Title: Electromagnetic Radiation EMR
1Electromagnetic Radiation(EMR)
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3Remote Sensing Uses EMR!Soyou need to
understand
- Basic physics of EMR
- Units used to describe EMR
- Divisions of EMR spectrum
- Behavior of EMR interacting with the atmosphere
and other materials
4- All objects warmer than absolute zero emit EMR
- Most objects reflect EMR emitted by other objects
- Key basis of remote sensing because objects of
interest interact in unique ways with EMR
Photo from Flickr by noqontrol
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6How do we describe EMR?
- Wavelength
- Frequency
- Energy
Photo from Flickr lolapaipro
Photo from Flickr by neon360
7Structure of electromagnetic radiation
8Wavelength
9Wavelength Units
- Meters (m)
- Centimeters (cm)
- Millimeters (mm)
- Micrometers (µm)
- Nanometers (nm)
- Angstroms (?)
10Frequency
- The number of waves that pass through an
imaginary plane in a specific amount of time
(e.g., 1 second)
Photo from Flickr by Patrick Treehouse
11Frequency Units
- Hertz (Hz)
- Kilohertz (KHz)
- Megahertz (MHz)
- Gigahertz (GHz)
- Etc.
12Velocity of Light (c)
- c wavelength x frequency (??)
- c 3 x 108 m/sec (the speed of light)
- 186,000 miles/sec
13Energy (Q)
Q h ? Q Energy of a quantum (joules) h
Plancks constant (6.626 10-34 J s) ?
Frequency So Energy is proportional to
frequency Energy is inversely proportional to
wavelength
14Frequency-Wavelength-Energy
Web Demo Electromagnetic Waves
15The EMR Spectrum
16Electromagnetic Spectrum
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18Visible Light
- Wavelengths that dominate radiation given off by
the sun - Most animals evolved to see these wavelengths
- Captured by your digital camera
19Additive Primaries (Color Theory) (Add together
in different proportions to make all other colors)
Red Blue Magenta Red Green Yellow Blue
Green Cyan Red Blue Green White
20Why is Color Theory Important?
- Your computer screen uses the 3 additive
primaries to display all possible colors - To interpret remotely sensed imagery you must be
able to interpret color
Photo from Flickr (by pixel eight)
21Infrared Portion of the Spectrum
22Infrared Radiation
- Near Infrared (NIR) 720 1300 nm
- Mid Infrared (MIR) 1300 3000 nm
- Far Infrared (FIR) 3000 nm
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24Other parts of the Spectrum
UV
Radar
25Atmospheric Effects
- Absorption
- Scattering (will discuss later in the semester)
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27Absorption
- Prevention or strong attenuation of the
transmission of radiant energy through the
atmosphere - Especially important Ozone (O3), Carbon Dioxide
(CO2), Water vapor (H2O)
28Transmission (opposite of aborption)
- Transmittance (t) Transmitted/Incident
- Varies with wavelength
- Atmospheric transmittance varies depending on
atmospheric conditions for each wavelength
29Absorption
Ozone Hole
Thermal IR Greenhouse Effect
30Ozone
- Absorbs strongly in the UV (short wavelengths)
- Protects us from skin cancer!
31Carbon Dioxide
- Absorbs in mid and far infrared
- Greenhouse effect!
32Water Vapor
- Very strong absorber in 5.5-7.0 um range
- Very strong absorber 27 um
- Variable in time and space
33Clouds!
- Most EMR wavelengths cant penetrate clouds
- Big problem in remotely sensed imagerytropics
especially - Temporal compositing to get rid of clouds
- Cloud shadows a problem too
34Riverton Landsat Image July 15 1999 Cloudy!
35Summary
- All of this is important because it determines in
part how objects of interest interact with EMR
which is what we use in remote sensing. The
better we understand these interactions, the
better we are at using the remote sensing tool!