ln P s T and P s T where R 22,105, D A 27, E B 97.

Thermal Crop Water Stress Indices

Climate Models & Climate Sensitivity: A Review

Thermodynamics. Thermodynamics is the study of the collective properties of a system containing many bodies (typically of order 10 23!

Biological Process Engineering An Analogical Approach to Fluid Flow, Heat Transfer, and Mass Transfer Applied to Biological Systems

Lecture 3A: Interception

Global Energy Balance: Greenhouse Effect

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

AR/IA 241 LN 231 Lecture 4: Fundamental of Energy

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

Heat Transfer: Physical Origins and Rate Equations. Chapter One Sections 1.1 and 1.2

C ONTENTS CHAPTER TWO HEAT CONDUCTION EQUATION 61 CHAPTER ONE BASICS OF HEAT TRANSFER 1 CHAPTER THREE STEADY HEAT CONDUCTION 127

Global Climate Change

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

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

Lecture 3: Light and Temperature

The Choice of Supply Design Conditions

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

ApacheLoads Calculation Methodology as used in Revit MEP 2008 <Virtual Environment> 5.7

HEAT TRANSFER 1 INTRODUCTION AND BASIC CONCEPTS 5 2 CONDUCTION

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

Diffusional Growth of Liquid Phase Hydrometeros.

Heat and Mass Transfer Unit-1 Conduction

Reading Problems , 15-33, 15-49, 15-50, 15-77, 15-79, 15-86, ,

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

Energy flows and modelling approaches

Evapotranspiration. Rabi H. Mohtar ABE 325

Lecture 3: Atmospheric Radiative Transfer and Climate

Physics 221, March 22

General Physics (PHY 2130)

Transcription:

Greenhouse Steady State Energy Balance Model The energy balance for the greenhouse was obtained by applying energy conservation to the greenhouse system as a control volume and identifying the energy terms. In this study, the energy storage term in the greenhouse was ignored since the heat capacity of internal air and plants was small compared to the existing fluxes (Walker, 1965 and Kindelan, 1980). The air in each defined zone in the greenhouse was assumed to be well mixed resulting in no spatial variation in temperature. The greenhouse surface and the surrounding were assumed gray bodies and the sky was at sky temperature. Also, it was assumed that the greenhouse ground was completely covered with plants. During the periods of high solar radiation when ventilation was required, the heat loss to ground, the heat of respiration and heat utilized in photosynthesis were assumed to be very small compared to other fluxes and were neglected (Walker, 1965). The cover was assumed to be double layer polyethylene. Neglecting the rate of change of energy stored in the greenhouse and other small fluxes, the energy balance equation for the greenhouse was written as: 0 = Q sr - Q e - Q cd - Q v - Q t (1) where Q sr was the amount of direct and diffuse shortwave solar radiation in the greenhouse (W), Q e was the latent heat energy flux due to plant transpiration (W), Q cd was the conduction heat transfer through the greenhouse covering material (W), Q v was the energy removed by ventilation air (W), and Q t was the net thermal radiation through the 1

greenhouse covers to the atmosphere (W). Each term was defined by a relationship. The variable Q sr was expressed as: Q sr = τ c S l I sr A f (2) where τ c was the transmissivity of the greenhouse covering materials for solar radiation, S l was the shading level, I sr was the amount of solar radiation energy received per unit area and per unit time on a horizontal surface outside the greenhouse (W/m 2 ), and A f was the floor area of the greenhouse (m 2 ). The variable Q e in equation (1) was expressed as: Q e = ET L v A f (3) Where ET was rate of transpiration (Kg H2O /sec.m 2 ) and L v was latent heat of vaporization of water (J/Kg H2O ). The variable Q cd in equation (1) was defined by the following relationship: Q cd = U A c (T i - T o ) (4) where U was the heat transfer coefficient (W/m 2 o C), A c was area of the greenhouse covers (m 2 ), T i was the inside air temperature ( o C), and T o was the outside air temperature ( o C). Since the transmitted thermal radiation loss was considered separately and not included as a part of the U value for conduction heat loss, U was given the value of 2.73 W/m 2 o C (ASHRAE guide and data book fundamentals, 1981) The variable Q v in equation (1) was expressed as: Q v = V va (1/v) C p (T i - T o ) (5) where V va was the volumetric ventilation rate (m 3 /s), v was the specific volume of air 2

(m 3 /kg), and C p was the specific heat of air (J/Kg o C). When the evaporative cooling system was used, T o in equation (5) was the temperature of the air leaving the cooling system. It was expressed as: T e = T o - η(t 0 - T wb ) (6) The variable Q t was the difference between the thermal radiation emitted from the surface and the thermal radiation gained from the atmosphere such that: Q t = σ A f τ tc τ os ( ε i T 4 i - ε sky T 4 sky ) (7) where σ was the Stefan-Boltzmann's constant (5.67 x 10-8 W/m 2.K 4 ), τ tc and τ os were the transmissivities of the thermal radiation for the double layer polyethylene and the shading material, respectively, ε i was the average emissivity of the interior surface, and ε sky was the apparent emissivity of the sky. The emissivity of the sky was evaluated by the following equation (Idso, 1981): ε sky = 0.70 + 5.95E-7 * e 0 * exp (1500/T o ) (8) where e(t o ) and T o were ambient vapor pressure and temperature at a standard height in Pa. and K, respectively. The sky temperature was approximated by the Swinbank model (1963) as a function of outside air temperature (T o in unit of Kelvin): T sky = 0.0552 * (T o ) 1.5 (9) Substituting equations (2-5) into equation (1), and expressing each term per unit floor area yielded: I sri = ET L v + a (T i - T o ) + V va b (T i - T e ) + Q t /A f (10) where V va was the volumetric ventilation rate (m 3 /s.m 2 of floor area), a = UA c /A f, b = 3

(1/v)C p, T e = T o when the natural or fan ventilation was used without evaporative cooling, and I sri = τ c S l I sr. Then, an expression for the interior temperature was derived as: T i = [I sri - Q t /A f + (a T o + b V va T e ) - ET L v ] / (a + b V av ) (11) It is clear from equation (11) that the variables affecting inside greenhouse temperature (T i ) were the inside solar radiation (I sri ), outside temperature (T o ), transpiration rate (ET), and ventilation rate (V va ). Greenhouse Steady State Mass Balance Model To evaluate the inside relative humidity for a given ventilation rate and a rate of moisture production, a mass balance calculation was performed. In this study, it was assumed that moisture loss from the air by condensation on the surfaces was small and was neglected. Also, the plant transpiration was assumed to be the only source of moisture production in naturally and fan ventilated greenhouses. When the evaporative cooling system was used, additional moisture was added to the greenhouse environment by the cooling system. The overall mass balance was: M v = M et (12) where M v was the amount of moisture transferred from the inside air to the outside air via ventilation (Kg H2O /s), which was expressed as: M v = (1/v) V a (w i - w 0 ) (13) 4

where w i and w 0 were the humidity ratios of the inside and outside air, respectively, in Kg H2O /Kg dry air. The variable M et in equation (13) was the amount of moisture added by transpiration (Kg H2O /s). The relationship for relative humidity (RH) expressed as a percent was given by the equation: RH = [e(t) / e * (T)] *100 (14) where e(t) was the partial pressure of the water vapor in moist air (Pa) and e * (T) was the saturation vapor pressure (Pa). The partial pressure of water vapor was defined by: e(t) = (w + P atm )/(w + 0.622) (15) where P atm was the atmospheric pressure (Pa). The saturation vapor pressure for a given temperature was computed with the equation given by ASHRAE Handbook of Fundamentals, (1993): e * (T) = exp [ -5800.2206/T + 1.3914993-0.04860239 T + 0.41764768E-4 T 2-0.14452093E-7 T 3 + 6.5459673 ln (T) ] (16) where T was in K and e(t) was in Pa. Water use during the mass transfer process between the air and water for the evaporative cooler was evaluated by the steady flow mass balance equation: m a w o + m w = m a w e (17) where m w was the evaporative cooling system water intake (Kg H2O /s), m a was the mass flow rate of the outside air through the cooling system (Kg dry air /s), and w e was the 5

humidity ratio of the leaving air passed through the cooling system (Kg H2O /Kg dry air ). Therefore, m w = m a ( w e - w o ) (18) or m w = (1/v) V av ( w e - w o ) (19) Equation (19) can be used to evaluate the water evaporation rate in the evaporative cooling system for a given air flow rate through the greenhouse. However, a general formula for water intake for the cooling system as a function of outside conditions needed to be evaluated. Cooling load of the evaporative cooling system of a greenhouse was expressed as: Q v = Q sr - Q e - Q cd - Q t (20) The volumetric ventilation rate with an average inside design temperature was defined as: V va = [I sri - Q t /A f - a (T i T o ) - ET L v ] /b (T i - T e ) (21) where a and b were described in equation (10). Since the evaporative cooling process is an adiabatic exchange of heat, the amount of sensible heat removed from the air equals the amount of heat absorbed by the water evaporated as latent heat of vaporization. Therefore, the difference (w e -w o ) was expressed as: (w e - w o ) = C p /L v (T 0 - T e ) (22) Substituting equations (22) and (21) in equation (19) yielded: m w = {[I sri - Q t - a (T i - T 0 ) - ET L v ] /(T i - T e )} d (T 0 - T e ) (23) 6

where d=1/l v. In Equation (23), water intake by the evaporative cooling system was a function of solar radiation, ambient and inside temperatures. LIST OF REFERENCES ASHRAE guide and data book fundamentals. 1981. American Society of Heating, Refrigerating and Air-conditioning Engineers. New York ASHRAE guide and data book fundamentals (SI edition). 1993. American Society of Heating, Refrigerating and Air-conditioning Engineers. New York Idso, S. B. 1981. A set of equations for full spectrum and 8-μm to 14-μm and 10.5-μm to 12.5-μm thermal radiation from cloudless skies. Water Resources Res. 17: 295-304. Kindelan, M. 1980. Dynamic modeling of greenhouse environment. Transactions of the ASAE, 23:1232-1239. Walker, J. N. 1965. Predicting temperatures in ventilated greenhouses. Transactions of the ASAE 8(3): 445-448. 7