Air B Radiation and Climate. Solar Radiation The sun (Sol) is a huge fusion reactor - combines two nuclei of H to a He atom. – The produces a tremendous.

Slides:



Advertisements
Similar presentations
Energy in the Earth System
Advertisements

Chapter 16: Weather Factors
2.1 Energy in the Atmosphere
P2 Radiation and life Revision by J Bach St. Mary’s school.
KEY CONCEPT pg. 488 Fossil fuel emissions affect the biosphere.
How Does Heat Energy Travel and Insolation
Radiation and Climate The Electromagnetic Spectrum and Solar Radiation 1.
Solar Radiation and the Greenhouse Effect Earth Science Ms. Kurtzweil.
Chapter 23 The Atmosphere
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,
Chapter 2: Weather Factors
Greenhouse Effect How we stay warm. The Sun’s energy reaches Earth through Radiation (heat traveling through Space)
Solar Energy & the Atmosphere
Key Words radiation budget electromagnetic spectrum albedo Understand the concept of radiation and heat exchange Outline factors that control incoming.
P2. EM radiation Movement of energy in the form of a wave Movement of energy NOT matter Energy moves in packets called photons High frequency EM waves.
Aim: How is the earth's atmosphere similar to a greenhouse?
CH 24.3 Solar Radiation, Pressure, & Wind. Earth’s Energy Balance Input = Sun’s Energy = (Visible light + some UV) REFLECTED: ~ 25 % by clouds, dust,
Energy from the Sun Radiation is the transfer of energy by electromagnetic waves. Ninety-nine percent of the radiation from the Sun consists of visible.
Ozone & Greenhouse Effect. What is Ozone? Ozone is a molecule that occurs in the Stratosphere Ozone absorbs harmful UV rays from the sun O 3 + uv O 2.
Earth’s Atmosphere Ch. 22.
Greenhouse Effect - Natural Heating of Earth’s surface by certain atmospheric gases.
Environmental Chemistry Greenhouse effect, global warming,
Weather Factors Chapter 16.
Objectives Explain how radiant energy reaches Earth.
The Greenhouse Effect A large majority of the insolation that is radiated back into the atmosphere gets absorbed by greenhouse gases. A large majority.
The Greenhouse Effect Too much of a good thing?. Light from the sun is composed of many frequencies.
Climate Change and Greenhouse Effect Notes. What we want to know? What is climate change? What is the greenhouse effect? How will climate change affect.
AIM: What is Global Warming? Do Now: In your notes, discuss what you know about global warming. What causes it? Can it be stopped?
Unit 6.  Climate – the average weather conditions of an area over a long period of time  Weather is the day to day conditions *Climate you expect and.
S6E2.c. relate the tilt of earth to the distribution of sunlight through the year and its effect on climate.
Riddles 1. What has 4 eyes but can’t see?
P2- Radiation and Life. Electromagnetic Radiation Electromagnetic radiation transfers energy is ‘packets’ (photons) Each photon carries energy, the amount.
Global Changes in the Atmosphere
9/24/13 Objective: How are humans impacting the environment? Do Now: What is this picture depicting?
Topic 6 Insolation and the Seasons. Insolation (INcoming SOLar radiATION) Intensity of Insolation depends on the angle of the Sun’s rays, which are due.
Energy in the Atmosphere
Topic 6. Without energy from the sun, conditions on Earth would be different. What is the energy that is radiated from the Sun? The energy that is radiated.
Solar Energy Heat and Light. Energy Can take many different forms –____________ –Heat –____________.
Global Changes in the Atmosphere Pages What is global warming? The gradual increase in the temperature of Earth’s atmosphere Over the last 120.
Greenhouse Effect None Like it Hot. Three primary gases which absorb infrared (IR) energy:
radiation conduction convection Energy Transfer in the Atmosphere stability temperature inversiontemperature inversion.
9/24/14 Objective: How are humans impacting the environment? Do Now: Take out your Picture reflection from yesterday And your hw.
Chapter 22 Section 2 Handout
Energy in the Atmosphere Chapter 16 Section 1 Pages Chapter 16 Section 1 Pages
Heat in the Atmosphere The sun’s energy is transferred to earth and the atmosphere three ways Radiation, Convection and Conduction.
Earth’s Atmosphere Chapter 1.
Climate Change and Human Impact. Many natural processes cause climate change Volcanic eruptions – volcanic ash and dust in the atmosphere reflect solar.
Try this: - Get colored pencils: - Red, Orange,Yellow,Green,Blue,Violet – Use the spectroscope to look at the lights in the room and then out the window.
Human Activities and Climate Change 7.6 p
AIR Vocabulary.
The Greenhouse Effect. Natural heating of earth’s surface caused by greenhouse gases –CO 2 (Carbon Dioxide) –CH 3 (Methane) –N 2 O (Nitrous Oxide) –H.
Greenhouse Effect How we stay warm. The Sun’s energy reaches Earth through Radiation (heat traveling through Space)
3.1 Heat Transfer in the Atmosphere
Sun's Energy & Climate Change climate notes page 3.
Greenhouse Effect How we stay warm.
Greenhouse Effect How we stay warm.
The Greenhouse Effect.
AIM: What is Global Warming?
14.2 – NOTES Solar Radiation
Sun's Energy & Climate Change climate notes page 3.
Solar Energy and the Atmosphere
Energy in the Earth’s Atmosphere
Gases in the Atmosphere absorb Radiation
Atmosphere and Climate Change
climate notes page 3 Sun's Energy & Climate Change
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.
Radiation and Climate.
Greenhouse Effect How we stay warm.
15.3 energy in the atmosphere
Energy in the Earth’s Atmosphere
Presentation transcript:

Air B Radiation and Climate

Solar Radiation The sun (Sol) is a huge fusion reactor - combines two nuclei of H to a He atom. – The produces a tremendous amount of energy – Stars are the “birthplace” of all elements in the universe through the process of fusion.

Solar Radiation Some of the energy from the sun is in the form of electromagnetic radiation - low to high types of energy. All electromagnetic radiation is part of the electromagnetic spectrum

Electromagnetic Spectrum

Electromagnetic Radiation Electromagnetic Radiation is composed of photons – Photons are small bundles of energy – Photons travel as waves - at the speed of light – Photons can travel through a vacuum - they don’t need a medium to travel on (like sound)

Properties of Waves Frequency - how many times a waves passes per amount of time. Wavelength - the distance between two adjacent waves. – Must be the same “part” of the wave. The wavelength and frequency along with the size of the photon determine the type of wave and its energy.

Parts of a wave

The sun and the ER The sun’s radiant energy – 9% of it is UV rays – 46% is visible light – 45% is infrared light

Infrared Radiation Infrared Radiation is the portion of light just below red on the electromagnetic spectrum. – Causes molecules to vibrate this cause friction and the molecules heat up. – Most IR does not reach Earth’s surface. It is absorbed by CO 2. – Some higher level radiation does hit Earth and is absorbed and reradiated back as IR. This lead to the heating of the Earth’s atmosphere.

Visible Light Clear Day = 90% of visible light reaches the earth’s surface. – It is blocked by dust, clouds, pollution etc. It can energize electrons in some biochemicals = photosynthesis. It can excite cells in our eyes causing us to see.

Ultraviolet Radiation Stronger energy than visible light. Three categories of UV radiation: – UV-A: Longest wavelength, lowest energy – UV-B: Shorter wavelength, higher energy - causes cancer. – UV-C: Shortest wavelength, highest energy - used for sterilization – UV-A, UV-B, UV-C are mostly blocked by the ozone layer. – UV-C is absorbed by the atmosphere. – Mostly UV-A gets through to us.

UV radiation If all UV radiation reached the Earth’s surface - the Earth would be destroyed. However, we need some UV radiation - it helps us produce vitamin D when exposed to our skin.

The Carbon Cycle The carbon cycle is the movement of carbon throughout the Earth’s ecosystem. – 100 yrs ago it was predicted that the level of carbon dioxide in the atmosphere due to the increase in burning of fossil fuels would be detrimental – The law of conservation of matter states that the matter can’t be created or destroyed so the amount of carbon would just keep changing forms (physical states)

The Carbon Cycle Atmospheric “reservoirs” of Carbon: – Carbon dioxide in the air – Calcium Carbonate (CaCO3) in limestone – Natural gas (CH4) – Petroleum

The Carbon Cycle

71% of Carbon is in the form of CO 2 in ocean. 22% is in the form of fossil fuels The rest is in the rocks.

The Carbon Cycle - Burning Fossil Fuels Coal: C + O 2  CO 2 Natural Gas: CH 4 +2O 2  CO 2 +2H 2 O Gasoline: 2C 8 H O 2  16CO 2 +18H 2 O

Greenhouse gases and global change The greenhouse effect is a natural and necessary phenomenon. Carbon dioxide and water vapor are the two principle greenhouse gases. – These gases have been constant for millions of years…….until human came along.

Global warming There are 12 trillion tons of water vapor in the atmosphere. Human activity can effect the temp. of atmosphere. – This causes more water vapor to evaporate. – More water vapor (greenhouse gas) means more warming. – More warming means more evaporating. – More evaporating mean more warming etc. – However, increase water vapor increases cloud cover so the temperature increase is not as dramatic.

Global Warming Carbon dioxide is similar. – If too much CO2 is added to atmosphere then stored CO2 in ice and soil could be released and the warm up continues. Two other greenhouse gases: N2O and CH4 (methane).

Global Warming The last ten years have been the warmest to date. If nothing done, temp. will inc..3  C per year. By 2100 temp will inc. by 1  C per year.

Global Warming Most scientists agree that the Earth will increase in temperature by 3-5  C over the next century. However, new data shows that the lower atmosphere is not warming as fast as the Earth’s surface. So there must be other factors affecting the warming. – El Nino – La Nina

Effects of Global Warming. The oceans (melting polar ice caps) will rise 5 cm (about 2 in.) per decade over the next century. – Flooding in several major cities: brings disease, pestilence, wastewater. – Rain cycle and growing season would be affected – Possibility of big storms with long droughts in between. – Short winters with severe blizzards.

Preventing Global Warming Kyoto Protocol – Developing energy efficient technologies – Focus on renewable energies.