EM Plane Wave: z Wave propagates along k, magnitude = 2p/l

Slides:



Advertisements
Similar presentations
Introduction to Measurement Quantities Training Level: BASIC
Advertisements

Measurements in Fluid Mechanics 058:180:001 (ME:5180:0001) Time & Location: 2:30P - 3:20P MWF 218 MLH Office Hours: 4:00P – 5:00P MWF 223B-5 HL Instructor:
Section 10 Radiative Transfer
Chapter 33 - Light and Illumination
Light Visible electromagnetic radiation Power spectrum Polarization Photon (quantum effects) Wave (interference, diffraction) From London and Upton.
CPSC 641 Computer Graphics: Radiometry and Illumination Jinxiang Chai Many slides from Pat Haranhan.
Photomultipliers. Measuring Light Radiant Measurement Flux (W) Energy (J) Irradiance (W/m 2 ) Emittance (W/m 2 ) Intensity (W/sr) Radiance (W/sr m 2 )
May Chuck DiMarzio, Northeastern University ECE-1466 Modern Optics Course Notes Part 6 Prof. Charles A. DiMarzio Northeastern University.
OC3522Summer 2001 OC Remote Sensing of the Atmosphere and Ocean - Summer 2001 Review of EMR & Radiative Processes Electromagnetic Radiation - remote.
Radiometry and the Radiometer
The Light Meter An Introduction to Photometry. What is Photometry Photometry focuses on assigning numerical values to light energy emitted from wavelengths.
Light, Color & Perception CMSC 435/634. Light Electromagnetic wave – E & M perpendicular to each other & direction Photon wavelength, frequency f = c/
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Electromagnetic Radiation Physics 202 Professor Lee Carkner Lecture 20.
Electromagnetic Radiation Physics 202 Professor Lee Carkner Lecture 20.
p.1067 Ch 34 Electromagnetic Waves 34.1 Displacement Current and the General Form of Ampere’s Law I d =  0 d  E /dt B·ds =  0 (I + I d ) 
Appearance Models for Graphics COMS , Lecture 2 BRDFs and Radiometry Many slides courtesy Pat Hanrahan:
Electromagnetic Radiation Physics 202 Professor Lee Carkner Lecture 20.
Light Physics 202 Professor Vogel (Professor Carkner’s & CJV notes, ed) Lecture 10.
Electromagnetic Waves Electromagnetic waves are identical to mechanical waves with the exception that they do not require a medium for transmission.
Four equations (integral form) : Gauss’s law Gauss’s law for magnetism Faraday’s law Ampere-Maxwell law + Lorentz force Maxwell’s Equations.
The Electromagnetic Field. Maxwell Equations Constitutive Equations.
Homeaboutpartnersnewsdownloads principlesin depthapplicationsteaching resourceslearning resourcesprinciples REF Physics of light REF Photometry Radiometry.
EP324 Applied Optics Topic X PHOTOMETRY
Four equations (integral form) : Gauss’s law Gauss’s law for magnetism Faraday’s law Ampere-Maxwell law + Lorentz force Maxwell’s Equations.
TRB 2000Photometry for Traffic Engineers1 Photometry for Traffic Engineers... Workshop presented at the annual meeting of the Transportation Research Board.
CS348B Lecture 4Pat Hanrahan, 2005 Light Visible electromagnetic radiation Power spectrum Polarization Photon (quantum effects) Wave (interference, diffraction)
Lecture 21-1 Resonance For given  peak, R, L, and C, the current amplitude I peak will be at the maximum when the impedance Z is at the minimum. Resonance.
Physics 2112 Lecture 23 Electricity & Magnetism Lecture 23, Slide 1.
Physics for Scientists and Engineers, 6e
Optical sensing in Precision Farming (Techniques) Aerial remote sensing Film (visible/NIR/IR) and digitization Direct Digital recording Field machine based.
Optoelectronics Chapter 1 Terminology. EM Spectrum.
Light (simply) A Simple Review for Complex Seniors.
Wave Motion & EM Waves (IV)
Chapter 34 Electromagnetic Waves. Poynting Vector Electromagnetic waves carry energy As they propagate through space, they can transfer that energy to.
Electromagnetic Waves
Solar Energy Types of Generators Irradiance Insolation How Solar Cells work.
Global Illumination CMSC 435/634. Global Illumination Local Illumination – light – surface – eye – Throw everything else into ambient Global Illumination.
Copyright © 2012 Pearson Education Inc. PowerPoint ® Lectures for University Physics, Thirteenth Edition – Hugh D. Young and Roger A. Freedman Lectures.
Photoemissive Light Detectors ISAT 300 Foundations of Instrumentation and Measurement D. J. Lawrence Spring 1999.
Announcement Exam #2 grades are posted on E-learning Exam #2 grades are posted on E-learning Exam #2 average is 6.6 out of 10 (66%) Exam #2 average is.
Chapter 34 (continued) The Laws of Electromagnetism Maxwell’s Equations Displacement Current Electromagnetic Radiation.
Electromagnetic Waves
Classical Optics Prof. D. Rich
Copyright © 2009 Pearson Education, Inc. Energy in EM Waves: The Poynting Vector.
Heinrich Rudolf Hertz 1857 – 1894 The first person generated and received the EM waves 1887 His experiment shows that the EM waves follow the wave.
Computer Graphics III – Radiometry
Describe how electromagnetic energy is transferred through space as electromagnetic waves of varying wavelength and frequency.
Physics 1 H Created by Stephanie Ingle
CMSC 635 Global Illumination.  Local Illumination  light – surface – eye  Throw everything else into ambient  Global Illumination  light – surface.
Jan 2004 Chuck DiMarzio, Northeastern University ECEG287 Optical Detection Course Notes Part 2: Radiometry Profs. Charles A. DiMarzio and Stephen.
Lecture 21-1 Maxwell’s Equations (so far) Gauss’s law Gauss’ law for magnetism Faraday’s lawAmpere’s law *
The EM and Visible Spectra.  Electromagnetic (EM) waves are waves caused by oscillations occurring simultaneously in electric and magnetic fields  A.
Light & Optics. Electromagnetic Waves Electromagnetic waves include: light, radio, microwaves, x-rays, gamma rays, ultra-violet, and infrared radiation.
OPTOMETRY INTRODUCTION Er. FARUK BIN POYEN Dept. of AEIE, UIT, BU, BURDWAN, WB, INDIA
Today’s agenda: Electromagnetic Waves. Energy Carried by Electromagnetic Waves. Momentum and Radiation Pressure of an Electromagnetic Wave.
Physical Principles of Remote Sensing: Electromagnetic Radiation
Electromagnetic Waves
Light, Color & Perception
The Earth is {image} meters from the sun
Section 1 Characteristics of Light
Electromagnetic Waves. Energy Carried by Electromagnetic Waves.
Light Waves and Polarization
Color & Light CMSC 435/634.
Electromagnetic Waves
Maxwell’s Equations (so far)
Warm - Up 1) What is the speed of light?
Light and Illumination
Computer Graphics III – Radiometry
The Properties of Light
Presentation transcript:

EM Plane Wave: z Wave propagates along k, magnitude = 2p/l E and B constant on planar “phase front” k E and B are in phase E B x y

Energy density (J/m3) in an electrostatic field: Energy density (J/m3) in an magnetostatic field: Energy density in an electromagnetic wave is equally divided:

Rate of energy transport: Power (W) John Henry Poynting Rate of energy transport: Power (W) A cDt Power per unit area (W/m2): Pointing Vector Poynting

Poynting Vector oscillates very rapidly! Take the time average: “Irradiance” (W/m2)

EM radiation carries momentum: absorber Radiation pressure

Light is really made up of particles - photons absorber They carry energy: and momentum: “H-bar” is Planck’s constant:

Radiometry: the measurement of EM radiation Radiant Power Fe W Radiant Exitance Me W/m2 Irradiance Ee Radiant Intensity Ie W/sr Radiance (brightness) Le W/sr-m2 Le Me Fe Ee Ie W

Gamma ray X-ray UV Infrared radar radio l (meters) 10-15 10-12 10-9 10-6 10-3 1 103 Visible Light 400 nm 700 nm

Photometry: the measurement of EM radiation as perceived by the eye. equal radiance Luminous efficiency 1 (me) V(l) (you) 400 nm 700 nm (administrator)

Luminous Flux Fv lumen (lm) Luminous Exitance Mv lm/m2 Illuminance Ev lm/m2 or lux (lx) Luminous Intensity Iv lm/sr or candela (cd) Luminance (brightness) Lv cd/m2 or nit (Photometric value) = 685 x V(l) x (radiometric value)