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Fundamentals of Remote Sensing
Contents
• What is Remote Sensing?
• Process of Remote Sensing
• Electromagnetic Radiations
• Electromagnetic Spectrum
• Interaction with Atmosphere
• Radiations-Target Interactions
• Passive Vs Active Sensing
What is Remote Sensing?
"Remote sensing is the science (and to some extent, art)
of acquiring information about the Earth's surface
without actually being in contact with it.
This is done by sensing and recording reflected or
emitted energy and processing, analyzing, and applying
that information."
Process of Remote Sensing
• 1. Energy Source or Illumination
(A)
• 2. Radiation and the Atmosphere
(B)
• 3. Interaction with the Target (C)
• 4. Recording of Energy by the
Sensor (D)
• 5. Transmission, Reception, and
Processing (E)
• 6. Interpretation and Analysis (F)
• 7. Application (G)
1. Energy Source or Illumination (A) – the first requirement for remote sensing is to
have an energy source which illuminates or provides electromagnetic energy to the
targetof interest.
2. Radiation and the Atmosphere (B) – as the energy travels from its source to the target,
it will come in contact with and interact with the atmosphere it passes through. This
interaction may take place .
3. Interaction with the Target (C) - once the energy makes its way to the target through
the atmosphere, it interacts with the target depending on the properties of both the target
and the radiation.
4. Recording of Energy by the Sensor (D) - after the energy has been scattered by, or
emitted from the target, we require a sensor (remote - not in contact with the target) to
collect and record the electromagnetic radiation.
5. Transmission, Reception, and Processing (E) - the energy recorded by the sensor has to
be transmitted, often in electronic form, to a receiving and processing station where the data
are processed into an image (hardcopy and/or digital).
6. Interpretation and Analysis (F) - the processed image is interpreted, visually and/or
digitally or electronically, to extract information about the target which was illuminated.
7. Application (G) - the final element of the remote sensing process is achieved when we
apply the information we have been able to extract from the imagery about the target in order
to better understand it, reveal some new information, or assist in solving a particular problem.
Electromagnetic Radiation
• All electromagnetic radiation has
fundamental properties and behaves in
predictable ways according to the basics
of wave theory.
• Electromagnetic radiation consists of
an electrical field(E) which varies in
magnitude in a direction perpendicular to
the direction in which the radiation is
traveling, and a magnetic field (M)
oriented at right angles to the electrical
field. Both these fields travel at the speed
of light (c).
Two characteristics of electromagnetic radiation are particularly important for
understanding remote sensing. These are the wavelength and frequency.
The wavelength is the length of one wave cycle, which can be measured as
the distance between successive wave crests. Wavelength is usually represented by the
Greek letterlambda (λ).
Frequency refers to the number of cycles of a wave passing a fixed point per
unit of time. Frequency is normally measured in hertz (Hz).
Wavelength and frequency are related by the following formula:
Therefore, the two are inversely related to each other. The shorter the wavelength, the
higher the frequency. The longer the wavelength, the lower the frequency.
The Electromagnetic Spectrum
• The electromagnetic spectrum ranges from the shorter
wavelengths (including gamma and x-rays) to the longer
wavelengths (including microwaves and broadcast radio waves).
• There are several regions of the electromagnetic spectrum which
are useful for remote sensing.
For most purposes, the ultraviolet or UV portion of the spectrum has the
shortest wavelengths which are practical for remote sensing.
This radiation is just beyond the violet portion of the visible wavelengths,
hence its name.
Some Earth surface materials, primarily rocks and minerals, fluoresce or emit
visible light when illuminated by UV radiation.
Blue, green, and red are the primary colours or wavelengths of the visible
spectrum. They are defined as such because no single primary colour can be
created from the other two, but all other colours can be formed by combining
blue, green, and red in various proportions.
The light which our eyes - our "remote sensors" - can detect is part of the
visible spectrum.
There is a lot of radiation around us which is "invisible" to our eyes, but can be
detected by other remote sensing instruments and used to our advantage.
The visible wavelengths cover a range from approximately 0.4 to 0.7 μm.
The longest visible wavelength is red and the shortest is violet.
Violet: 0.4 - 0.446 μm
Blue: 0.446 - 0.500 μm
Green: 0.500 - 0.578 μm
Yellow: 0.578 - 0.592 μm
Orange: 0.592 - 0.620 μm
Red: 0.620 - 0.7 μm
Interactions with the Atmosphere
• Before radiation used for remote sensing reaches the Earth's surface it
has to travel through some distance of the Earth's atmosphere.
• Particles and gases in the atmosphere can affect the incoming light and
radiation.
• These effects are caused by the mechanisms of scattering and
absorption.
Scattering
• Scattering occurs when particles or
large gas molecules present in the
atmosphere interact with and cause the
electromagnetic radiation to be
redirected from its original path.
• How much scattering takes place
depends on several factors including the
wavelength of the radiation, the
abundance of particles or gases, and the
distance the radiation travels through the
atmosphere.
Absorption
• Absorption is the other main
mechanism at work when
electromagnetic radiation interacts with
the atmosphere.
• In contrast to scattering, this
phenomenon causes molecules in the
atmosphere to absorb energy at various
wavelengths.
• Ozone, carbon dioxide, and water
vapour are the three main atmospheric
constituents which absorb radiation.
Radiation - Target Interactions
• Radiation that is not absorbed or
scattered in the atmosphere can reach
and interact with the Earth's surface.
• There are three (3) forms of interaction
that can take place when energy
strikes, or is incident (I) upon the
surface.
• These are: absorption (A);
transmission (T); and reflection (R).
• The total incident energy will interact
with the surface in one or more of
these three ways. The proportions of
each will depend on the wavelength of
the energy and the material and
condition of the feature.
Absorption (A) occurs when radiation (energy) is absorbed into the
target while transmission (T) occurs when radiation passes through a
target. Reflection (R) occurs when radiation "bounces" off the target and
is redirected. In remote sensing, we are most interested in measuring the
radiation reflected from targets. We refer to two types of reflection,
which represent the two extreme ends of the way in which energy is
reflected from a target: specular reflection and diffuse reflection.
When a surface is smooth we get specular or mirror-like reflection where
all (or almost all) of the energy is directed away from the surface in a
single direction.
Diffuse reflection occurs when the surface is rough and the energy is
reflected almost uniformly in all directions.
Most earth surface features lie somewhere between perfectly specular or
perfectly diffuse reflectors.
Whether a particular target reflects specularly or diffusely, or somewhere in
between, depends on the surface roughness of the feature in comparison to
the wavelength of the incoming radiation. If the wavelengths are much
smaller than the surface variations or the particle sizes that make up the
surface, diffuse reflection will dominate.
Leaves
• Leaves: A chemical compound in leaves
called chlorophyll strongly absorbs
radiation in the red and blue wavelengths
but reflects green wavelengths.
• Leaves appear "greenest“ to us in the
summer, when chlorophyll content is at
its maximum.
• In autumn, there is less chlorophyll in the
leaves, so there is less absorption and
proportionately more reflection of the red
wavelengths, making the leaves appear
red or yellow (yellow is a combination of
red and green wavelengths).
Water
• Longer wavelength visible and near
infrared radiation is absorbed more
by water than shorter visible
wavelengths.
• Thus water typically looks blue or
blue-green due to stronger
reflectance at these shorter
wavelengths, and darker if viewed at
red or near infrared wavelengths.
Passive vs. Active Sensing
• The sun provides a very convenient source of
energy for remote sensing.
• Remote sensing systems which measure energy that
is naturally available are called passive sensors.
• Passive sensors can only be used to detect energy
when the naturally occurring energy is available.
• For all reflected energy, this can only take place
during the time when the sun is illuminating the
Earth.
• There is no reflected energy available from the sun
at night.
• Energy that is naturally emitted (such as thermal
infrared) can be detected day or night, as long as the
amount of energy is large enough to be recorded.
Active sensors
• Active sensors, on the other hand, provide their own
energy source for illumination.
• The sensor emits radiation which is directed toward the
target to be investigated.
• The radiation reflected from that target is detected and
measured by the sensor.
• Advantages for active sensors include the ability to obtain
measurements anytime, regardless of the time of day or
season.
• Active sensors can be used for examining wavelengths
that are not sufficiently provided by the sun, such as
microwaves, or to better control the way a target is
illuminated.
• However, active systems require the generation of a fairly
large amount of energy to adequately illuminate targets.
• Some examples of active sensors are a laser fluorosensor
and a synthetic aperture radar (SAR).
Thanks

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Fundamentals of Remote Sensing

  • 2. Contents • What is Remote Sensing? • Process of Remote Sensing • Electromagnetic Radiations • Electromagnetic Spectrum • Interaction with Atmosphere • Radiations-Target Interactions • Passive Vs Active Sensing
  • 3. What is Remote Sensing? "Remote sensing is the science (and to some extent, art) of acquiring information about the Earth's surface without actually being in contact with it. This is done by sensing and recording reflected or emitted energy and processing, analyzing, and applying that information."
  • 4. Process of Remote Sensing • 1. Energy Source or Illumination (A) • 2. Radiation and the Atmosphere (B) • 3. Interaction with the Target (C) • 4. Recording of Energy by the Sensor (D) • 5. Transmission, Reception, and Processing (E) • 6. Interpretation and Analysis (F) • 7. Application (G)
  • 5. 1. Energy Source or Illumination (A) – the first requirement for remote sensing is to have an energy source which illuminates or provides electromagnetic energy to the targetof interest. 2. Radiation and the Atmosphere (B) – as the energy travels from its source to the target, it will come in contact with and interact with the atmosphere it passes through. This interaction may take place . 3. Interaction with the Target (C) - once the energy makes its way to the target through the atmosphere, it interacts with the target depending on the properties of both the target and the radiation. 4. Recording of Energy by the Sensor (D) - after the energy has been scattered by, or emitted from the target, we require a sensor (remote - not in contact with the target) to collect and record the electromagnetic radiation.
  • 6. 5. Transmission, Reception, and Processing (E) - the energy recorded by the sensor has to be transmitted, often in electronic form, to a receiving and processing station where the data are processed into an image (hardcopy and/or digital). 6. Interpretation and Analysis (F) - the processed image is interpreted, visually and/or digitally or electronically, to extract information about the target which was illuminated. 7. Application (G) - the final element of the remote sensing process is achieved when we apply the information we have been able to extract from the imagery about the target in order to better understand it, reveal some new information, or assist in solving a particular problem.
  • 7. Electromagnetic Radiation • All electromagnetic radiation has fundamental properties and behaves in predictable ways according to the basics of wave theory. • Electromagnetic radiation consists of an electrical field(E) which varies in magnitude in a direction perpendicular to the direction in which the radiation is traveling, and a magnetic field (M) oriented at right angles to the electrical field. Both these fields travel at the speed of light (c).
  • 8. Two characteristics of electromagnetic radiation are particularly important for understanding remote sensing. These are the wavelength and frequency.
  • 9. The wavelength is the length of one wave cycle, which can be measured as the distance between successive wave crests. Wavelength is usually represented by the Greek letterlambda (λ). Frequency refers to the number of cycles of a wave passing a fixed point per unit of time. Frequency is normally measured in hertz (Hz). Wavelength and frequency are related by the following formula: Therefore, the two are inversely related to each other. The shorter the wavelength, the higher the frequency. The longer the wavelength, the lower the frequency.
  • 10. The Electromagnetic Spectrum • The electromagnetic spectrum ranges from the shorter wavelengths (including gamma and x-rays) to the longer wavelengths (including microwaves and broadcast radio waves). • There are several regions of the electromagnetic spectrum which are useful for remote sensing.
  • 11.
  • 12. For most purposes, the ultraviolet or UV portion of the spectrum has the shortest wavelengths which are practical for remote sensing. This radiation is just beyond the violet portion of the visible wavelengths, hence its name. Some Earth surface materials, primarily rocks and minerals, fluoresce or emit visible light when illuminated by UV radiation. Blue, green, and red are the primary colours or wavelengths of the visible spectrum. They are defined as such because no single primary colour can be created from the other two, but all other colours can be formed by combining blue, green, and red in various proportions.
  • 13. The light which our eyes - our "remote sensors" - can detect is part of the visible spectrum. There is a lot of radiation around us which is "invisible" to our eyes, but can be detected by other remote sensing instruments and used to our advantage. The visible wavelengths cover a range from approximately 0.4 to 0.7 μm. The longest visible wavelength is red and the shortest is violet. Violet: 0.4 - 0.446 μm Blue: 0.446 - 0.500 μm Green: 0.500 - 0.578 μm Yellow: 0.578 - 0.592 μm Orange: 0.592 - 0.620 μm Red: 0.620 - 0.7 μm
  • 14. Interactions with the Atmosphere • Before radiation used for remote sensing reaches the Earth's surface it has to travel through some distance of the Earth's atmosphere. • Particles and gases in the atmosphere can affect the incoming light and radiation. • These effects are caused by the mechanisms of scattering and absorption.
  • 15. Scattering • Scattering occurs when particles or large gas molecules present in the atmosphere interact with and cause the electromagnetic radiation to be redirected from its original path. • How much scattering takes place depends on several factors including the wavelength of the radiation, the abundance of particles or gases, and the distance the radiation travels through the atmosphere.
  • 16. Absorption • Absorption is the other main mechanism at work when electromagnetic radiation interacts with the atmosphere. • In contrast to scattering, this phenomenon causes molecules in the atmosphere to absorb energy at various wavelengths. • Ozone, carbon dioxide, and water vapour are the three main atmospheric constituents which absorb radiation.
  • 17. Radiation - Target Interactions • Radiation that is not absorbed or scattered in the atmosphere can reach and interact with the Earth's surface. • There are three (3) forms of interaction that can take place when energy strikes, or is incident (I) upon the surface. • These are: absorption (A); transmission (T); and reflection (R). • The total incident energy will interact with the surface in one or more of these three ways. The proportions of each will depend on the wavelength of the energy and the material and condition of the feature.
  • 18. Absorption (A) occurs when radiation (energy) is absorbed into the target while transmission (T) occurs when radiation passes through a target. Reflection (R) occurs when radiation "bounces" off the target and is redirected. In remote sensing, we are most interested in measuring the radiation reflected from targets. We refer to two types of reflection, which represent the two extreme ends of the way in which energy is reflected from a target: specular reflection and diffuse reflection.
  • 19. When a surface is smooth we get specular or mirror-like reflection where all (or almost all) of the energy is directed away from the surface in a single direction. Diffuse reflection occurs when the surface is rough and the energy is reflected almost uniformly in all directions. Most earth surface features lie somewhere between perfectly specular or perfectly diffuse reflectors. Whether a particular target reflects specularly or diffusely, or somewhere in between, depends on the surface roughness of the feature in comparison to the wavelength of the incoming radiation. If the wavelengths are much smaller than the surface variations or the particle sizes that make up the surface, diffuse reflection will dominate.
  • 20. Leaves • Leaves: A chemical compound in leaves called chlorophyll strongly absorbs radiation in the red and blue wavelengths but reflects green wavelengths. • Leaves appear "greenest“ to us in the summer, when chlorophyll content is at its maximum. • In autumn, there is less chlorophyll in the leaves, so there is less absorption and proportionately more reflection of the red wavelengths, making the leaves appear red or yellow (yellow is a combination of red and green wavelengths).
  • 21. Water • Longer wavelength visible and near infrared radiation is absorbed more by water than shorter visible wavelengths. • Thus water typically looks blue or blue-green due to stronger reflectance at these shorter wavelengths, and darker if viewed at red or near infrared wavelengths.
  • 22. Passive vs. Active Sensing • The sun provides a very convenient source of energy for remote sensing. • Remote sensing systems which measure energy that is naturally available are called passive sensors. • Passive sensors can only be used to detect energy when the naturally occurring energy is available. • For all reflected energy, this can only take place during the time when the sun is illuminating the Earth. • There is no reflected energy available from the sun at night. • Energy that is naturally emitted (such as thermal infrared) can be detected day or night, as long as the amount of energy is large enough to be recorded.
  • 23. Active sensors • Active sensors, on the other hand, provide their own energy source for illumination. • The sensor emits radiation which is directed toward the target to be investigated. • The radiation reflected from that target is detected and measured by the sensor. • Advantages for active sensors include the ability to obtain measurements anytime, regardless of the time of day or season. • Active sensors can be used for examining wavelengths that are not sufficiently provided by the sun, such as microwaves, or to better control the way a target is illuminated. • However, active systems require the generation of a fairly large amount of energy to adequately illuminate targets. • Some examples of active sensors are a laser fluorosensor and a synthetic aperture radar (SAR).