· Are human activities responsible for the warming? Separating out the impact of human activity from natural climate variation is extremely difficult.

Slides:



Advertisements
Similar presentations
Earth Science 17.1A Atmosphere Characteristics
Advertisements

CALEB BRITISH ACADEMY LAGOS NIGERIA. Earth’s temperature depends on the balance between energy entering and leaving the planet’s system.energy entering.
Objectives Describe the composition of Earth’s atmosphere.
 The atmosphere is a layer of gases that surround the Earth.  These layers differ in temperature, in density, and in the relative amounts of the different.
Weather World Geography Notes 1.5. Atmosphere Atmosphere is a thin layer of gases This protects the surface from Temperature extremes (acts as insulation)
Climate Change Myths and Educational Resources 2010 Satellites Educators Conference.
Handout (yellow) Solar Energy and the Atmosphere Standard 3 Objective 1 Indicators a, b, and c Standard 3 Objectives 1, 2, and 3 Workbook Pages 3,
GREENHOUSE EFFECT Climate Change. Greenhouse Effect Is a natural process that permits the Earth to retain some of the heat from the sun. Gases in the.
Warm Up 3/4/08 True or False: The seasons are caused by changes in Earth’s distance from the sun. False Does land or water heat more rapidly? Land heats.
Solar Energy & the Atmosphere
Conservation.
Earth’s Atmosphere Ch. 22.
The Greenhouse Effect A hot topic…. Energy that drives the Greenhouse Effect starts as solar energy from the sun. The shortwave thermal energy reaches.
Chapter 17.1 Atmospheric Characteristics
The Greenhouse Effect *The earth is similar to a greenhouse. The earth atmosphere acts like the glass in a greenhouse. *Sunlight streams through the.
Climate Change. Greenhouse Effect Earth would be too cold to live on without the Greenhouse Effect Greenhouse gases are carbon dioxide, water vapor, methane,
Welcome Back Write down the 4 layers of the atmosphere (in order) and 1 fact about each.
Lecture Outlines Physical Geology, 14/e Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Plummer, Carlson &
Ch Solar Energy and the Atmosphere
The Atmosphere.
Major Factors affecting climate
GREENHOUSE EFFECT BY: EDGAR B., LUIS C., FERNANDO O., ADAMARI ARVAYO.
EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens 
The Atmosphere: Structure and Temperature
The Atmosphere: Energy Transfer & Properties Weather Unit Science 10.
Energy in the Atmosphere
Conversations with the Earth Tom Burbine
Atmosphere: Structure and Temperature Bell Ringers:  How does weather differ from climate?  Why do the seasons occur?  What would happen if carbon.
Atmosphere Test Review
The Atmosphere Preview Section 2 Atmospheric Heating Concept Mapping.
17.1 Atmosphere Characteristics
The AtmosphereSection 1 Layers of the Atmosphere 〉 What are the parts of Earth’s atmosphere? 〉 The atmosphere has several layers. These layers differ in.
Bell work How is food heated in an oven? How is food heated on a range top?
Chapter 22 Section 2 Handout
Incoming & Outgoing of Energy of the Earth. The Earth’s Energy Balance The Earth's average temperature remains fairly constant from year to year. Therefore,
Heat in the Atmosphere The sun’s energy is transferred to earth and the atmosphere three ways Radiation, Convection and Conduction.
The Atmosphere: Structure and Temperature
Solar Energy and the Atmosphere
1. The atmosphere 2 © Zanichelli editore 2015 Characteristics of the atmosphere 3 © Zanichelli editore 2015.
17 Chapter 17 The Atmosphere: Structure and Temperature.
Earth and sky, woods and fields, lakes and rivers, the mountain and the sea, are excellent schoolmasters, and teach some of us more than we can ever learn.
Section 1.3 Gases in the atmosphere absorb radiation.
Composition of the Atmosphere 14 Atmosphere Characteristics  Weather is constantly changing, and it refers to the state of the atmosphere at any given.
Earth’s Atmosphere. The Air Around You Weather- the condition of Earth’s atmosphere at a particular time Atmosphere- envelope of gases that surrounds.
The Dynamic EarthSection 2 Objective #9 Describe the layers of the Earth’s atmosphere.
The Dynamic EarthSection 2 WATCH?V=RIHRI_Z2KGS&FEA TURE=RELMFU&SAFE=ACTIV E.
Students type their answers here
Climate Change: Impacts and Responses Topic 2: The Earth's Climate System 1.
17 Chapter 17 The Atmosphere: Structure and Temperature.
Climate Change. Causes Several factors affect global climate: 1.Changes in solar output 2.Changes in Earth's orbit 3.Changes in the distribution of continents.
Atmospheric Heating Radiation Conduction Convection.
Warmup What are three natural ways in which climate changes? What timescale do these processes generally occur?
The Atmosphere: Structure & Temperature. Atmosphere Characteristics Weather is constantly changing, and it refers to the state of the atmosphere at any.
The AtmosphereSection 1 Section 1: Characteristics of the Atmosphere Preview Key Ideas Bellringer Layers of the Atmosphere Changes in Earth’s Atmosphere.
Atmospheric Heating.
Guided Notes about the Earth’s Atmosphere
The Atmosphere: Structure & Temperature
The Greenhouse Effect 8.6 The greenhouse effect is a natural process whereby gases and clouds absorb infrared radiation emitted by Earth’s surface and.
Heat in the Atmosphere.
Solar Energy and the Atmosphere
Gases in the Atmosphere absorb Radiation
ATMOSPHERE.
The Atmosphere Earth’s atmosphere is a mixture of gases that distributes heat and enables life to exist on Earth.
Earth's atmosphere reflects or absorbs some sunlight but allows most of the visible light pass through to Earth's surface. 4 ways the atmosphere affects.
Journal #25 What is a greenhouse? What is the greenhouse effect?
Earth's atmosphere reflects or absorbs some sunlight but allows most of the visible light pass through to Earth's surface. Atmosphere affects light in.
Atmosphere 1.3 RSG-B Answers.
Climate Earth’s Energy Budget.
The Structure of the Atmosphere
Presentation transcript:

· Are human activities responsible for the warming? Separating out the impact of human activity from natural climate variation is extremely difficult. Nonetheless, the IPCC concluded there is a 'discernible human influence' on climate. This means the observed global warming is unlikely to be the result of natural variability alone and that human activities are at least partially responsible.

· What Role does Solar Radiation play in Determining the Earth's Climate? Energy or solar radiation enters the atmosphere as sunshine. The sky reflects a portion of this radiation, the rest is absorbed by the Earth and is eventually released again as thermal radiation. Both man-made and naturally occurring events can limit the amount of solar radiation at the earth's surface. Urban air pollution, smoke from forest fires, and airborne ash resulting from volcanic activity reduce the solar resource by increasing the scattering and absorption of solar radiation. Some scientists think of the radiation budget in terms of a balance. If the Earth gets more energy from the Sun, the Earth heats up and emits more thermal energy. This brings the radiation budget into balance. If the Earth emits more of this thermal energy than it absorbs from solar radiation, the Earth cools off. As it cools off, the Earth emits less energy. This change also brings the radiation budget back into balance.

Ozone depletion describes two distinct but related phenomena observed since the late 1970s: a steady decline of about 4% per decade in the total volume of ozone in Earth's stratosphere (the ozone layer), and a much larger springtime decrease in stratospheric ozone over Earth's polar regions. The latter phenomenon is referred to as the ozone hole. In addition to these well- known stratospheric phenomena, there are also springtime polar tropospheric ozone depletion events

· How are the amounts of greenhouse gases measured? Non-isotopic measurements of greenhouse gases are generally made with two techniques: Non-Dispersive Infrared (NDIR) analysis, or by gas chromatography. The amount of CO2 in the atmosphere is large enough that the NDIR method of measurement works well. An NDIR analyzer relies on the same principle of IR absorption that makes greenhouse gases important in the first place. An infrared analyzer consists of an infrared source at one end, and an infrared detector separated by a gas cell. The gas of interest is passed through this cell, and absorbs some of the infrared radiation coming from the source. The detector converts the amount of IR reaching it to a usable signal, such as a voltage. So as the concentration of CO2 changes in the sample, the signal from the detector changes. By flowing a gas with a known amount of CO2 through the cell, we can calibrate the analyzer so that the voltage output from the detector can be converted into amounts of CO2.

· Where are these gases measured? GMD's Carbon Cycle group (CCGG) makes continuous and discrete measurements of greenhouse gases at numerous worldwide surface sites, towers, aircraft, and ships of opportunity. There is a world map of the many different sampling sites. Air samples are collected in glass flasks from sampling sites of the NOAA GMD CCGG Cooperative Air Sampling Network and returned to the CCGG laboratory in Boulder, Colorado for analysis. In-Situ, continuous measurements are made at the 4 baseline GMD Observatories, and at 2 tall tower sites in the United States

· How much CO 2 is in the atmosphere? For the year 2006, the estimated global average CO 2 amount was about 381 parts per million (ppm). If we use a value of 5.13 ×10 18 kg for the mass of the dry atmosphere (excluding water vapor), and take into account that the average molecular weight of air equals 29.0 g/mole and the atomic weight of carbon 12.0 g/mole, then 1 ppm of CO 2 corresponds to 2.12 Gt (billion metric ton) of carbon. This gives us a value of about 808 Gton of carbon in the atmosphere. If we include the mass of the two oxygen atoms in each CO 2 molecule, the total mass of CO 2 would be 2960 Gton. Watch out: in the news and in reports you may see emissions expressed either as tons of carbon or as tons of carbon dioxide. The latter is 3.67 times heavier than the former, although the same number of CO 2 molecules is involved