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    JOHN PHILIP CHANREPORTER 

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    Atmosphere

    “How do I livewithout you?”

    Without the atmosphere, livingorganisms would not be able to

    live.

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  • 8/16/2019 Report Atmosphere

    5/33“o !rote"tion”

    With o AtmosphereWith Atmosphere

    Example:

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    Atmosphere

    Example:

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    Cmp!e!"s:

    Air

    #$one

    Water %apor

    &ust !arti"les

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    A"msp#ere#ne ma'or reason why life is possible

    Earth.#ther planet have also atmosphere but di(erent in"omposition.

     )upiter

    *ethane

    Helium

    %enus

    *er"ury

    %E+,%E+ -HI

    A-*#!HE+E

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    Cmpsi"i! $ Air

    /0.10 22

    31.40 2#2

    1.45 2Ar

    1.15 26#2

    1.1170 2e

    1.1118 2He 1.1178 26H4

    1.1179 2:r 1.11118 2H2

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    %a"er &apr

    -he sour"e of all

    6louds !re"ipitation

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    WA-

    E+ 

    6  6;

    E

    traofo

    anhe

    abrel

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    provide the nu"lei on whi"h moistur

    "an "olle"t to form fogs, "louds andpre"ipitation.

    'us" Par"i(les

    Prism E$$e("opti"al phenomena ofhaving varied hues of redand orange during to thepresen"e of the dustparti"les.

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    O)!e La*er*ole"ules that "ontains 5 atoms of

    o

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    A li=uid or solid that is >nely

    dispersed in air and is in a stablestate.

    Aersl

    uspended variable in the atmosphere.

    6louds mog

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    A clear cloudless day-time s+* is

    lue because molecules in the airscatter lue  light from the sun more than

    they scatter red light. When we look

    towards the sun at sunset, we see red and

    orange colors because the lue light hasbeen scattered out and away from the line

    of sight.

    %#* "#e s+* is lue-

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    !roviding appropriate amount of

    gases needed for photosynthesisand respiration

    u!("i!s $ A"msp#ere

    !hotosynthesis +espiration

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    *oderator of temperature

    u!("i!s $ A"msp#ere

    Heat 6old

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    !rote"tion from meteor parti"les

    u!("i!s $ A"msp#ere

    *eteor

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    @ormation of "louds that brings

    u!("i!s $ A"msp#ere

    Weather 6limate

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    ;owest region of the earthBs

    atmosphere, where masses of airare very well mi

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    A thin layer forming the boundary

    between the troposphere andstratosphere.

      Trppause

    - + # ! # ! A E

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    -emperature in"reases as the

    altitude in"rease and where o$onelayer is lo"ated.

      /"ra"sp#ere

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    Air masses are relatively mi

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    ;ayer of the atmosphere that is >rst

    erst heated by the sun.

      T#ermsp#ere

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    +egion of the earthBs atmosphere

    that is >lled with "harged parti"les.

      I!sp#ere

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    -he true upper limit of the earthBs

    atmosphere.

      Exsp#ere

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    La*ers *

    ele("ri(al prper"ies

    eutral Atmosphere;ies below 91 miles

    Ionosphere+egion of the earthBs atmosphere that is >lled with "

    parti"les.*agnetosphere

    *agneti" envelope shelters the earth from ioni$ed blthe solar wind.

    Rei!s $ I!sp#ere

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    Rei!s $ I!sp#ere& +egion

    E

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    La*ers *

    i"s (mpsi"i!

    Homosphere-urbulen"e "auses a "ontinuous mi