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Marine Science 102: Introduction to Weather and Climate

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Marine Science 102: Introduction to Weather and Climate Instructors: Prof. Sharan Majumdar (Section Q) smajumdar_at_rsmas.miami.edu and Prof. Brian Mapes (Section R) – PowerPoint PPT presentation

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Title: Marine Science 102: Introduction to Weather and Climate


1
Marine Science 102 Introduction to Weather and
Climate Instructors Prof. Sharan Majumdar
(Section Q)smajumdar_at_rsmas.miami.eduandProf.
Brian Mapes (Section R)bmapes_at_rsmas.miami.eduTA
Mr David Painemaldpainemal_at_rsmas.miami.eduCou
rse Websiteshttp//metofis.rsmas.miami.edu/msc1
02
2
Weather Map Links
http//www.hpc.ncep.noaa.gov weather
animations http//www.spc.noaa.gov storm
watches and warnings http//www.nhc.noaa.gov -
hurricanes
3
  • What are Weather and Climate?
  • Weather is the condition of the atmosphere at a
    particular moment
  • Precipitation, temperature, wind speed and
    direction, relative humidity, dewpoint, cloud
    cover,
  • METEOROLOGY is the study of the science of
    weather.
  • Climate is the condition of the atmosphere over
    many years
  • Long-term averages of temperature, moisture,
    winds, clouds, precipitation,

4
  • Climate is what you expect, weather is what you
    get! Robert A. Heinlein
  • Ed Lorenz (MIT) The Father of Chaos

5
Syllabus
  • Broken into 3 sections
  • (i) Fundamentals (ii) Weather (iii) Climate
  • Syllabus (subject to change)
  • http//metofis.rsmas.miami.edu/msc102/schedule.ht
    ml

6
Grades
  • Exams (70)
  • 3 exams (Feb 17, Mar 26, Apr 30)
  • Short answers.
  • No Final Exam.
  • Quizzes (30)
  • 6 Pop quizzes at beginning or end of class.
  • Easy.

7
Textbook
OR
8
Rules
  • Arrive on time.
  • Cell phones, Laptops, iPhones etc off.
  • No talking, txting, reading non-class material
  • No copying in quizzes / exams.
  • Deduction in grade for violations.

9
Chapter One Composition and Structure of the
Atmosphere
10
  • Chapter 1 Outline
  • Composition of the Atmosphere
  • Physical Properties
  • Composition
  • Evolution of the Atmosphere
  • Important Trace Gases
  • Water vapor (H2O)
  • Carbon Dioxide (CO2)
  • Ozone (O3)
  • Others Aerosols, Methane,
  • Vertical Structure of the Atmosphere
  • Pressure and Density
  • Other Planetary Atmospheres

11
Making an Atmosphere Gases and Gravity
12
  • Physical Properties
  • A mixture of gas molecules and very small
    particles of solid and liquid.
  • Behaves as a fluid!
  • The majority of atmospheric mass is contained in
    a rather thin layer near the surface (99.9 is
    below 50 km).
  • Compared with the radius of the Earth (6500 km),
    the atmosphere is very thin (50 km or 1).
  • Atmospheric motions (winds) are largely
    horizontal rather than vertical.

13
Composition of the Atmosphere
78 Nitrogen
20 Oxygen
Remaining 2 trace gases (argon, carbon dioxide,
water vapor, methane, ozone, chlorofluorocarbons,
aerosols)
14
Permanent vs. Variable Gases
Methane CH4
15
(No Transcript)
16
Evolution of the Atmosphere
  • Solar System Formed (6 billion years ago)
  • Planets form from left over dust/gas
  • Earth Formed (4.5 billion years ago)
  • Initially hot atmosphere consisting mainly of
    hydrogen, helium
  • Lightest gases (H, He) escaped gravity into space
  • Secondary Atmosphere from Volcanic Emissions
  • Water vapor (85), Carbon dioxide (CO2 10) and
    Nitrogen (lt5)
  • Nitrogen is chemically stable no reactions with
    gases or Earth
  • Oceans Form
  • Water vapor condensed and formed clouds as Earth
    cooled
  • Precipitation formed oceans (and rivers, lakes
    and glaciers)
  • CO2 dissolved in the ocean Nitrogen built up in
    atmosphere.
  • Oxygen
  • Produced by green-blue algae that evolved in the
    ocean
  • Photosynthesis absorbs CO2, releases oxygen

17
Evolution of the Atmosphere
3 BY old fossil
18
Important Trace Gases
  • Carbon Dioxide (CO2)
  • Water Vapor (H2O)
  • Ozone (O3)
  • Methane (CH4)
  • Aerosols (solid particles, not a gas)

19
Trace Gases Carbon Dioxide (CO2)
  • Carbon Dioxide
  • A trace gas accounting for only 0.036 of total
    atmospheric mass
  • Important to Earths greenhouse effect
  • Greenhouse effect gases absorb radiation emitted
    by Earth warming
  • Naturally occurring.
  • Added through respiration (breathing), volcanic
    activity, organic decay, diffusion from ocean and
    natural and human-related combustion
  • Removed through photosynthesis, diffusion into
    ocean, weathering of rocks.
  • Human contribution
  • Atmospheric CO2 has increased over the past 200
    years due to burning fossil fuels.
  • Spring maximum/Fall minimum reflects breathing
    of land plants.

20
500,000 Year Record of CO2
Current CO2 360 parts per million
21
Carbon Reservoirs (GTC)
Reservoir An area of carbon storage. 1 GTC 1
gigaton 1015 g
750
Input (sources) Removal (sinks)
Decomposition
650
36000
4000?
22
Carbon Fluxes (GTC/yr) Pre-Industrial
Flux The exchange of carbon between reservoirs
750
Input Removal
120
lt1
120
lt1
0
Decomposition
90
90
650
36000
4000?
Atmospheric Residence Time 750 GTC / (90120 GTC
yr-1) 3 yr
23
Atmospheric Residence Time
  • Atmospheric Residence Time The average time a
    molecule of a particular gas resides in the
    atmosphere.
  • Residence Time Amount in Reservoir / Rate of
    Input
  • Carbon Dioxide (CO2)
  • 750 Gigatons / 210 Gigatons per year 3.6
    yr Variable
  • Oxygen (O2)
  • 750000 Gigatons / 400 Gigatons per year 2000
    yr Well mixed
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