Micro meter = millionth of a meter Micro meter = m Visible light 0.4 m to 0.7 m.

Slides:



Advertisements
Similar presentations
There are all sorts of electromagnetic waves. The shorter the wavelength the higher the energy of the waves. The energy from the sun is mostly visible.
Advertisements

Venus Earth Mars The surface temperature of Venus is around 460 C (890 degrees F ), the hottest average temperature in the Solar System. This is due.
Chapter 16: Weather Factors
Radiation:.
Light and Atoms Chapter 3.
Announcements Today will be Project 1 presentation first then new material Homework Set 5: Chapter 5 # 44, 46, 47, 50, 52, 53 & 54 Exam 2 is in two weeks.
Structure of Atmosphere From Cunningham & Cunningham, 2004, Fig. 9.1.
Spectral Exitance (Temp. &  )  = 1.0. Earth’s reflective (sun) & emissive (reradiation) regions.
Principles of Radiation. 1. All object possesses (sensible) heat and emit 1. All object possesses (sensible) heat and emit radiation energy as long as.
Radiation Infra-red radiation transfers heat between all objects. Infra-red radiation is an electromagnetic wave and can travel through a vacuum. Heat.
1. 2 Definition 1 – Remote sensing is the acquiring of information about an object or scene without touching it through using electromagnetic energy a.
Solar Ovens Developing a mathematical model for energy transfer.
Thermal radiation Any object that is hot gives off light known as Thermal Radiation.  The hotter an object is, the more light it emits.  As the temperature.
Sayfa 1 Department of Engineering Physics University of Gaziantep June 2014 Topic X BLACKBODY RADIATION EP324 Applied Optics.
Solar Energy On how the Sun emits energy as radiation, and how the Earth receives it.
Many sources (hot, glowing, solid, liquid or high pressure gas) show a continuous spectra across wavebands. Emission spectra Elements in hot gases or.
An improved energy balance model Goals: understand the effects of atmosphere and Greenhouse gases on the earth temperature.
Energy Budget of the Earth- Atmosphere System. Energy Transfer Conduction -- direct molecular transfer Convection -- fluids; air or water –Sensible heat.
Astronomy 1 – Winter 2011 Lecture 7; January
Metr Lab #9 Satellite Imagery. The visible spectrum covers less than half an octave.
Quantum physics. Quantum physics grew out failures of classical physics which found some quantum remedies in the Planck hypothesis and wave-particle duality.
Solar Radiation Emission and Absorption
Radiation Curves. Continuous Radiation How bright is the continuous spectrum at different colors? How does a perfect light source emit its light? 400nm.
Electromagnetic Radiation. Is light a wave or a particle? Yes It’s both, and neither At atomic scales, we have no exact analogs for phenomena For some.
Lecture 5 Abiol 574 Blackbody Radiation/ Planetary Energy Balance This material is from Ch. 3 of The Earth System, ed. 3, by Kump, Kasting, and Crane.
Physics of Planetary Climate Cors221: Physics in Everyday Life Fall 2009 Module 3 Lecture 2: Equilibrium Temperature and The Greenhouse Effect.
Wave property of light Waves can carry energy Wavelength ( ) : distance between successive crests (or troughs) Frequency (f): # of waves passing a point.
Climate Long time, Large Area. Weather short term, small area.
Power Generation from Renewable Energy Sources Fall 2013 Instructor: Xiaodong Chu : Office Tel.:
11/14/2015 Global Warming Archer chapters 1 & 2 GEO 307 Dr. Garver.
Chapter 2 Heating Earth’s Surface and Atmosphere The Atmosphere 10e Lutgens & Tarbuck Power Point by Michael C. LoPresto.
Sun Controls Earth’s Climate System Earth has a global climate system that includes air, land, liquid water, ice, and living things.climate system The.
Topic 6. Without energy from the sun, conditions on Earth would be different. What is the energy that is radiated from the Sun? The energy that is radiated.
Blackbody Radiation Astrophysics Lesson 9.
Wavelength Intensity of emitted e/m radiation 6000K 2000K 1500K 1000K VIBGYOR Wien’s Displacement Law for black body radiation peak wavelength  1 / Temp.
The Greenhouse Effect - Atomic level By Kaelin O’Hare.
Energy Balance. HEAT TRANSFER PROCESSES Conductive heat transfer Convective heat transfer Radiation heat transfer.
Radiation (Ch 12 YAC) Thermal energy is emitted by matter as a result of vibrational and rotational motion of molecules, atoms and electrons. The energy.
Blackbody Radiation/ Planetary Energy Balance
Chapter 16 : Weather Factors Section1 : Energy in the Atmosphere By : Katelyn Angers.
Blackbody. Kirchhoff’s Radiation  Radiated electromagnetic energy is the source of radiated thermal energy. Depends on wavelengthDepends on wavelength.
Energy from the Sun Radiation is the transfer of energy by electromagnetic waves. Ninety-nine percent of the radiation from the Sun consists of visible.
Blackbody Radiation/ Planetary Energy Balance
Blackbody Radiation/ Planetary Energy Balance
Energy Flow Concept Image Sensor Energy Source
Timescales Geological time (big changes globally)
VISHWAKARMA GOVERNMENT ENGINEERING COLLEGE
Radiation.
Black body radiation A blackbody is a perfect absorber of radiation, able to absorb completely radiation of any wavelength that falls on it. A blackbody.
Global Warming Topic 8.5.
Radiation Thermal energy emitted by matter as a result of vibrational and rotational movements of molecules, atoms and electrons. The energy is transported.
Radiation  = 1 for blackbody (emissivity) Qr = T4
Energy from the Sun Sun’s energy travels 148 million km to Earth in only 8 minutes Earth receives less than one-billionth of the Sun’s energy Reaches Earth.
Understand the electromagnetic spectrum and how it is organized.
Blackbody Radiation.
ELECTROMAGNETIC RADIATION
Which parts of Earth are emitting radiation?
NATS 101 Lecture 6 Greenhouse Effect and Earth-Atmo Energy Balance
Energy Budget Subtitle.
17.2 Heating the Atmosphere
Review Items Heat Transfer Latent Heat
Atmospheric Heating Notes
Radiation Thermal energy emitted by matter as a result of vibrational and rotational movements of molecules, atoms and electrons. The energy is transported.
Light.
Understand the electromagnetic spectrum and how it is organized.
Thermodynamics Atmosphere
17.2 – Heating the atmosphere – Part I
ELECTROMAGNETIC RADIATION
Unit 5 Earth’s Energy Budget.
RADIATION LAWS.
Presentation transcript:

Micro meter = millionth of a meter Micro meter = m Visible light 0.4 m to 0.7 m

Radiation Laws As temperature increases wavelength of maximum radiant intensity, max, increases. Weins Displacemnet Law. Sun Earth T=6000 K T=300 K

Radiation Laws As temperature increases wavelength of maximum radiant intensity, max, increases. Weins Displacemnet Law. Sun Earth

Radiation Laws As temperature increases total radiation output increases. Stefan_Boltzman Radiation Law. Brightness = Intensity Energy leaving an object each sec per square meter As T double Brightness increases by ___??____ As T triples Brightness increases by _______

Radiation Laws As temperature increases total radiation output increases. Stefan_Boltzman Radiation Law. Brightness = Intensity Energy leaving an object each sec per square meter As T double Brightness increases by 16 As T triples Brightness increases by _____

Black Body =1.0

The hole acts like a blackbody. All radiant energy is absorbed none is reflected. If the inside of the cavity were to become hot then the hole would glow.

Image modified from: Surface gets energy only from the sun when there is no atmosphere No Atmosphere Solar In IR out

Surface gets solar energy from the sun and infrared energy from the atmosphere when there is an atmosphere. Image modified from: With an Atmosphere