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

Similar documents
Level 3 Earth and Space Science, 2017

Chapter 9 Atmosphere Study Guide

IV. Atmospheric Science Section

Unit 3 Review Guide: Atmosphere

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

Atmospheric circulation

The Atmosphere - Chapter Characteristics of the Atmosphere

CHAPTER 6 Air-Sea Interaction Pearson Education, Inc.

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

2010 Pearson Education, Inc.

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

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

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

The Transfer of Heat

ATMOSPHERE PACKET CHAPTER 22 PAGES Section 1 page 546

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

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

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

Chapter 4 Lesson 1: Describing Earth s Atmosphere

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

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

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

,Solar Energy, Greenhouse effect, Convection.notebook October 31, 2016

Section 2: The Atmosphere

Earth s Atmosphere. Energy Transfer in the Atmosphere. 3. All the energy from the Sun reaches Earth s surface.

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

Day 1 of Global Warming. Copyright 2008 Pearson Education, Inc., publishing as Pearson Benjamin Cummings

2. Fargo, North Dakota receives more snow than Charleston, South Carolina.

Topic # 11 HOW CLIMATE WORKS continued (Part II) pp in Class Notes

Thermal / Solar. When air is warmed it... Rises. Solar Energy. Evaporation. Condensation Forms Clouds

1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely

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

COMPOSITION OF THE ATMOSPHERE

FORCING ANTHROPOGENIC

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

Topic # 12 How Climate Works

Topic # 12 Natural Climate Processes

Chapter 9 External Energy Fuels Weather and Climate

Website Lecture 3 The Physical Environment Part 1

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

General Comments about the Atmospheres of Terrestrial Planets

Short-Term Climate Variability (Ch.15) Volcanos and Climate Other Causes of Holocene Climate Change

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

Key Concept Heat in Earth s atmosphere is transferred by radiation, conduction, and convection.

Fluid Circulation Review. Vocabulary. - Dark colored surfaces absorb more energy.

Atmosphere. Transfer in the Atmosphere

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

5.1. Weather, climate, and components of the climate system

Science 1206 Chapter 1 - Inquiring about Weather

The Atmosphere and Atmospheric Energy Chapter 3 and 4

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

Clouds and Rain Unit (3 pts)

Climate. Energy & Wind Masses. Ocean Explorer Module 5

COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION

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

The Atmosphere EVPP 110 Lecture Fall 2003 Dr. Largen

Troposphere and mesosphere Stratosphere and thermosphere radio

WEATHER. Review Note Cards

NATURAL CLIMATIC FORCING Part II

Torben Königk Rossby Centre/ SMHI

Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate

2/22/ Atmospheric Characteristics

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

The Structure and Motion of the Atmosphere OCEA 101

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week

Atmosphere - Part 2. High and Low Pressure Systems

Ocean s Influence on Weather and Climate

Topic # 11 HOW CLIMATE WORKS PART II

Energy Transfer in the Atmosphere

Name Period Date 8R MIDTERM REVIEW I. ASTRONOMY 1. Most stars are made mostly of. 2. The dark, cooler areas on the sun s surface are

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

The Atmosphere. Composition of the Atmosphere. Section 2

The Atmosphere. 1 Global Environments: 2 Global Environments:

1. The and the act as one interdependent system. 2. Why do we have to study both to understand the relationship?

The Atmosphere of Earth

Multiple Choice Identify the choice that best completes the statement or answers the question.

Overview Atmosphere. Meeting Individual Needs. Directed Reading for Content Mastery

Meteorology Study Guide

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

Environmental Science Chapter 13 Atmosphere and Climate Change Review

UNIT TEST PRACTICE TEST

Science Chapter 13,14,15

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

Energy Efficiency Review

Name Class Date STUDY GUIDE FOR CONTENT MASTERY

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

ATMOSPHERE M E T E O R O LO G Y

Level 3 Earth and Space Science, 2014

1 Our Dynamic Climate Guiding Question: What factors determine Earth s climate?

Wednesday February 1 st, Daily Science: How are the upper and the lower part of the stratosphere different?

A) usually less B) dark colored and rough D) light colored with a smooth surface A) transparency of the atmosphere D) rough, black surface

GEO1010 tirsdag

Surface Processes and the Hydrosphere Unit Heating the Earth s Atmosphere Chapter 11 (pg )

The Atmosphere. All weather occurs here 99% of water vapor found here ~75 % of total mass of the atmosphere

Atmosphere Weather and Climate

Concepts of energy and heat

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

Transcription:

NCEA Level 3 Earth and Space Science (91414) 2017 page 1 of 6 Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414) Evidence Statement Q Evidence Achievement Merit Excellence ONE Convection Cell A convection cell is a circulation caused by density differences within a body of air (liquid / gas) where warmer less dense air rises and cooler, denser air drops. Role of solar radiation and Earth s rotation Air mass movement is driven by the energy from the Sun at the surface, as warm air rises and colder air sinks. Unequal heating of the Earth s surface is the main driver; the Equator receives more heat than the poles, causing the warm air to rise, while the cold dense air at the poles sinks and moves towards the Equator, replacing the warm air that has risen. The rotation of the Earth causes the Coriolis effect, which is the apparent deflection of air currents towards the right in the Northern Hemisphere and left in the Southern Hemisphere. The result of this is to break the air circulation into three convective cells. Formation of Cells Hadley The circulation of air mass closest to the Equator is the Hadley cell. This air mass rises at or near the Equator rapidly due to the intensity of the Sun s radiation on this part of the Earth s surface. This creates a low pressure zone around this region of the Earth s surface, and certain extreme weather events (e.g. thunderstorms, cyclones). The rising air mass spreads and cools moving in higher altitudes until falling in the region of 30 degrees north or south of the Equator. This falling air mass creates an area of high pressure and subsequently moves across the Earth s surface back toward the Equator or towards the higher latitudes (60 degrees North and South). Label / annotate a diagram showing the convection cells and air movement. A description and / or a labelled diagram of a convection cell. Explains the formation of one cell. Explains the difference between open and closed cells. Describe the uneven heating effect of solar radiation in heating the Earth. Describes the effect of Earth s rotation on surface. Explanation of how a convection cell forms in terms of heating / density differences. Explanation of how the unequal heating of the Earth s surface between the equator the poles leads to the formation of the Hadley and Polar Cells. Explanation of how the Ferrel cell is the result of interaction of air movement between the the Hadley and Polar Cells. Explanation of how air movement is affected by Earth s rotation. Explains the difference between the formation of open and closed cells with reference to examples of each. Comprehensive explanation of how the three cells are formed AND why the Ferrel cell differs from the Hadley and Polar. Ferrel lie between the Hadley and Polar cells (30 to 60 degrees latitude). Some of the sinking air mass at 30 degrees North continues travelling northwards along the Earth s surface towards the pole. This air is still warm as it has originated from the Equator, and at 60 degrees latitude, approaches cold air moving down from the pole. This causes the warm air mass to rise, with some mixing taking place between the two air masses. This is known as the Polar Front, where weather events can originate. At higher altitudes, part of the air mass moves towards the pole, carrying heat energy with it. The heat energy is the result of condensing water vapour (latent heat) that originated from the Equator. The remaining air mass

moves back towards the Equator. Polar lies between the poles and 60 degrees North and South. These are closed cells. Cold, dense air descends over the poles and the cold air is circulated towards the Equator along the Earth s surface. The air from the poles rises at 60 degrees latitude and some of this air returns to the poles at altitude, completing the Polar Cell. Differences between open and closed loop cells Hadley and Polar cells are closed, the Ferrel cell is open. Closed loop cells either have a heat source such as the Equator for the Hadley cell, or a cold heat sink such as the poles for the Polar cells. Either of these things drives convection. The Ferrel cell, which is open, does not have either of these, and as a result air moves in the reverse direction to the other two cells and the cell overlaps with each of the other cells. Annotated diagram NCEA Level 3 Earth and Space Science (91414) 2017 page 2 of 6 Not Achieved Achievement Merit Excellence

NCEA Level 3 Earth and Space Science (91414) 2017 page 3 of 6 N0 = no response; no relevant evidence. N1 = 1 partial point from Achievement. N2 = 1 point from Achievement. A3 = 2 points. A4 = 3 points. M5 = 1 point M6 = 2 points E7 = Point with minor omissions / error. E8 = Point fully Q Evidence Achievement Merit Excellence TWO Aerosols are minute solid and liquid particles suspended in the atmosphere. Types of volcanic aerosol and layer they are found in Volcanic eruptions produce ash, rock fragments, and gases such as sulfur dioxide. Due to its size and mass, volcanic ash rapidly falls out of the atmosphere in rain a few hours or days after the eruption; therefore it does not reach further than the troposphere. If the plume reaches the stratosphere, it may inject sulfur dioxide gas into this layer. When this happens, the sulfur dioxide layer is very quickly converted to droplets of sulfuric acid over the course of a week or several months after the eruption. These sulfuric acid droplets are the aerosol. Once formed, they stay in the atmosphere for approx. two years. Relationship between type of eruption and layers Minor eruptions do not extend high enough into the atmosphere to extend beyond the troposphere. Describes what an aerosol is. Links a type of volcanic aerosol to correct atmospheric layer. Links size of eruption to the effect on the atmospheric layers. Links stratospheric / high level aerosols to global climate variation. Links tropospheric / low level / short lived aerosols to regional climate variation. Explains relationship between type of aerosol particle and the layer it is found in. Explains the effect of volcanic aerosols on regional climate variation. Explains the effect of volcanic aerosols on global climate variation. Explains the relationship between the size of the eruption and the overall climatic effect. Comprehensive explanation of how different types of volcanic aerosols affect BOTH regional and global climate. Explosive eruptions can send up a plume of aerosol particles into the stratosphere. Effect on regional and global climates Volcanic ash released into the atmosphere will cause temporary cooling of the regional climate. This is because these larger aerosol particles fall out of the air quickly. Small ash particles in the troposphere form a dark cloud that shades and cools the area directly below it. These particles do not remain in the troposphere for long, therefore the effect on the climate is very localised and short-lived. (If eruption occurs in the mid to high latitudes, stratospheric aerosols will influence only regional climate, as air is carried only towards the poles.) Stratospheric aerosols influence the global climate system. These aerosols include very fine ash and droplets of sulfuric acid / sulfates, which are formed in the stratosphere. These aerosols form a haze which reflect incoming solar (short wavelength) radiation away from the surface, causing the surface to cool. (They also absorb long wavelength radiation from the Earth s surface). Because these particles stay in the stratosphere for several

years and are moved around by winds in the stratosphere, the effect of the cooling is experienced worldwide. (If eruption occurs at the Equator, global circulation will carry the stratospheric aerosols towards both poles, causing global climatic changes.) NCEA Level 3 Earth and Space Science (91414) 2017 page 4 of 6 Not Achieved Achievement Merit Excellence N0 = no response; no relevant evidence. N1 = 1 partial point. N2 = 1 point from Achievement. A3 = 2 points. A4 = 3 points. M5 = 1 point M6 = 2 points E7 = Point with minor omissions / error. E8 = Point fully

NCEA Level 3 Earth and Space Science (91414) 2017 page 5 of 6 Q Evidence Achievement Merit Excellence THREE Greenhouse Effect The Earth s surface absorbs solar radiation, and then re-radiates infrared radiation back to the atmosphere, where it can be absorbed by clouds and greenhouse gases such as CO 2, H 2 O, methane, CFCs, and nitrous oxide. The greenhouse gas molecules absorb the radiation, and as a result gain energy and speed up, leading to a rise in temperature. The gases eventually radiate some of this energy back to the Earth s surface. Examples of positive feedbacks on the climate system Water vapour warm air can hold more water vapour than cool air can. Therefore, as the temperature increases, the amount of water vapour also increases, causing a greater absorption of solar (short wavelength) radiation, which then leads to a further increase in temperature. Clouds An increase in cloud cover (due to increased levels of water vapour) causes more long wavelength (infrared / terrestrial) radiation to be absorbed, resulting in an increase in global temperature. Annotated diagram showing the greenhouse effect. Explains that the Earth s surface absorbs solar radiation and re-radiates heat. Links increasing greenhouse gases to prevention of atmospheric heat loss. Links greenhouse gas increases to a particular example of a cause of global warming. Links greenhouse gas increases to a particular example of a cause of global cooling. Explains the greenhouse effect. Explains how one feedback system works to enhance global warming. Explains how one feedback system works to negate global warming. Explains how one further feedback system works. A comprehensive explanation of the greenhouse effect and how the feedback loops affect global warming. Melting permafrost when permafrost melts due to increased temperatures, it releases large amounts of methane gas, a type of greenhouse gas, into the atmosphere. By increasing the amount of greenhouse gases, the effect of global warming is increased. Warming oceans cooler water is able to absorb more carbon dioxide than warm water. As temperatures of the ocean increase, less carbon dioxide will be absorbed by the ocean, leading to more carbon dioxide remaining in the atmosphere, amplifying the effect of global warming. Melting sea ice as temperatures rise, sea ice melts. Sea ice has a high albedo; therefore, as it disappears, more solar radiation will be absorbed, causing the global temperatures to increase. Desertification loss of carbon dioxide sink Examples of negative feedbacks on the climate system Clouds as cloud cover increases, more solar radiation is reflected back into space away from the surface of the Earth, helping to cool the global climate. Desertification as temperatures increase, more areas around the Earth will become deserts. Deserts have a high albedo, leading to more solar radiation being reflected away from the surface of the Earth back into space, helping to cool the Earth.

NCEA Level 3 Earth and Space Science (91414) 2017 page 6 of 6 Not Achieved Achievement Merit Excellence N0 = no response; no relevant evidence. N1 = 1 partial point. N2 = 1 point from Achievement. A3 = 2 points. A4 = 3 points. M5 = 1 point M6 = 2 points E7 = Point with minor omissions. E8 = Point fully Cut Scores Not Achieved Achievement Achievement with Merit Achievement with Excellence 0 6 7 12 13 18 19 24