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Title: GE3502GE5502 Geographic and Land Information Systems


1
GE3502/GE5502Geographic and LandInformation
Systems
Lecture 16 Remote sensing II Principles
2
Lecture Plan
  • 1. How does remote sensing work (principles of
    EMR)?
  • 2. Aerial photography
  • 3. Satellite imagery

3
Electromagnetic Radiation
  • To produce a remotely-sensed image, need to
    measure a parameter that can be related to the
    scene.
  • This parameter must be able to reach the sensor
    from some distance away (000s of kms).
  • eg. You can read the whiteboard because visible
    light (from the sun or artificial lights) hits
    the board, and is reflected or scattered into
    your eyes.
  • White reflects much of the light
  • Black reflects little.
  • These signals are transmitted by electromagnetic
    waves.

4
Electromagnetic Radiation
  • Remote sensing devices measure electromagnetic
    radiation (EMR).
  • Spectral resolution determines what is seen by a
    sensor and what features of earth environments
    are recorded.
  • Electromagnetic (EM) energy is one of a number of
    forms of energy. Others - chemical (convection),
    electrical (conduction) and mechanical (contact).
  • EM energy is transferred by radiation and this
    can occur through empty space. Thus an EM energy
    source can be sensed REMOTELY from a distance
    with a SENSOR.
  • The main source of EMR is solar energy (ITR).
    Smaller amounts of EMR are emitted by the earth
    (OTR).

5
EMR (cont.)
  • EM radiation travels through vacuum at (c) speed
    of light ( 300,000 km/s)
  • Waves consist of electric and magnetic fields.
  • Always at right angles to each other
  • Always at right angles to direction of wave
    travel.
  • Wavelength (?) distance between two successive
    peaks (µm).
  • Frequency (f) number of peaks that pass a point
    in a second (Hz).
  • Amplitude maximum value of the fields. A
    measure of the energy.

6
Electromagnetic Radiation (cont.)
  • WAVELENGTH is usually measured in microns (?m)
  • 1 x 10-6 m 0.000001 m
  •  
  • Visible light 0.40 - 0.70 ?m blue green -
    red
  • Different colours in visible light area of
    spectrum have differing wavelengths e.g. orange
    0.55 - 0.62 ?m

7
Electromagnetic Radiation (cont.)
  • FREQUENCY is number of cycles (or wave-crests)
    passing a fixed point within a given period of
    time. It is usually measured in Hertz (Hz) ( no.
    of cycles/second
  • FREQUENCY is inversely related to WAVELENGTH
    thus
  • long wavelength low frequency
  • short wavelength high frequency

8
Electromagnetic Radiation (cont.)
  • Although all EMR travels at the speed of light
    the wavelengths vary.
  • High energy forms of EMR eg. X-rays have short
    wavelength and high frequency
  • Low energy forms like radio waves have long
    wavelength and low frequency.

9
The Electromagnetic Spectrum
  • EMR is usually referred to by wavelength and is
    scaled on an EM spectrum. Solar radiation
    comprises the greatest part of the terrestrial EM
    spectrum used in remote sensing.
  • The spectrum extends from radio and TV
    frequencies, which are low frequency (1012 - 104
    Hz) and 1mm to 1 km in wavelength, to cosmic rays
    (1022Hz ).
  • Such a wide range means frequency and wavelengths
    are plotted on a log scale. 

10
EM MODIFICATION
  • Physical objects modify electromagnetic energy by
    REFLECTANCE (R), TRANSMISSION (T), ABSORPTION
    (A), or EMITTANCE (E).
  • The energy distribution depends on the physical
    (shape, roughness) and chemical structure (what
    it is made of) the object emitting energy.
  • BLACK BODY RADIATION THEORY is used to understand
    how EM energy is distributed across the spectrum
    and how differing kinds of physical materials
    interact with EM energy i.e. the relative amounts
    of EM energy () that are R, T, A or E . This
    understanding is crucial to the recognition of
    terrestrial and aquatic features in remote
    sensing.

11
BLACK BODY RADIATION
  •  A BLACKBODY is a perfect radiator and absorber
    of energy. It is an abstract concept i.e. it does
    not really exist in nature. A blackbody absorbs
    ALL incident radiant energy (and re - emits it at
    longer wavelength as heat). The opposite is a
    whitebody.
  •  
  • A WHITEBODY is a perfect reflector. None of the
    radiant energy is absorbed at all.
  •  
  • Most objects are GREYBODIES - some of the
    incident energy is absorbed some is reflected
    and some is transmitted and emitted - the
    relative balance depends on chemical, electrical
    and physical properties of an object.

12
e.g. Spectral Reflectance Characteristics of
Vegetation
  • Spectral reflectance in vegetation is controlled
    by
  • Cell structure of leaf
  • Surface properties of the leaf and of the
    vegetation canopy grass fronds bush or tree 
  • Vegetation pigmentation
  • - esp. chlorophyll content and Water Content
  • These have marked effect on spectral properties
    of vegetation in visible - NIR spectrum.
  •  

13
Spectral Reflectance Curve for Vegetation
  • Generally vegetation has high IR reflectance -
    bright in TM Band 4 low visible reflectance
    particularly in TM Band 3 (red) and TM Band 1
    (blue).
  •  
  • NIR reflectance can be species dependant, thus
    species of vegetation can be identified from NIR
    BVs.
  • Biomass productivity
  • Crop estimates can be made and
  • Stress detected, i.e. of moisture shortage,
    toxicity, and effect of pollutants affect NIR and
    visible reflectance levels.

14
Vegetation reflectance
15
Plant disease reflectance
16
(No Transcript)
17
Spectral resolution of Landsat TM imagery
  • Band 1 is for bathymetry Bands 2 and 3 are for
    vegetation discrimination bands 2 and 4 are for
    measuring plant vigour bands 5 and 7 are for
    measuring water stress in plants, and for
    discrimination of rock types. All are 30 m
    spatial resolution.
  •  
  • Band 6 is for thermal mapping (120 m). There is
    also a Band 8 on LANDSAT 7 which takes black and
    white (panchromatic) imagery with a pixel size of
    15 m.

Thematic Mapper Bands (?m) 1 0.45 -
0.52 (blue) 2 0.52 - 0.60 (green) 3 0.63 - 0.69
(red) 4 0.76 - 0.90 (NIR) 5 1.55 - 1.75 (MIR) 6
10.4 - 12.5 (TIR) 7 2.08 - 2.35 (MIR)
18
Seeing Heat
Coincident images of the Brazilian rain forest at
.657 µm (red) and 4.05 µm (thermal infra-red),
respectively. The visible light image shows
only smoke, while the thermal infra-red image
shows details of the fire beneath it.
19
Recording EMR
  • Low radiant energy levels (Absorbed) are given
    low BVs and high radiant energy levels are given
    high BVs (Reflected).
  • The BV is usually recorded as a digital number
    (DN a positive integer) for display and
    analysis in a computer.

20
Scanned Data Format
  • Brightness values are recorded in a grid, or
    raster, format. This is a matrix of cells or
    pixels organised into an array of rows (lines)
    and columns (samples).

21
Unprocessed TM image
22
Atmospheric Absorption
Only radiation within certain wavelengths can
pass through the atmosphere to reach the Earth.
Different gases absorb different wavelengths.
Nitrogen Little absorbtion O2 ultraviolet and
at 6.3um CO2 number of wavelengths Water vapour
V important O3 ultraviolet Therefore,
certain wavelengths where most or all EMR gets to
the surface are called atmospheric windows.
23
2. Aerial Photography
  • Aerial photography has long been a primary source
    of base map data for many common products
  • Two major issues
  • The ability to obtain required classifications
    from the photography requires the use of an
    interpretation key
  • Rectification (scale, relief and tilt
    distortions) and lack of reference grid the
    photo must be georeferenced to a coordinate
    system, which requires the use of ground control
    points (GCPs)

24
Distortions on an aerial photograph
25
AP of Townsville at 125000
26
Why choose aerial photography
  • Examine large areas
  • Measure things that are difficult to examine on
    the ground
  • Measure features that are continuous (change
    gradually across space)
  • Examine how a place changes over time
  • Finer resolution than satellite imagery (usually)
  • You can control when and where images are taken,
    i.e. you are not limited to the position of a
    satellite in orbit
  • You can coordinate a ground survey to take place
    at the same time

27
Things to consider
  • Can be expensive to get all the photos you need
  • Can require lots of room to store and use on your
    computer
  • Requires processing before you can use in GIS
    can be time consuming
  • Includes distortions due to the camera lens, and
    the angle and height of the aircraft

28
Sources of aerial photography
  • Geoscience Australia
  • GBRMPA Great Barrier Reef Marine Park Authority
  • AIMS Australian Institute of Marine Science
  • TESAG Cartography (Adella Edwards)
  • Private companies

29
3. Satellite Imagery
30
Why use satellite imagery?
  • Examine large areas of the Earth at once
  • Measure things that are dangerous and difficult
    to examine from the ground
  • Measure features that are continuous (change
    gradually across space)
  • Examine how a place changes over time

31
Active vs. Passive Sensors
32
Things to consider
  • Cost satellite imagery can be very expensive
  • Can require lots of room to store and use on your
    computer
  • Requires processing before you can use it in a
    GIS this can be very time consuming
  • Spatial and temporal resolution will be limited
    to availability of satellites

33
Where to get satellite imagery from
  • ACRES Australian Centre for Remote Sensing
  • BOM - Australian Bureau of Meteorology
  • NOAA National Oceanographic and Atmospheric
    Association
  • NASA - National Aeronautics and Space
    Administration
  • JCU Dept of Electrical and Computer Engineering
  • TESAG Cartography (Adella Edwards)
  • Note Always check a few different sources when
    chasing data it is often possible to enter data
    share agreements where agencies provide data at a
    greatly reduced cost.

34
Points to remember
  • Remote sensing data are not gathered directly
  • Electromagnetic signals are received as
    surrogates of what is actually on the ground
  • The raw data must be processed by experienced
    interpretation specialist before object
    categories can be properly identified

35
Problems stemming from RS data
  • The quantisation of space into pixels imposes a
    level of abstraction and simplification on the
    Earths features.
  • Objects that are much smaller than the pixels
    cannot be directly identified
  • Satellite remotely sensed raw data provides
    little information until it has been analysed
  • Two major types of data processing
  • Image enhancement
  • Image classification

36
More problems with RS data
  • Different RS data sources may prove to be
    incompatible
  • Problems
  • Categories may not relate well to each other
  • Data may be collected at different scales
  • The above are particularly a problem if RS data
    are being used to update historical maps
  • Changing atmospheric conditions
  • Cloud cover
  • Haze
  • Sensors age may result in sensor drift

37
Getting the data into a GIS
  • Data needs to be in a digital format
  • This is already the case with satellite imagery,
    however aerial photos will need to be scanned
  • The data needs to be in the correct format for
    the particular GIS software you are using
  • Most image processing software has tools to
    export and convert data between different formats
  • If the image is rectified you will need to know
    the coordinate system, projection and datum
  • This is essential for when you are comparing
    different data sets of the same area

38
Summary
  • Remote sensing is useful for gathering
    information over large areas
  • Remotely sensed data needs to be used with
    caution and requires validation by field measures
  • Remote sensing is still a rapidly maturing field
    of investigation with much scope for future
    research
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