120729 Atmosphere Research

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    Ultraviolet (UV) light is electromagnetic radiation with a wavelength shorter than that o visible light, but longer than X-rays, that is, in the range 10 nm to 400 nm, corresponding to photon energies

    rom 3 eV to 124 eV. It is so-named because the spectrum consists o electromagnetic waves with requencies higher than those that humans identiy as the colour violet. Tese requencies are invisibleto humans, but visible to a number o insects and birds. Tey are also indirectly visible, by causing uorescent materials to glow with visible light.

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    AtmosphereNan Wu Owen Xing Pei Wang

    What is Ozone?

    Also called trioxygen

    Less stable than dioxygen

    Toxic in large doses

    Formed by diatomic oxygen reacting with UV photons

    Destroyed by reacting again with dioxygen

    Ozone & UV

    The Ozone Layer

    Ozone is naturally present in our atmosphere

    Around 10% in the troposphere

    The remainng 90% in the stratosphere

    Between 10 km and 50 km off the surface

    This is the ozone layer

    Relative low aboudance of zone in the stratosphere

    Uneven abundance around the globe

    What does the Ozone layer do?

    The ozone layer helps block UVB radiation

    It absorbs around 97-99% of this UV radiation

    Also helps moderate day and night temperature swings

    What is the Ozone Hole?

    The area above the Antarctic where ozne is depleted

    Not a total absence of ozone, but a reduction

    First discovered in 1985 by British scientists

    Is at its worst in the spring of the Southern Hemisphere

    What is UV?

    Ultraviolet (UV) light is electromagnetic radiation with a wavelength shorter than that of visible light, but longer than X-

    rays

    UV light is found in sunlight and is emitted by electric arcs and specialized lights such as black lights

    Most ultraviolet is classied as non-ionizing radiation

    Sources of UV

    Natural sources and lters of UV

    Articial sources of UV

    Black lights"

    Ultraviolet uoarescent lamps

    Gas-discharge lamps

    Ultraviolet LEDs

    Ultraviolet lasers

    Human health-related effects of UV radiation

    Harmful effects

    Skin cancer Eye damage such as cataracts

    Immune system damage

    Damage to the DNA in various life-forms

    Possibly other things too that we don't know about at the moment

    Benecial effects

    UVB exposure induces the production of vitamin D in the skin

    Medical applications

    Applications of UV

    Sanitary compliance

    Biological surveys and pest control

    Air purication

    Analyzing minerals

    Chemical markers Checking electrical insulation

    Ozone diagram

    Ozone hole

    Bug Zapper

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    AtmosphereNan Wu Owen Xing Pei Wang

    Ozone & UV_ Human health-related effects of UV radiation

    Benecial effects Harmful effects

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    AtmosphereNan Wu Owen Xing Pei Wang

    Ozone & UV_ Applications of UV

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    AtmosphereNan Wu Owen Xing Pei Wang

    The Discovery

    In 1985, using satellites, balloons, and surface stations, a team of researchers had discovered a balding patch of

    ozone in the upper stratosphere, the size of the United States, over Antarctica.

    CFCs and Ozone depletion

    Chlorouorocarbons are created and used in refrigerators and air conditioners. These chlorouorocarbons are not

    harmful to humans and have been a benet to us. Once released into the atmosphere, chlorouorocarbons are

    bombarded and destroyed by ultraviolet rays. In the process chlorine is released to de stroy the ozone molecules

    Responsibility for ozone damage each year

    Effects of UV rays on Aquatic Ecosystems

    Ozone depletion causes increases in UV rayss effects on aquatic ecosystems by:

    1. decreasing the abundance of phytoplankton affects the food stock for shes and the absorption of CO2

    2. decreasing the diversity of aquatic organisms reduces food stock and also destroys several sh and amphib-

    ians.

    Ozone & UV_Ozone Depletion

    Monitoring the Antarctic Ozone Hole

    Ozone Hole Areas over different time: Area[106 km2]

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    AtmosphereNan Wu Owen Xing Pei Wang

    Ozone & UV_Christchurch UV levels

    UV levels over NZ

    The UV Index is a measure of the intensity of UV radiation. The larger the number, the more intense the UV. InNew Zealand, its maximum summer value is generally about 12, but it can exceed 13 in the far North. In winter it

    reaches peak values of 1 or 2. Values of 10 or more should be considered as extreme. At high altitude tropical

    sites (eg Mauna Loa Observatory, Hawaii), the UV Index can exceed 20.

    Increased UV levels

    New Zealands location in the remote southern Pacic and Southern oceans and its low population density mean it

    has an exceptionally clean atmosphere over most of the country. For example, New Zealand has little of the par-

    ticulates and shorter-lived industrial gases that affect heavily industrialised countries in the northern hemisphere.

    Our latitude and clarity of atmosphere mean that high levels of radiation from the sun reach the ground relatively

    unhindered. This results in higher levels of UV radiation at ground level in New Zealand than in other developed

    countries. Ozone depletion further exacerbates this effect, resulting in increased intensity of the UV radiation that

    causes sunburn.

    The environmental and health impacts of raised levels of UV can be severe, particularly for New Zealand where

    high levels of UV are already experienced. The impacts include increases in the rates of skin cancers and eye

    cataracts. Raised levels of UV also suppress human and animal immune systems. Plants can also be affected. For

    example, high UV levels reduce the growth of plankton, a critical building block of the marine food chain. Increasedexposure to UV damages some man-made materials such as paints, plastics and construction materials.

    UV leveld at Christchurch in different time of a year

    Summer

    Winter

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    AtmosphereNan Wu Owen Xing Pei Wang

    Atmosphere and Weather_Precipitation and Cloud types

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    Air qualityis the introduction o chemicals, particulate matter, or biological materials that cause harm or discomort to humans or other living organisms, or cause damage to the natural environment

    or built environment, into the atmosphere.Te atmosphere is a complex dynamic natural gaseous system that is essential to support lie on planet Earth. Stratospheric ozone depletion due to air p ollution has long been recognized as a threat tohuman health as well as to the Earths ecosystems.

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    AtmosphereNan Wu Owen Xing Pei Wang

    Air Quality

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    AtmosphereNan Wu Owen Xing Pei Wang

    Air Quality_Emission Factor

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    AtmosphereNan Wu Owen Xing Pei Wang

    Air Quality_Spreading

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    AtmosphereNan Wu Owen Xing Pei Wang

    Air Quality_Health issue

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    AtmosphereNan Wu Owen Xing Pei Wang

    Air Quality_Solution

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    Global warming is the rise in the average temperature o Earths atmosphere and oceans since the late 19th century, and its projected continuation. Since the early 20th century, Earths mean surace tem-

    perature has increased by about 0.8 C (1.4 F), with about two-thirds o the increase occurring since 1980. Warming o the climate system is unequivocal, and scientists are more than 90% certain thatit is primarily caused by increasing concentrations o greenhouse gases produced by human activities such as deorestation and t he burning o ossil uels.Tese fndings are recognized by the nationalscience academies o all major industrialized nations.

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    AtmosphereNan Wu Owen Xing Pei Wang

    Atomsphere layers_Overview

    40km

    30km

    350km

    The troposphere is the lowest layer of

    Earth's atmosphere. The troposphere

    starts at Earth's surface and goes up

    to a height of 7 to 20 km (4 to 12miles, or 23,000 to 65,000 feet) above

    sea level. Most of the mass (about

    75-80%) of the atmosphere is in the

    troposphere. Almost all weather occurs

    within this layer. Air is warmest at the

    bottom of the troposphere near ground

    level. Higher up it gets colder. Air

    pressure and the density of the air are

    also less at high altitudes. The layer

    above the troposphere is called the

    stratosphere. Nearly all of the water

    vapor and dust particles in the atmo-

    sphere are in the troposphere.

    The stratosphere is a layer of Earth's

    atmosphere. The stratosphere is the

    second layer, as one moves upward

    from Earth's surface, of the atmo-sphere. The stratosphere is above the

    troposphere and below the meso-

    sphere. The top of the stratosphere

    occurs at 50 km (31 miles) altitude.

    The boundary between the strato-

    sphere and the mesosphere above is

    called the stratopause. The altitude of

    the bottom of the stratosphere varies

    with latitude and with the seasons,

    occurring between about 8 and 16 km

    (5 and 10 miles, or 26,000 to 53,000

    feet). The bottom of the stratosphere

    is around 16 km (10 miles or 53,000

    feet) above Earth's surface near the

    equator, around 10 km (6 miles) at

    mid-latitudes, and around 8 km (5

    miles) near the poles.

    The thermosphere is a layer of Earth's

    atmosphere. The thermosphere is

    directly above the mesosphere and

    below the exosphere. It extends fromabout 90 km (56 miles) to between

    500 and 1,000 km (311 to 621 miles)

    above our planet.Temperatures climb

    sharply in the lower thermosphere

    (below 200 to 300 km altitude), then

    level off and hold fairly steady with

    increasing altitude above that height.

    Solar activity strongly influences

    temperature in the thermosphere. The

    thermosphere is typically about 200

    C (360 F) hotter in the daytime than

    at night, and roughly 500 C (900 F)

    hotter when the Sun is very active

    than at other times.

    The thermosphere is a layer of Earth's

    atmosphere. The thermosphere is

    directly above the mesosphere and

    below the exosphere. It extends fromabout 90 km (56 miles) to between

    500 and 1,000 km (311 to 621 miles)

    above our planet.

    Temperatures climb sharply in the

    lower thermosphere (below 200 to 300

    km altitude), then level off and hold

    fairly steady with increasing altitude

    above that height. Solar activity

    strongly influences temperature in the

    thermosphere. The thermosphere is

    typically about 200 C (360 F) hotter

    in the daytime than at night, and

    roughly 500 C (900 F) hotter when

    the Sun is very active than at other

    times.

    Very high up, the Earth's atmosphere

    becomes very thin. The region where

    atoms and molecules escape into

    space is referred to as the exosphere.The exosphere is on top of the thermo-

    sphere.

    100km+

    Troposphere Stratoshpere Mesosphere Thermosphere Exosphere

    Troposphere

    Stratoshpere

    Mesosphere

    Thermosphere

    Exosphere

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    AtmosphereNan Wu Owen Xing Pei Wang

    Atomsphere layers_Composition

    The atmosphere is composed of a shell of gases that surrounds the Earth. This shell is remarkably thin, only

    about several hundred kilometers thick. While this may seem large, it is extremely small when you consider it in

    comparison with the size of the Earth.

    The atmosphere contains many gases, but the 2 most abundant by far are Nitrogen and Oxygen. Together,

    these 2 gases make u p approximately 99% of the air. The chart on right hand side shows this. The chart refersto the "Troposphere", which is the bottom layer of the atmosphere.

    Only easured for ozonesondes; for other sources it is extracted from reanalyses

    B-factors for O3, N2O and H2O as a function of

    changing time period (panels a, c and d respec-

    tively) and for O3 as a function of accumulated

    data sources (panel b). The 80% level in all panels

    in shown for reference.

    (a) Ozone anomalies (left) and meanannual cycle (right) for data extracted from the BDBP, for altitudes between 1 km and 70km and for the latitude zone from 40 N to 50 N. (b) same as (a), for data extracted from R&W. White areas indicate where novalues are available.

    (a) Monthly mean ozone number density ( in DU/km) atthe equator and 25km from the BDBP ( red crosses withlines joining adjacent value). (b) A comparison of themean annual cycles calculaed from the monthly meansplotted in panel(a) where R&W values were excludedwhen BDBP values were not available to avoid anytemporal biasing. (c) The monthly mean ozone anomalytimes series calculated by subtracting the mean annualcycles plotted in panel (b) from the time series plotted in

    panel (a).

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    AtmosphereNan Wu Owen Xing Pei Wang

    Composition Increase of CO2 Decrease of flame Decrease of temperture

    Atmosphere Composition Increase of CO2 Increase of flame Increse of temperture

    Atomsphere layers_Effect of omposition

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    AtmosphereNan Wu Owen Xing Pei Wang

    Some of the greenhouse gases occur in nature like water vapor, carbon dioxide; methane and nitrous oxide, on

    the other side there are exclusively human-made like gases used for aerosols.

    Annual Greenhouse Gas Emissions by Sector

    Levels of several important green-

    house gases have increased byabout 25 percent since large-scale

    industrialization began around 150

    years ago. During the past 20 years,

    about three-quarters of human-made

    carbon dioxide emissions were from

    burning fossil fuels.

    Trends in Atmospheric Concentrations and Anthropogenic Emissions of Carbon Dioxide

    From the trend we can clearly see he rices of CO2, thus it is important to lower the greenhouse gases. Atmosphericconcentrations of greenhouse gases are determined by the balance between sources (emissions of the gas fromhuman activities and natural systems) and sinks (the removal of the gas from the atmosphere by conversion to adifferent chemical compound).

    Positive effectThe greenhouse effect was made to have a positive effect, but human activities have made it a negative one.

    The greenhouse effect was made to keep the Earth's average temperature (14oC or 57oF) the same. The

    atmosphere has small amounts of greenhouse gases to trap heat and warm the Earth. Without this greenhouse

    effect, the Earth's temperature could be as low as -18oC (-0.4oF). So the greenhouse effect assures us we

    won't freeze to death.

    Harmful effectOn the negative side, this Greenhouse effect slowly but steadily increases the temperature of the world! Our

    Earth is getting hotter and hotter every year. Ice in the North is melting and the polar bears and other dwellers of

    the cold are losing their homes quickly. The greenhouse effect WAS supposed to simply keep the Earth at the

    same temperature. But carbon dioxide (CO2) levels and other greenhouse gases are increasing in the ozone

    layer and trap more heat because we have invented the car, burned fossil fuels in factories, burned wood as

    campfires, and cut down the forests. As we continue to release these gases, the Earth will rapidly get hotter.

    The change of global temperature and strength of it can be positive and negative influence. However people are

    more attentive to the negative side. The global warming causing by the greenhouse effect to the nature eco-

    system has causing influences such as unusual temperature, surface of sea level rises, ice-age melt, lake and

    river that late frost and melt early as well as some numbers of plant and animal are decreasing.

    Global warming_Green house effect

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    AtmosphereNan Wu Owen Xing Pei Wang

    Global warming_Science & Impact

    Green house

    gases

    Green house

    effectCO2

    Scince of Global warming Impact of Global warming

    Prediction Warming

    Economic Depressed Worse than

    War

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    AtmosphereNan Wu Owen Xing Pei Wang

    Global warming_Solutions

    Buy local

    food

    Use less

    Home

    Solutions of Global warming - Doing something

    Switch to

    greenpowerLess travel

    Be a

    catalyst

    Have an

    energy audit

    Eat less

    meat

    Plant trees

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    AtmosphereNan Wu Owen Xing Pei Wang

    A carbon sink is a natural or artificial reservoir that accumulates and stores some carbon-containing

    chemical compound for an indefinite period. The process by which carbon sinks remove carbon dioxide

    (CO2) from the atmosphere is known as carbon sequestration. Public awareness of the significance of

    CO2 sinks has grown since passage of the Kyoto Protocol, which promotes their use as a form of

    carbon offset.

    The main natural sinks are:

    Absorption of carbon dioxide by the oceans via physicochemical and biological

    processes

    Photosynthesis by terrestrial plants

    Natural sinks are typically much larger than artificial sinks. The main artificial sinks are:

    Landfills

    Carbon capture and storage proposals

    Carbon sources include:

    Fossil fuels

    Farmland; there are proposals for improvements in farming practices to

    reverse this.

    Diagram illustrating a simplified version of the carbon cycle.

    Part of understanding how the climate is likely to change in future is understanding how some reservoirs

    which are currently absorbing carbon (carbon sinks) might stop absorbing carbon in future.

    As result of harmful effect of carbon dioxide, Carbon sinks are the most effective way for New Zealand-

    ers to extract carbon from the atmosphere. They allow you to have the benefit, use and control of your

    initiative without relying solely on the government to save us.

    Natural ways of eliminates carbon dioxides

    Ocean

    One way to increase the carbon sequestration

    efficiency of the oceans is to add micrometre-sizediron particles in the form of either hematite (iron

    oxide) or melanterite (iron sulfate) to certain regions

    of the ocean. This has the effect of stimulating

    growth of plankton. Iron is an important nutrient for

    phytoplankton, usually made available via upwelling

    along the continental shelves, inflows from rivers and

    streams, as well as deposition of dust suspended in

    the atmosphere. Natural sources of ocean iron have

    been declining in recent decades, contributing to an

    overall decline in ocean productivity. Yet in the

    presence of iron nutrients plankton populations

    quickly grow, or 'bloom', expanding the base of

    biomass productivity throughout the region and

    removing significant quantities of CO2 from the

    atmosphere via photosynthesis.

    Soils & Forest

    Since the 1850s, a large proportion of the world's grasslands

    have been tilled and converted to croplands, allowing the rapid

    oxidation of large quantities of soil organic carbon.

    Methods that significantly enhance carbon sequestration in soil

    include no-till farming, residue mulching, cover cropping, and

    crop rotation, all of which are more widely used in organic

    farming than in conventional farming.[35][36] Because only 5%

    of US farmland currently uses no-till and residue mulching,

    there is a large potential for carbon sequestration.[37] Conver-

    sion to pastureland, particularly with good management of

    grazing, can sequester even more carbon in the soil.

    So in order to reduce carbon dioxide is to growing forests a

    mature tropical forest, at first glance, would seem to be a huge

    sink for carbon dioxide. After all, the rate of photosynthesis is

    huge.

    Global warming_Carbon sink