Phy100: Heat transport Three basic forms of thermal heat transport

Slides:



Advertisements
Similar presentations
Astronomy Notes to Accompany the Text Astronomy Today, Chaisson, McMillan Jim Mims.
Advertisements

Light and Atoms Chapter 3.
WELCOME! Our Sun is the major source of energy for our planet. Consider all you know about the Sun and it’s energy and answer these questions: 1. What.
4-1 Radiant Energy. Waves  Light travels in Waves similar to ocean waves  Light waves are electromagnetic and consist of an electric and magnetic fields.
Radiant Energy Electromagnetic wave, crest, trough, medium,
ENTRY TASK Get your notebooks Pencil Highlighter.
Light Solar System Astronomy Chapter 4. Light & Matter Light tells us about matter Almost all the information we receive from space is in the form of.
Phy100: Blackbody radiation
Phy100: Heat transport Three basic forms of thermal heat transport
Blackbody radiation Goals: Understand properties of Black body radiation; Black body radiation Radiation power, intensity and angle dependence.
MET 60: Chapter: 4 (W&H) and 2 (Stull) Radiative Transfer Dr. Craig Clements San José State University.
1 NATS 101 Lecture 5 Radiation. 2 Review Items Heat Transfer Latent Heat.
Energy in Earth’s Atmosphere
Energy and Waves.
Chapter 3 Light and Matter
Chapter 3 Radiation. Units of Chapter Information from the Skies 3.2 Waves in What? The Wave Nature of Radiation 3.3 The Electromagnetic Spectrum.
What you will learn: You will determine how waves transfer energy You will describe wave reflection and discuss its practical significance.
Introduction to Optics. 1. The Great Debate 2. What is light? 3. Properties of light 4. The wave-like model 5. Theories of colour.
Energy the ability to cause change Mechanical Energy Energy of motion AND position (sum of the potential and kinetic energy of an object)
Climate Long time, Large Area. Weather short term, small area.
Heat Transfer. Heat is the transfer of thermal energy between substances that are at different temperatures.
Radiation Fundamental Concepts EGR 4345 Heat Transfer.
CHAPTER 12 RADIATION HEAT TRANSFER. Electromagnetic Radiation – electromagnetic waves (brought upon by accelerated charges or changing electric currents)
II. Global Energy Balance. A. Electromagnetic Radiation: self-propagating electric and magnetic waves. Or …. Radiation transmitted through the vacuum.
Earth’s Energy Budget Ch ways heat can be transferred: Conduction Conduction Convection Convection Radiation Radiation.
Question 1 1) wavelength 2) frequency 3) period 4) amplitude 5) energy
Electromagnetic Waves
Chapter 3 Radiation. Units of Chapter Information from the Skies 3.2 Waves in What? The Wave Nature of Radiation 3.3 The Electromagnetic Spectrum.
5.1 Electromagnetic Radiation. Wave motion The transfer of energy without matter is called wave motion Two Types.
Waves and Properties of Light
Light is a Particle Physics 12.
S OLAR R ADIATION. R ADIATION Sun is a sphere of hot gaseous matter with a diameter of 1.39*10^9m. Due to its temperature, sun emits energy in the form.
The Cycling of Energy Chapter 3-3 Study Guide. What is heat flow?  The transfer of energy from a warmer object to a cooler object.
The Nature of Light  Light is the only form of energy that can travel like a wave through empty space and some materials.  It behaves like a special.
Lecture 2: Heat and radiation in the atmosphere. TEMPERATURE… is a measure of the internal heat energy of a substance. The molecules that make up all.
Topic 5 Energy. Energy is the ability to do work or cause change Kinetic energy: energy of motion  faster objects have more kinetic energy Temperature.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 3.
Wave Basics. Wave Definition  Any traveling disturbance that transfers energy. WAVES DON’T MOVE MATTER!!!
Radiation in Astronomy Electromagnetic Radiation I. Electromagnetic Radiation (EM) (EM) Energy travels through space as EM. $ Electromagnetic electric.
Radiation, Conduction, Convection
Radiation in Astronomy
Waves Unit 8.
Electromagnetic Radiation
Chapter 3: Electromagnetic Waves and Light
Introduction to Waves Essential Question:
Section 1 Characteristics of Light
NATS 101 Updates Add your name to Class ListServe!
What is light?.
25.1 The Electromagnetic Spectrum
25.1 The Electromagnetic Spectrum
Photons and Energy A photon is a bundle of energy.
Solar Radiation and the Atmosphere
NATS 101 Lecture 5 Radiation
Energy in Earth’s Atmosphere
17.2 Heating the Atmosphere.
Doppler Effect & Electromagnetism
The Electromagnetic Spectrum
The Electromagnetic Spectrum
Chapter 3-1 Notes: The Electromagnetic Spectrum
FLAME TEST.
Radiation, Spectroscopy, and Telescopes
Vocab #7 Mr. Addeo.
NATS 101 Updates Add your name to Class ListServe!
5.2 Properties of Light Our goals for learning What is light?
Light as a Wave: Part 1 SNC2D.
Light and Quantized Energy
NATS 101 Updates Add your name to Class ListServe! First QUIZ on today
Chapter 2 Energy in transit
Wave Properties.
Solar Radiation and the Atmosphere
Presentation transcript:

Phy100: Heat transport Three basic forms of thermal heat transport 1) Conduction; Convection; Radiation.

Convection Convection is heat transfer by motions of materials in a substance. Usually this occurs in a fluid (air or water) when fluids are moving from heat sources and carrying energy with it.

Radiation Heat can also be transferred by radiating light (i.e. photons) or electromagnetic waves with different wavelengths. In empty space, collisions or mass motions are impossible and there are no conduction or convection and therefore radiation is the only mean to transfer heat. The heat is transferred from the sun to the earth mostly by visible light.

Radiation power spectrum For a hot object with temperature T, Q1: what kinds of photons are emitted (visible or invisible) ? Q2: How much energy emitted per second, i.e. radiation power? About electromagnetic waves: Radiation as a self-propagating electric and magnetic (EM) wave. 2) Any form of radiation or EM waves moves at the speed of light c=3 X 10^8 m/s or 300,000km/s (Boeing Jet cruise speed about 0.3km/s) 3) In electromagnetic waves, both electric fields and magnetic fields Oscillate as a function of time and spatial coordinates. These waves consist are crests and troughs. The distance between two adjacent crests = wavelength. The number of crests one observes at a given point in one second =Frequency wavelength X frequency = speed of light

Full range of forms of radiation

Blackbody radiation Radiation power in a given wave length interval delta-lamba at wavelength lambda

Blackbody radiation at T=3000K-6000K

Blackbody radiation at T=310K

Blackbody radiation at T=3K

Conclusions Wien’s displacement law Radiation power concentrated in an interval of wavelength. The peak position in the power spectrum move to longer wavelengths when T decreases; 2) The integrated radiation power (the area below the power spectrum) decreases as T decreaes. Wien’s displacement law