meteorology gel-1370. grading scheme assignment – 30 points exam – 1 – 30 points exam – 2...
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METEOROLOGY
GEL-1370
Grading Scheme
• Assignment – 30 points
• Exam – 1 – 30 points
• Exam – 2 – 30 points
• Final Exam – 40 points
Lowest one unit of 30 points will be dropped
Turning-in Assignment is a MUST!! – If not, one of the tests will not be counted towards the final course grade
Pop Quizzes as a bonus will be periodically given
Historical Developments - Meteorology
• ‘Meteorology’ comes from the Greek Word ‘Meteoros’ meaning ‘high in the air’
• STUDY OF THE ATMOSPHERE AND ITS PHENOMENA
• Greek Philosopher Aristotle (340 BC) wrote a book on natural philosophy entitled “Meteorologica” – first attempt to explain atmospheric phenomena in a philosophical and speculative manner
• Aristotle’s student, Theophrastus, compiled a book on weather forecasting – ‘Book of Signs”
Historical Developments – contd.
• Meteorological Parameters: Air temperature, pressure, humidity, wind speed and direction
• During 1500s, Italian Physicist and Astronomer, Galileo: Invented a cruse water thermometer
• 1643: Evangelista Torricelli, student of Galileo, invented Hg barometer to measure air pressure
• A few years later, Blaise Pascal and Rene Descartes (French): Atmospheric pressure decreases with increasing altitude
• 1667: Robert Hooks (British): Invented a Plate Anemometer for measuring wind speed
Historical Developments – contd.• 1719: Gabriel Fahrenheit (German), developed a temperature
scale• 1742: Anders Celsius (Swedish), developed centigrade scale• 1780: Horace deSaussure (Swiss), invented hair hygrometer to
measure humidity• 1787: Jacques Charles (French), discovered the relationship
between temperature and volume of air• 1835: Gaspard Coriolis (French) demonstrated the effect that the
earth’s rotation has on atmospheric motion• 1840s: Ideas about winds and storms were partially understood• 1843: Invention of Telegraph• 1869: Isobars (lines of equal pressure) were placed on weather
maps• Ca. 1920: Concepts of air masses and weather fronts were
formulated in Norway.
Historical Developments – contd.
• 1940s: Upper-air balloon observations of T, P, Humidity yielded 3-D view of the atmosphere and military aircrafts discovered existence of jet streams
• 1950s: High-speed computers to solve mathematical equations to describe the atmospheric behavior
• 1960: First weather satellite, Tiros I was launched – Space Age Meteorology
• Princeton, NJ (Geophysical Fluid Dynamics Program): Numerical methods to predict weather
• Mid-1990s: Conventional radars were replaced by Doppler radars to peer into severe thunderstorms and unveil their winds
•
Chapter One Chapter One
The Earth’s AtmosphereThe Earth’s Atmosphere
Grading
• Assignment – 30 points
• Exam – 1 – 30 points
• Exam – 2 – 30 points
• Final Exam – 40 points
Lowest one unit of 30 points will be dropped
Turning-in Assignment is a MUST!! – If not, one of the tests will not be counted towards the final course grade
Pop Quizzes as a bonus will be periodically given
Some Basic Questions – Why Meteorology??
• If we approach near a fire place, we feel hotter – if we move to a hill resort (towards the sun) why we feel cooler (not hotter)?
• What is the role of atmosphere in ‘Greenhouse Effect’ and ‘acid rain’
• Why hurricanes is confined to certain regions – lessons from (St.) Andrew?
• Why thunderstorm in the Gulf Coast is much stronger than the Midwest?
• What would happen to this planet if there were no atmosphere??
How Weather Affects our Lives?• Our lives center around the weather – type of clothing we wear,
plants we grow, our comforts in the form of heating/cooling our homes, etc.
• Wind chill makes us feel lot colder than what it is• Health is affected – Arthritis pain is likely to occur when rising
humidity with falling pressure; our mood swings (hot, dry wind vs cool breeze); incidence of heart attacks shows statistical peak after the passage of warm fronts when rain and wind are common
• Cold summer of 1992 – saved billions of $ to people• Bitter cold winter of 1986-1987 in Europe: several hundred
people died• Huge Ice storm in Jan 1998 in Northern New England and
Canada – millions of people without power
How weather affects our lives – contd.
• 1999: Heat waves in US caused 250 deaths• 1995: >500 people died due to high humidity and heat
waves in Illinois• People are killed by Tornadoes• 10 yrs ago, 55 people died due to Andrews in FL (30
billion $ loss)• Fog can affect the visibility• Weather Channel, NOAA Weather Radio Station
CHAPTER – 1
THE EARTH’S ATMOSPHERE*ATMOSPHERE: LIFE-GIVING BLANKET OF AIR
HORIZONTAL LONG-DISTANCE MOVEMENT IS EASY – WE CAN’T DO MORE THAN 8 KM FROM EARTH’S SURFACE - SUFFOCATION
SURVIVING WITHOUT FOOD OR WATER FOR A FEW DAYS POSSIBLE – NOT WITHOUT AIR
IF THERE IS NO ATMOSPHERE, THERE WON’T BE ANY LAKE OR OCEANS
ATMOSPHERE SERVES AS A BUFFER FOR EARTH’S CLIMATE – FROM UNBEARINGLY HOT DURING DAY AND UMIMAGINABLY COLD AT NIGHT
AIR PROTECTS FROM SCORCHING SUN – AIR MOLECULES TRAVEL FROM ONE CONTINENT TO ANOTHER IN LESS THAN A WEEK TIME SCALE
:
Introduction-contd.
• Our planet is driven by the solar energy – a small portion of the outgoing solar radiation is intercepted by the Earth- Sun is at 150 million km away from us (93 million miles)
• Average temp of earth ~15°C (59 °F)
• Temperature fluctuation: -85 °C to 50 °C (-121 °F to 122 °F)
Introduction-contd.• Composition of the Atmosphere (Permanent
Gases)
• Gas Symbol % (volume) dry air– Nitrogen N2 78.08
– Oxygen O2 20.95
– Argon Ar 0.93– Neon Ne 0.0018– Helium He 0.0005
– Hydrogen H2 0.00006
– Xenon Xe 0.000009
Composition of the Atmosphere Near the Earth’s surface-contd.
Gas & particles Symbol % (volume) ppm
Water vapor H2O 0 to 4
Carbon dioxide CO2 0.037 368
Methane CH4 0.00017 1.7
Nitrous Oxide N2O 0.00003 0.3
Ozone O3 0.000004 0.04
Particles (dust, soot, etc) 0.000001 0.01-0.15
Chlorofluorocarbons (CFCs) 0.00000002 0.0002
Atmospheric composition-contd.• 99% of the atmosphere lies within 30 km from surface of
the earth– Atmosphere protects us from
• UV Radiation from Space• Impact of high energy particles from Cosmos• Extreme temperature fluctuations
• Water vapor varies from place to place – up to 4% warm tropical locations to <1% in colder arctic areas
• Condensation (vapor into liquid) and evaporation (liquid becoming vapor)
• Importance of Water vapor in the atmosphere:– Releases large amounts of latent heat (source of atmospheric
energy for thunderstorms and hurricanes)– Water vapor is a ‘greenhouse gas’ (absorbs outgoing energy)
Importance of CO2
• 0.037% • Sources: Burning of fossil fuel, deforestation, volcanic eruption, decay
of vegetation, exhalation of animal life
• Ocean is a huge reservoir – Phytoplankton uptake (source and Sink; Fe expt; atmospheric transport of dust)
• Oceans hold X 50 times the atmospheric CO2
• Before Industrial revolution, CO2 level at 280 ppm and it is now ~370 ppm
(1.5 ppm/yr; ~32% increase) and expected to reach 500 ppm by end of this century [Freight train won’t stop; US consumption of 1/3 vs population of 5%]
• Increase in CO2 will result in global warming – 1 to 3.5°C – Flooding in
certain areas and drought in other regions; global sea level change; global air currents that guide the major storm systems could shift
Measurements of CO2 (ppm) at Mauna Loa Observatory
Other Greenhouse gases
• Methane: Increases by 0.5%/year; Sources include: Paddy fields (breakdown of plant material by certain bacteria), wet oxygen-poor soil, biological activity of termites and biochemical reactions in the stomachs of cow
• Nitrous Oxides: Increases by 0.25%/year; Sources include: release from industrial activity followed by chemical reactions, formation in the soil by microbial activity
• Chloroflurorocarbons (CFCs): Increases with time; Sources include: solvents for cleaning electronic microcircuits; propellants for the blowing of plastic-foam insulation, etc – Play a part in destroying Ozone molecule in the stratosphere - Implications
Ozone (O3)
• The Primary ingradient of photochemical smog (chemical reaction of pollutants in big cities with sunlight)
• ~92% found in stratosphere (11-50 km) – formed when O combines with O2 – abundance < 0.002% by volume
• Shields plants, animals and humans from sun’s harmful UV rays- offers protective shield – CFCs release ozone destroying Cl – Ozone conc. has been decreasing over parts of the Northern and Southern Hemisphere – Ozone hole in Antarctica during September & October
Aerosols
• Smoke from Forest fires, salt particles from sea-water spray, aeolian dust, fine ash particles and gases derived from volcanic eruptions –aerosols– Act as surfaces for nuclei condensation
• Pollutants: Derived from automobiles: CO, hydrocarbons, NO2, sulfur-containing fuels (coal and oil) releases SO2 --- lead to acid rain; NO2 reacts with hydrocarbon in the presence of light to produce ozone
Early Atmosphere• Earth’s first atmosphere is believed to contain mainly H
and He (with traces of NH3 and CH4) – Earth’s hot surface led to the escape of these gases
• Later, escaped gases from volcanic eruptions & steam vents, surrounded the Earth – Mostly water vapor and CO2 formed the second atmosphere --- CO2 reached the ocean and eventually got locked in carbonate rocks --- Slowly but steadily, the N2 content of the atmosphere increased
• Energetic cosmic rays split H2O molecule in O and H – escape of H lead to increase in Oxygen – Plant growth led to the increase in Oxygen levels
Vertical Structure of the Atmosphere• Classification based on: Temperature, composition or
electrical properties• Air Density: number of air molecules/volume• Atmospheric Pressure: Force/area of surface • Total weight of air 5,600 trillion tons• Units of pressure: 1 Atmosphere = 1.01325 bars =
1013.25 millibars (mb) = 101326 Pascal = 1013.25 hectopascal = 29.92 in. Hg = 760 mm Hg = 14.7 lb/inch
Air pressure and density decrease with increasing altitude
Atmospheric pressure rapidly decreases with height
Layers of atmosphere• Earth’s surface to 11 km – temp decreases – sunlight warms the
earth’s surface and the surface warms the air above it
• Lapse Rate (LR) = Rate of decrease of temp. with height; in the lower atmosphere, LR ~ 6.5°C/km; colder air leads to higher LR and warmer air to lower LR; LR fluctuates from day to day & season to season;
• Isothermal Zone: At Tropopause, Stratopause and Mesopause, the Lapse Rate is zero
• Temperature Inversion: Occasional increase of temp. with height known as Temp. Inversion;
• Troposphere: From earth’s surface to where the air stops becoming colder with height; up to 11 km from earth’s surface; controls all the weather; the layer is well mixed by ascending/descending air masses
Temperature-based classification of atmosphere
Atmospheric layers – contd.
• Stratosphere: From the top of tropopause to until the temperature remains constant (~50 km);
• Tropopause height varies – higher in the equatorial region & decreases poleward; tropopause is higher in summer and lower in winter at all latitudes;
• In some regions, tropopause breaks, leading to stratosphere-troposphere air mixing (mainly during spring/summer months and in mid latitudes – Stratosphere-Troposphere Exchange; these breaks also mark the position of jet streams (wind speeds >100 knots)
• At ~20 km from earth, air temperature increases with height – Temperature Inversion – This inversion reduces the vertical movement of air masses within the stratosphere (temp at ~30 km from earth is ~-46°C); this reason
Atmospheric layers – contd.• Inversion in the stratosphere is due to heating of
stratosphere from the absorption of UV rays by O3; absence of O3 ---- air would become colder with height
• Mesosphere: Extremely thin air, low pressure and density; average temp. ~-90°C;
• Thermosphere: Hot layer above Mesosphere; very few atoms and molecules in air; Range of an air molecule ~ 1km (compare with < 10-6 cm in earth’s surface)
• At the top of thermosphere (>500 km from earth’s surface), particles can escape to space – Water Loss Possible?? (this region called Exosphere- upper limit of our atmosphere)
Composition-based Atmospheric Layering
Homosphere: A well-mixed layer in terms of composition; below the thermosphere, the composition of air (78% N2 and 21% O2) remains constant by turbulent mixing
Heterosphere: Complete stirring in the thermosphere is not possible due to few atoms/molecules; diffusion is dominant; heavier atoms at the bottom & lighter atoms at the top – heterogeneity in introduced
Ionosphere: Region within the upper atmosphere where large concentrations of ions and free electrons exist
Layers of atmosphere
Ionosphere
Simplified surface weather map
Weather Map
• Weight of air in the column varies and hence atmospheric pressure
• L: Marks the center of the middle-latitude storm• H: Regions of high atmospheric pressure, anticyclones• Coriolis Force: Earth’s rotation causes the wind to
deflect toward the right in the Northern Hemisphere. This deflection causes the winds to blow clockwise and outward from the center of the highs & counterclockwise and inward toward the center of the low
• Front: A boundary that separates the warm and cool air appears as a heavy, dark line on the map.
Weather Map – contd.
• Weather front is to the west of Chicago – when westerty winds push the front eastward, areas in outskirts of Chicago will observe the approaching front as a line of thunderstorms – heavy showers with thunder and lightning and gusty winds are expected