Topic 9: Introduction to Remote Sensing Flashcards
(44 cards)
Explain the wave and particle theory of EMR
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Explain the different types of energy-matter interactions
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Explain spectral reflectance curves
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Explain how band selection and assignment in a RGB model produces different colour images
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Remote sensing: definition
the science and art of obtaining information about an object, area, or phenomenon through analysis of data acquired by a device that is not in contact with the object, area, or phenomenon under investigation
How is EMR generated?
- EMR from the sun is generated during thermonuclear fusion
- EMR is absorbed by an atom in the form of potential energy stored in the excited state of electrons
- ## EMR is given off when the electron “looses its excited state”
Wavelength
- Distance between crests (or troughs) of wave form
- measured in micrometers or nanometers
Frequency
- # of crests that pass a point per unit time (one second)
- Usually measured in megahertz or gigahertz
Wave theory
- EM waves are perpendicular to the direction of travel
c = vl
l = wavelength v = frequency c = speed of light (3 x 10^8 m/s)
Wavelength and frequency are inversely proportioned
Particle theory
- EMR is composed of photons
- Energy of a photon is given by:
Q = hv
Q = energy of a photon, Joules (J) h = Planck's constant (6.626 x 10^-34 J.s v = frequency
Black bodies
A theoretical object that completely absorbs all incident radiation, and emits the absorbed energy at the maximum possible rate as given by the Stefan Boltzmann law
object is a perfect radiator
on earth, the closest black body is water
Blackbody Emission Spectra
Peak blackbody emittance given by Wien’s displacement law
- tells the wavelength of maximum radiation given off by a body
hotter the object = shorter the wavelength
colder the object = longer the wavelength
Radiant flux
- Radiant energy per unit time (Joules/ second)
- Watts hitting surface
Irradiance
- Radiant flux that is incident on a surface
- Watts/m^2
Radiant emittance or exitance
- Amount of energy leaving a surface
- Thermal
- Watts/m^2
Radiance
Radiant flux leaving a surface within a given solid angle
RS Instruments and EMR
Remote sensing instruments collect data across specific wavelengths, depending on the instrument’s purpose, platform, and technology
Material interactions
Comes from sun and hits atmosphere
- EMR encounters ozone in stratosphere - aborbs shortwave lengths (UV)
- what is left enters lower level of of atmosphere - troposphere (where all the weather takes place, pollutants, particular matter, water) - some of the radiation scatters off of different things. Depending what is there affects how much scattering there is
- transmitted - some makes it to the ground (some is absorbed, some is reflected, some is scattered
- EMR is also being emitted from the ground
Transmission & refraction
- “Bending” of light
- Occurs when EMR is transmitted through matter
- Index of refraction
1. 0 vacuum
1. 002926 atmosphere
1. 33 water - wavelength dependent
- When EMR passes through the atmosphere it slows down because of that it refracts
- part of the reason it is difficult to get high resolution from space
Atmospheric scattering
- Similar to reflection, but unpredictable
- operates through absorption and re-radiation by atoms or molecules
- when scattering occurs in a volume (as in the atmosphere), we specify three types: Mie, Rayleigh, Non-selective
Rayleigh scattering
- Occurs when the particles are smaller (usually < 0.1 times) the wavelength
- Caused mainly by gases in the upper atmosphere
- eg., why the sky is blue
Mie scattering
- Occurs when particles are approximately the same size as wavelength
- Caused by dust, smoke, particulates in lower atmosphere
- eg., think sunsets - prettier colours when it is dusty
Non-selective scattering
- Occurs with particles many times greater in size than wavelength
- Caused by water droplets, ice crystals in lower atmosphere
- Non-selective with respect to visible wavelengths
Absorption
- Occurs when EMR is absorbed by material and converted into other forms of energy (water vapour, CO2, oxygen, ozone, chlorophyll, minerals)
- Wavelength dependent: those not greatly affected called ‘atmospheric windows’