ATMOSPHERE M E T E O R O LO G Y

Similar documents
Unit 3 Review Guide: Atmosphere

The Atmosphere. Chapter Test A. Multiple Choice. Write the letter of the correct answer on the line at the left.

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

The troposphere is the layer closest to Earth s surface. Extends from 9-16 km above Earth s Surface It contains most of the mass of the atmosphere.

The Earth s Atmosphere-II. GEOL 1350: Introduction To Meteorology

The Atmosphere EVPP 110 Lecture Fall 2003 Dr. Largen

Common Elements: Nitrogen, 78%

Atmospheric Layers. Ionosphere. Exosphere. Thermosphere. Mesosphere. Stratosphere. Troposphere. mi (km) above sea level 250 (400) 50 (80) 30 (50)

Science 1206 Unit 2: Weather Dynamics Worksheet 8: Layers of the Atmosphere

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? About 10 km thick

Unit 2 Meteorology Test **Please do not write on this test** 5. El Nino & La Nina 6. Photosynthesis 7. Coriolis Effect 8.

Section 2: The Atmosphere

Name Class Date STUDY GUIDE FOR CONTENT MASTERY

Atmosphere & Heat Transfer Basics Notes

Characteristics of the Atmosphere

Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

Chapter 9 Atmosphere Study Guide

The Atmosphere - Chapter Characteristics of the Atmosphere

The Atmosphere. Characteristics of the Atmosphere. Section 23.1 Objectives. Chapter 23. Chapter 23 Modern Earth Science. Section 1

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres

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

EARTH'S ATMOSPHERE. 1. The graph below shows the average concentration of ozone in Earth's atmosphere over Arizona during 4 months of the year.

The Atmosphere. 1 Global Environments: 2 Global Environments:

Space Atmospheric Gases. the two most common gases; found throughout all the layers a form of oxygen found in the stratosphere

ESS 111 Climate & Global Change. Week 1 Weather vs Climate Structure of the Atmosphere Global Wind Belts

Earth s Atmosphere. Composition

surrounds Earth and protects it somewhat from solar radiation. Like all other matter, air has weight,

Average Temperature Readings at Various Altitudes

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Layers of the Atmosphere

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

Earth s Atmosphere About 10 km thick

LAB 3: Atmospheric Pressure & Moisture

Meteorology. I. The Atmosphere - the thin envelope of gas that surrounds the earth.

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

The Atmosphere of Earth

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Characteristics of the Atmosphere

1. CLIMATOLOGY: 2. ATMOSPHERIC CHEMISTRY:

K32: The Structure of the Earth s Atmosphere

Thickness of the Atmosphere

2/22/ Atmospheric Characteristics

The Transfer of Heat

Lecture Outlines PowerPoint. Chapter 16 Earth Science 11e Tarbuck/Lutgens

METEOROLOGY A SCIENCE ACTIVITY BOOK

9.5 Troposphere. Describe the characteristics and importance of the troposphere. Explain temperature inversion and its role in the troposphere.

ROYAL CANADIAN AIR CADETS PROFICIENCY LEVEL THREE INSTRUCTIONAL GUIDE SECTION 1 EO M DESCRIBE PROPERTIES OF THE ATMOSPHERE PREPARATION

Atmosphere : Properties and Standard Atmosphere

The Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Weather vs Climate! What!are!the!!four!factors!that!determine!weather?!!

Unit 3: 4/14/2015. Meteorology. Meteorologist. Research. The Earth s Atmosphere How do we collect information on the atmosphere?

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens

2010 Pearson Education, Inc.

Temperature Pressure Wind Moisture

Atmospheric Basics Atmospheric Composition

WATER IN THE ATMOSPHERE

Our Atmosphere as seen from the bottom of it near Grand Pre, NS. Info modified from various sources by TWebb HHS

COMPOSITION OF THE ATMOSPHERE

The Atmosphere Made up of mainly two gases: Nitrogen 78% Oxygen 21% Trace Gases 1%

WEATHER. Review Note Cards

Energy Transfer in the Atmosphere

Final Weather Unit Study Guide

I T A T I O N H B I T B T V A O C J K M R S A T M O S P H E R E

Unit 5. Seasons and Atmosphere

WO2 ROZSA-HRABINSKI METEOROLOGY 1

Website Lecture 3 The Physical Environment Part 1

The Study of the Atmosphere

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement

Chapter 9 External Energy Fuels Weather and Climate

Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414)

Atmospheric circulation

Chapter 15 The Atmosphere and Weather

Meteorology Practice Test

In the space provided, write the letter of the description that best matches the term or phrase. as waves. thermosphere

Your web browser (Safari 7) is out of date. For more security, comfort and the best experience on this site: Update your browser Ignore

Atmospheric Structure

INTRODUCTION TO METEOROLOGY PART TWO SC 208 DECEMBER 2, 2014 JOHN BUSH

Week: Dates: 3/2 3/20 Unit: Climate

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement

Atmosphere. Earth's atmosphere is a mixture of gases, solids, and liquids that surround the planet.

The Atmosphere and Atmospheric Energy Chapter 3 and 4

10.1 TEMPERATURE, THERMAL ENERGY AND HEAT Name: Date: Block: (Reference: pp of BC Science 10)

The Layered Atmosphere:

2. What are the four most common gasses in the atmosphere and their percentages?

Weather Part I- Weather Variables

IV. Atmospheric Science Section

CLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1

1 Characteristics of the Atmosphere

WOULD THERE BE WIND IF THE EARTH S TEMPERATURE WAS THE SAME EVERYWHERE? ANSWER IN PARAGRAPH FORM AND PROVIDE EVIDENCE TO DEFEND YOUR ANSWER.

General Comments about the Atmospheres of Terrestrial Planets

Science Chapter 13,14,15

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves

Unit 2: The atmosphere

Outline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued

Name Period Date L.O: SWBAT DESCRIBE THE PROPERTIES OF THE ATMOSPHERE.(

Name Team Period. Station #1 (drawing)

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

Goal 2.5. The Atmosphere

Climate & Earth System Science. Introduction to Meteorology & Climate CHAPTER 1 LECTURE 1. Question: Introduction to the Atmosphere

Transcription:

1.05.01 ATMOSPHERE 1. 0 5 M E T E O R O LO G Y

INTRODUCTION ATMOSPHERIC COMPOSITION The atmosphere of Earth is the layer of gases, commonly known as air, that surrounds the planet Earth and is retained by Earth's gravity The atmosphere becomes thinner and thinner with increasing altitude, with no definite boundary between the atmosphere and outer space Several layers can be distinguished in the atmosphere, based on characteristics such as temperature and composition The atmosphere of Earth protects life on Earth by creating pressure allowing for liquid water to exist on the Earth's surface, absorbing ultraviolet solar radiation, warming the surface through heat retention (greenhouse effect), and reducing temperature extremes between day and night

CHEMICAL COMPOSITION ATMOSPHERIC COMPOSITION The three major constituents of air, and therefore of Earth's atmosphere, are nitrogen, oxygen, and argon By volume, dry air contains 78% nitrogen, 20.9% oxygen, 0.9% argon, 0.03% carbon dioxide, and small amounts of other gases

ATMOSPHERE LAYERS STRUCTURE OF THE ATMOSPHERE Atmosphere consists of layers of air masses separated by physical properties (mainly by temperature). Main layers of atmosphere (excluding exosphere) are: Thermosphere: from mesopause to 500 ~ 1000 km (1 600 000 ~ 3 300 000 ft) Mesosphere: from stratopause to 80 ~ 85 km (260 000 ~ 280 000 ft) Stratosphere: from tropopause to 50 ~ 55 km (50 to 55 km (164 000 ~ 180 000 ft) Troposphere: extends from surface to 9 ~ 17 km (36 000 ~ 56 000 feet)

TROPOSPHERE STRUCTURE OF THE ATMOSPHERE The lowest layer of Earth's atmosphere extends from earth surface up to 12 km on average - 9 km on poles and to 17 km on equator (36 000-56 000 feet) The troposphere is bounded above by the tropopause, a boundary marked in most places by a temperature inversion (in troposphere temperature drops to -56.5 C (- 68.8 F) and goes up in stratosphere) 50% of the total mass of the atmosphere is located in the lower part (5.6 km or 18,000 ft) of the troposphere. It is most dense part of the atmosphere All atmospheric water vapor or moisture is found in the troposphere our weather is happening only in this layer 15 C (59 F)

STRATOSPHERE STRUCTURE OF THE ATMOSPHERE Stratosphere extends from tropopause up to 50 ~55 km 164 000 ~ 180 000 ft The atmospheric pressure at the top of the stratosphere is roughly 1/1000 the pressure at sea level temperatures rises with increasing altitude from -56.5 C (- 68.8 F) to 0 C (32 F) at the top of layer. This rise in temperature is caused by the absorption of ultraviolet radiation (UV) from the Sun by the ozone layer situated in stratosphere. The stratospheric temperature profile creates very stable atmospheric conditions - the stratosphere is almost completely free of clouds and other forms of weather.

80 85 km MESOSPHERE STRUCTURE OF THE ATMOSPHERE Mesosphere the layer above the stratosphere 50 km (160,000 ft) and below the thermosphere 80~85 km (260,000~280,000 ft) Temperatures drop with increasing altitude to the mesopause that marks the top of this middle layer of the atmosphere. It is the coldest place on Earth and has an average temperature around 85 C ( 120 F) mesopause stratopause tropopause noctilucent clouds 50 55 km -85 C ( 120 F) 0 C (32 F) -56.5 C (-68.8 F) thermospher e Mesosphere ozone layer stratosphere troposphere The air so low that very scarce water vapor at this altitude can be sublimated into polar-mesospheric noctilucent clouds

80 85 km THERMOSPHERE STRUCTURE OF THE ATMOSPHERE exosphere It extends from the mesopause (which separates it from the mesosphere) at an altitude of about 80~85 km (260,000~280,000 ft) up to the thermopause at an altitude range of 500 1000 km (1 600 000 3 thermopause 500 1000 km 1500 C (2700 F) thermosphere 300 000 ft) where the exosphere begins The temperature of this layer can rise as high as 1500 mesopause -85 C ( 120 F) Mesosphere C (2700 F) because of very low density of the gas stratosphere in the layer

ICAO STANDARD ATMOSPHERE PHYSICAL PROPERTIES At mean sea level (MSA): Temperature - 15 C (59 F) Temperature lapse rate 1.98 C per 1000ft Pressure 1013.25 hpa (29.92 Hg) Pressure lapse rate 1 hpa per 30ft Density - 1.225 kg/m3 STANDARD ATMOSPHERE

GAS PHYSICAL PROPERTIES Air is a mix of gases, containing particles (molecules), and these particles are moving bouncing with each other. The velocity with witch particles move related with particles kinetic energy. Increasing temperature causes faster movement of particles and demands more space for them - therefore gas takes more volume in the same pressure and become less dense. Decreasing in temperature makes particles move slower and gas shrinks and takes less volume in the same pressure

GAS FORMULA PHYSICAL PROPERTIES Formula, bringing relation between temperature (T), pressure (P) and volume (V): P*V = n*r*t (n amount of gas in moles; R gas constant) In other words, pressure and volume of gas directly proportional to its temperature, for example, if you fix volume, then increasing T will increase pressure; if you fix pressure, increasing T will increase volume. Proportion of the given gas always the same. gas expands with increasing temperature and shrinks with decreasing temperature

TEMPERATURE U.M. PHYSICAL PROPERTIES Temperature - is a way the express how subject is hot or cold (how many kinetic energy has the amount of gas). Temperature is measured in different units of measurements like: K (Kelvin) - SI (international system of units) F (Fahrenheit) used in US mostly C (Celsius) - commonly used in the rest of world To Fahrenheit from Celsius: [ F] = [ C] 9 5 + 32 To Celsius from Fahrenheit: [ C] = ([ F] 32) 5 9 To Kelvin from Celsius: [K] = [ C] + 273.15 To Celsius from Kelvin: [ C] = [K] 273.15

TEMPERATURE LAPS RATE PHYSICAL PROPERTIES In troposphere temperature gradually drops from 15 C (59 F) on the MSA to -56.5 C (-68.8 F) with gradient of 1.98 C per 1000 ft up to altitude of 36 000 ft This is ISA (environmental) temperature laps rate

DRY ADIABATIC LAPS RATE PHYSICAL PROPERTIES In real dry air temperature lapse rate is 3.05 C per 1000 ft Non condensed water vapor does not affect cooling process, air cools easily It is dry adiabatic lapse rate

DEW POINT LAPS RATE PHYSICAL PROPERTIES When water vapor starts condensing, vapor condensation process release lantern heat and cooling gradient slows Until water vapor is not fully condensed, temperature lapse rate is 0.57 C per 1000 ft It is dew point lapse rate Lifting condensation level level where water vapor condensation begins

WET ADIABATIC LAPS RATE PHYSICAL PROPERTIES When water vapor fully condensed, water had released its lantern energy and starts cooling with air again. Temperature gradient increases again. Temperature lapse rate is 1.52 C per 1000 ft It is wet adiabatic lapse rate

HADLEY CELLS AIR CIRCULATION Temperature on equator much higher than on poles. Masses of hot less dense air raises up creating low pressure areas On the upper level of atmosphere air cools down and moves down on poles creating high pressure areas Differential in pressure on the surface creates flow of masses of the air from poles to equator This movement creates planetary circulation of the air masses called Hadley cell

HADLEY CELLS AIR CIRCULATION But because of more complicated processes on planet (involving planet rotation and placement of continents on the earth) this circulation divided on 3 segments on each semisphere: Hadley cell most intensive Ferrel cell circulation on opposite direction Polar cell less intensive circulation in same as Hadley cell direction

CORIOLIS EFFECT AIR CIRCULATION Coriolis effect deflects direction of movement of the masses of the air flowing from poles to equator to westbound for Hadley and polar cells For Ferrel cells Coriolis effect deflect direction to eastbound In northern hemisphere wind is always deflected to the right; in southern to the left NP L L H H H H 60 N 30 N Equator This creates a map of common wind directions on planet for different latitudes and directs rotation of cyclones and anticyclones: Rotation of Earth H H H H L L 30 S Cyclone type Northern hemisphere Southern hemisphere L (anticyclone) anticlockwise clockwise SP 60 S H (cyclone) clockwise Anticlockwise

Please visit Q/A section to prepare to the theory examination Thank you! 1.05 METEOROLOGY