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NATS 101 Updates

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Title: PowerPoint Presentation - NATS 101 Updates Author: Emil Kursinski Last modified by: Emil Kursinski Created Date: 8/29/2006 2:04:43 PM Document presentation format – PowerPoint PPT presentation

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Title: NATS 101 Updates


1
NATS 101 Updates
  • Add your name to Class ListServe!
  • First QUIZ on Thursday
  • Review session tomorrow at 5PM
  • Location TBD. Will be announced via Listserve
  • Textbooks
  • Note-takers takees meet after class
  • PBS NOVA Mars Dead or Alive tonight 800
  • 1st anniversary of Katrina this week
  • Quick update on Ernesto

2
4 by 6 Cards
  • Todays assignment
  • Name, SID legible penmanship
  • What worked
  • What didnt and needs clarification

3
Practice Surface Station
  • Sea Level Pressure
  • Leading 10 or 9 is not plotted
  • Examples
  • 1013.8 plotted as 138
  • 998.7 plotted as 987
  • 1036.0 plotted as 360

4
Average and Record MAX and MIN Temperatures for
Date
5
Climate of TucsonProbability of Last Freeze
Cool Site Western Region Climate Center
6
Climate of TucsonProbability of Rain
Cool Site Western Region Climate Center
7
Climate of TucsonExtreme Rainfall
Cool Site Western Region Climate Center
8
Climate of TucsonSnow!
Cool Site Western Region Climate Center
9
Summary
  • Weather - atmospheric conditions at specific time
    and place
  • Weather Maps ? Instantaneous Values
  • Climate - average weather and the range of
    extremes compiled over many years
  • Statistical Quantities ? Expected Values

10
NATS 101
  • Lecture 3Temperature, Heat Transfer
  • and begin
  • Radiation

11
What is Temperature?
  • Microscopic View
  • Energy due to random jiggling of molecules
  • Related to average molecular speed 500 m/s
    (1100 mph) at room temperature for air

12
Temperature and Density
  • Consider volume of air
  • If air is warmed
  • The molecules will move faster, have stronger
    collisions, and tend to become spaced farther
    apart
  • Volume increases, so density decreases
  • Warmer ? less dense

13
Temperature Scales
  • Fahrenheit (oF) - relative
  • US public standard
  • Celsius (oC) - relative
  • Freezing point 0oC
  • Boiling point 100oC
  • oC 5/9 (oF-32)
  • Kelvin (K) - absolute
  • K oC273

Ahrens p27
14
What is Heat?
  • Heat-Energy in the process of being transferred
    from a warmer object to a cooler object
  • Consider a pot of water on a hot burner.
  • Consider the following questions

Williams, p. 19
15
Heat Transfer Questions
  • What causes the
  • Pan bottom and handle to get warmer?
  • Top of the water to become warmer?
  • Water temperature to not exceed 100oC?
  • Region away from side of pan to feel warm?

Williams, p. 19
16
Conduction
  • Heat transfer due to collision of molecules.
  • Conduction warms the bottom of the pan!
  • Conductivity - rate of heat transfer across a 1
    cm thick slab of material if one side is kept 1oC
    warmer than the other
  • Cheap Experiment Touch your chair!

17
Heat Conductivity
18
Specific Heat Capacity
  • Heat required to raise temperature of 1 gm of
    substance 1oC.
  • Metal has lower heat capacity than water!

19
Convection
  • Heat transfer due to vertical exchange of mass
  • Occurs in fluids (liquids, gases) because of
    gravity
  • Warm, buoyant air rises - Cool, dense air sinks
  • Convection warms top of liquid!

20
Convection Movies
  • 2D Convection Tank Animation ?
  • 2D Convection Model Ra106
  • 2D Convection Model Ra107 IC1
  • 2D Convection Model Ra107 IC2
  • 3D Rayleigh-Benard Convection Model ?
  • Last hour movie of clouds and moist convection
  • over Catalina mountains

21
Energy States and Water Phases
water molecules are tightly packed in a crystal
alignment that prevents them from changing shape
LOW ENERGY STATE
attractive forces btw molecules weaken and
individual molecules can move around each other,
but they can not break away SLIGHTLY HIGHER
ENERGY STATE
water molecules move very rapidly and are not
bound together EXTEMELY HIGH ENERGY STATE
Large Energy Change
Small Energy Change
22
Latent Heat
Surrounding air cools
Less Ordered Phase
More Ordered Phase
-620 cal/gm
-80 cal/gm
-540 cal/gm
Strong attraction between molecules
Weak attraction between molecules
Some attraction
540 cal/gm
80 cal/gm
620 cal/gm
Surrounding air warms
Ahrens, p 28
23
Latent Heat
  • Energy associated with phase of matter.
  • Must be either added to or taken from a substance
    when it changes its phase.
  • To turn liquid water into solid ice, must remove
    energy from the liquid water.
  • To turn liquid water into vapor, must add a lot
    of energy to the liquid water.

24
Heat Transfer Questions
  • What causes the
  • Pan bottom and handle to get warmer?
  • Top of the water to become warmer?
  • Water temperature to not exceed 100oC?
  • Region away from side of pan to feel warm?

Williams, p. 19
25
Modes of Heat Transfer
Latent Heat
Williams, p. 19
26
Take Home Concepts
  • Heat-Energy transfer due to temperature
    differences
  • Three modes of heat transfer
  • Conduction molecule to molecule
  • Convection transport of fluid
  • Radiation electromagnetic waves
  • Latent Heat energy of phase changes

27
Modes of Heat Transfer
  • Energy is only converted from one form to another
    or transferred from one place to another.
  • Energy is transferred from hot to cold.
  • Conduction - Molecules colliding most efficient
    at interface.
  • Convection - Requires movement of a fluid or gas.

28
Radiation
  • Any object that has a temperature greater than 0
    K, emits radiation.
  • This radiation is in the form of electromagnetic
    waves, produced by the acceleration of electric
    charges.
  • These waves dont need matter in order to
    propagate they move at the speed of light
    (3x105 km/sec) in a vacuum.

29
Electromagnetic Waves
  • Two important aspects of waves are
  • What kind Wavelength or distance between peaks.
  • How much Amplitude or distance between peaks and
    valleys.

Wavelength
Amplitude
Frequency
30
Why Electromagnetic Waves?
  • Radiation has an Electric Field Component and a
    Magnetic Field Component
  • Electric Field is Perpendicular to Magnetic Field

31
Photons
  • NOT TO CONFUSE YOU, but
  • Can also think of radiation as individual packets
    of energy or PHOTONS.
  • In simplistic terms, radiation with
  • shorter wavelengths corresponds to photons with
    more energy and
  • higher wave amplitude to more BBs per second

32
Electromagnetic Spectrum
Wavelengths of Meteorology Significance
Danielson, Fig. 3.18
WAVELENGTH
33
Emitted Spectrum
  • Emitted radiation has many wavelengths.

Prism
(Danielson, Fig. 3.14)
34
Emitted Spectrum
Energy from Sun is spread unevenly over all
wavelengths.
Emission spectrum of Sun
Energy Emitted
Ahrens, Fig. 2.7
Wavelength
35
Wiens Law
Danielson, Fig. 3.19
  • The hotter the object, the shorter the brightest
    wavelength.

36
Wiens Law
  • Relates the wavelength of maximum emission to the
    temperature of mass
  • ?MAX (0.29?104 ?m K) ? T-1
  • Warmer Objects gt Shorter Wavelengths
  • Sun-visible light
  • ?MAX (0.29?104 ?m K)?(5800 K)-1 ? 0.5 ?m
  • Earth-infrared radiation
  • ?MAX (0.29?104 ?m K)?(290 K)-1 ? 10 ?m

37
Wiens Law
  • What is the radiative temperature of an
    incandescent bulb whose wavelength of maximum
    emission is near 1.0 ?m ?
  • Apply Wiens Law
  • ?MAX (0.29?104 ?m K) ? T-1
  • Temperature of glowing tungsten filament
  • T (0.29?104 ?m K)?(?MAX)-1
  • T (0.29?104 ?m K)?(1.0 ?m)-1 ? 2900K

38
Stefan-Boltzmanns (SB) Law
  • The hotter the object, the more radiation
    emitted.
  • When the temperature is doubled, the emitted
    energy increases by a factor of 16!
  • Stefan-Boltzmanns Law
  • E (5.67?10-8 Wm-2K-4 )?T4
  • E2?2?2?216
  • 4 times

Sun Temp 6000K
Earth Temp 300K
Aguado, Fig. 2-7
39
How Much More Energy is Emitted by the Sun per m2
Than the Earth?
  • Apply Stefan-Boltzman Law
  • The Sun Emits 160,000 Times More Energy per m2
    than the Earth,
  • Plus Its Area is Mucho Bigger (by a factor of
    10,000)!

40
Radiative Equilibrium
  • Radiation absorbed by an object increases the
    energy of the object.
  • Increased energy causes temperature to increase
    (warming).
  • Radiation emitted by an object decreases the
    energy of the object.
  • Decreased energy causes temperature to decrease
    (cooling).

41
Radiative Equilibrium (cont.)
  • When the energy absorbed equals energy emitted,
    this is called Radiative Equilibrium.
  • The corresponding temperature is the Radiative
    Equilibrium Temperature.

42
Key Points
  • Radiation is emitted from all objects that have
    temperatures warmer than absolute zero (0 K).
  • Wiens Law wavelength of maximum emission
  • ?MAX (0.29?104 ?m K) ? T-1
  • Stefan-Boltzmann Law total energy emission
  • E (5.67?10-8 W/m2 ) ? T4

43
Key Points
  • Radiative equilibrium and temperature
  • Energy In Energy Out (Eq. Temp.)
  • Three modes of heat transfer due to temperature
    differences.
  • Conduction molecule-to-molecule
  • Convection fluid motion
  • Radiation electromagnetic waves

44
Reading Assignment
  • Ahrens
  • Pages 30-42
  • Problems 2.7, 2.9, 2.10, 2.11, 2.12
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