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9.1 Physical Basics

9.2 Recording Techniques 9.3 Image Processing

9.4 Thematic Classification 9.5 Summary

9 Remote Sensing

hBp://saturn.unibe.ch/.../Fotogrammetrie-­‐Bildflug.pdf  

(2)

•   A geographic information system (GIS) is a computer hardware and software system designed to

–  Collect –  Manage –  Analyze –  Display

geographically referenced data (geospatial; spatial)

•  It is a specialized information system consisting of a (spatial) database and a (special) database system

9 Remote Sensing

Visualiza(on,   Cartography  

Spa(al  Data   Management   Collec(on  of  

Spa(al  Data  

Analysis,   Modelling  

Func$onal  Components   Structural  Components  

(3)

•  Recording on site

– Terrestrial survey techniques

•  Global navigation satellite systems (e.g. GPS)

•  Very long baseline interferometer (VLBI)

•  Theodolite: measuring both horizontal and vertical angles optically

•  Total station: electronic theodolite (transit) integrated with an electronic distance meter

– Hydrographic survey

•  Aerial survey and survey by remote sensing

9 Remote Sensing

hBp://i00.i.aliimg.com/  

(4)

•  Remote sensing is the acquisition of information of an object or

phenomenon by the use of device(s)

that are not in

physical or intimate contact with the

object

indirect observation technique

9 Remote Sensing

hBp://www.etsu.edu/cas/geosciences/  

(5)

– That uses the electromagnetic radiation

which is emitted by the observed object

– That carries receiving devices on aircraft or spacecraft

– That serves for the observation of the surface of the earth including all objects thereon, the oceans or the atmosphere

9 Remote Sensing

hBp://www.aero-­‐news.net/  

(6)

•  Photogrammetry

– Greek: photo - grammetry = image-measurement – Acquisition and analysis of images to determine the

properties, form and position of arbitrary objects – Remote sensing is the acquisition of

physical properties of objects whereas photogrammetry is the reconstruction

of their geometric form

based on this data

9 Remote Sensing

hBp://www.gisdevelopment.net/…/mm063d_155.htm   www.maps.google.de    

(7)

•   System characteristics

–  Recording techniques

•  Radiometric resolution

•  Geometric resolution

–  Platform

•  Kind of platform

•  Altitude

•  Orbit

•  Period

–  Mission

•  Temporal coverage

•  Spatial coverage

9 Remote Sensing

hBp://www.wdr.de/tv/quarks/  

hBp://www.dlr.de/  

hBp://www.chip.de/  

hBp://www.mari$me-­‐technik.de/  

(8)

•  Electromagnetic waves as information carrier

– Straight propagation with the speed of light – Speed of light = wavelength x frequency

– Longer wavelength, lesser energy → more difficult to sense

9.1 Physical Basics

electrical  field   distance  

magne$c  field   M  

E  

                                     c  

speed  of  light  

ν:  frequency  

λ:  wavelength  

number  of  cycles  that  passes     a  certain  point  per  second  

hBp://www.fe-­‐lexikon.info/images/  

Elektromagne$scheWelle.jpg  

(9)

•  Electromagnetic spectrum

– The electromagnetic

spectrum is the range of all possible frequencies of electromagnetic

radiation

9.1 Physical Basics

hBp://en.wikipedia.org/  

(10)

•  Behavior of electromagnetic waves at interfaces

9.1 Physical Basics

Reflec$on  

Emission   Absorp$on  

Transmission  

ScaBering  

Transmission  +  Reflec$on  +  Absorp$on  =  1  

(11)

9.1 Physical Basics

[AS14]  

solar  radia$on  

sensor  

received  signal  

scaBered  light   atmospheric  absorp$on  

 and  scaBering   sky  radia$on  

reflec$on  at  the  surface   scaBering  at  the  surface  

absorp$on  and  reflec$on     in  the  water  (suspended    

                         par$cles)  

reflection at the ground

water  depth  

(12)

– The albedo (lat. albedo = "whiteness"), reflectivity

•  The extent to which an object diffusely reflects light from the sun

9.1 Physical Basics

(13)

– Albedo depends on wavelength

•  There is a strong difference between visual and infrared albedos of natural materials

9.1 Physical Basics

 [AS14]  

(14)

•  The sun is the most important source of electromagnetic radiation

•  With the exception of objects at absolute zero, all objects emit electromagnetic radiation

– The higher the temperature,

the shorter the wavelength

of maximum emission

9.1 Physical Basics

www.eduspace.esa.int/eduspac  e/.../images/03.jpg  

(15)

•  Blackbody

– Hypothetical source of energy that behaves in an idealized manner

– It absorbs all incident radiation, none is reflected – It emits energy with perfect efficiency

– Its effectiveness as a radiator of energy varies only as temperature varies

9.1 Physical Basics

hBp://mynasadata.larc.nasa.gov/images/BB_illustra$on2.jpg  

(16)

•  Emissivity

– The ratio between the emitance of a given object and that of

blackbody at the same temperature

– Useful measure of the

effectiveness of objects as radiators

– Kirchhoff‘s law: At thermal

equilibrium, the emissivity of a body (or surface) equals its

absorptivity

9.1 Physical Basics

surface   emissivity           (8-­‐14  μm)   blackbody   1  

water,  

depending   on  pollu$on  

0,973-­‐0,979  

water  with  

oil  film   0,96-­‐0,979  

snow   0,99  

grass,  

dense,  short   0,92-­‐0,97   Sands,  

depending   on  water   moisture  

0,88-­‐0,985  

(17)

•  Atmospheric window(s)

– Portion(s) of the electromagnetic spectrum that can be transmitted through the atmosphere

9.1 Physical Basics

hBp://www.geographie.ruhr-­‐uni-­‐bochum.de/agklima/  

(18)

– Ultraviolet 0.01 - 0.4 μm

•  Reflected solar radiation

•  Because of atmospheric absorption it can only be used on aircrafts flying at low altitude

•  Main application: oil contamination detection in water

– Visible light 0.4 - 0.7 μm

•  Reflected solar radiation

•  Atmospheric influences particularly on blue and green light

•  Several applications, e.g. land use mapping

9.1 Physical Basics

hBp://www.samtgemeinde-­‐nord-­‐elm.de/  

(19)

– Near infrared 0.7 - 3 μm

•  Reflected solar radiation

•  Nearly no atmospheric influences

•  Main application: Classification of vegetation, forest health survey (healthy green plants strongly reflect near infrared radiation),

classification of water (expanses of water seem dark as they absorb all)

9.1 Physical Basics

 hBp://www.forestwatch.sr.unh.edu/  

(20)

– Far infrared (thermal energy) 3 - 1000 μm (usually : 8 - 14 μm)

•  Radiation emitted by the earth

•  Nearly no atmospheric influences (but clouds are

impermeable, CO2 as well: greenhouse effect is measurable!)

•  Applicable day and night

•  Measurements beneath the surface to some extent

(pipelines and leaks...)

•  Applications for which the temperature and its change are important, e.g. sea

temperature, thermal properties of stone, tectonics

9.1 Physical Basics

 hBp://www.qualitas1998.net/paul/  

(21)

– Passive microwaves 1 - 300 mm

•  Emitted radiation

•  Nearly no atmospheric influences (capable to measure through clouds)

•  Measurements beneath the surface to some extent

•  Complex signal difficult to interpret

•  Low ground resolution (weak signal)

•  Disadvantageous signal-to-noise ratio noisy images

•  Main applications: Meteorology (temperature profiles of the atmosphere) and oceanography (ice observation)

9.1 Physical Basics

 hBp://nsidc.org/cryosphere/  

(22)

– Active microwaves (radar) 1 - 300 mm

•  Reflected, transmitted microwave radiation

•  Nearly no atmospheric influences (except reaction on water drops)

•  Applicable day and night

•  Measurements beneath the surface to some extent

•  Polarization effects

•  Higher ground resolution as passive microwaves

•  Complex signal

•  Doppler effect allows detection of

moving objects (military applications), sea pollution

9.1 Physical Basics

 hBp://www.weBeronline.de/  

(23)

•  Orbits

– Altitude, orbital period, – Apogee/perigee

•  Greatest/least distance from the earth

– Inclination

•  Angular distance of the orbital plane from the equator

9.1 Physical Basics

v   orbital  speed  

R   Earth‘s  radius=  6  370  km  

g0   gravita$onal  accelera$on   on  the  Earth‘s  surface  =   9,81  m/s2  

r   radius  of  the  satellite   orbit  

www.satellitentracking.de/txt/  04_satellitenbahnen.html  

(24)

– Low Earth Orbit (LEO)

•  Heights between 200 and 600 km

•  Manned space stations: low inclination and heights above 400 km

•  Satellites with biological or material experiments and astronomical satellites

•  Spy satellites 90° inclination , perigee 200-250 km, apogee 600-900km

– Medium Earth Orbits (MEO)

•  All orbits above 1000 km up to 36000 km

•  Navigation satellite systems (GPS, Glonass)

•  Small communication satellites

9.1 Physical Basics

 hBp://www.tobedetermined.org/  

(25)

– Geosynchronous/geostationary Orbit (GSO)

•  Orbit height approximately 35786 km, 0° inclination

•  Period is equal to the Earth's rotational period It

maintains the same position relative to the Earth's surface

•  Television satellites, weather satellites

– Sun Synchronous Orbit (SSO) or Polar Earth Orbit (PEO)

•  Orbit height between 700 and 1000 km, inclination approximately 90°

•  Orbit ascends or descends over any given point of the Earth's surface at the same local mean solar time so the

surface illumination angle will be nearly the same every time

•  Earth observation satellites

9.1 Physical Basics

 hBp://cimss.ssec.wisc.edu/sage/  

(26)

– To scale

representation of the Earth, LEO, and MEO

9.1 Physical Basics

the  Earth   LEO  

MEO  

(27)

•  Passive systems: photography, scanner (optomechanical, optoelectronical)

•  Active systems: radar sensors

9.2 Recording Techniques

reflected  solar    radia$on   thermal    

radia$on   reflected  ar$ficial  

 radia$on  

R   R  

T/R  

passive  systems   ac$ve  systems  

(28)

•   Passive technique

•  VIS and NIR (400-1000 nm)

•   Analog storage medium

•   Common types of films

–  Black and white/panchromatic:

•  Highest geometric resolution

–  Infrared

•  Unusual representation

•  Contrastier

•  Distinction between coniferous and deciduous forests

•  Surfaces of water easier to identify

9.2 Photographic Systems

[AS14]  

(29)

– Color/chromatic:

•  Worse geometric resolution as black and white, better thematic interpretability

– Color infrared films:

•  The blue-sensitive layer is replaced by an emulsion sensitive to a portion of the near infrared region

•  Good thematic interpretability (vegetation)

9.2 Photographic Systems

[AS14]  

(30)

•  Example: Cosmos with KVR 1000 Camera

– Russian spy satellite

– Polar, sun-synchronous – Altitude 200km

– Ground resolution 2m – Black and white film – Durability 45 days – Missions 1981–2000

9.2 Photographic Systems

hBp://www.spo$mage.fr/web/en/186-­‐kvr-­‐1000.php  

(31)

•  Example: digital

aerial orthophotos of Braunschweig

– Central projection – Planimetrically  

corrected

– 30. March 2014

9.2 Photographic Systems

hBps://www.braunschweig.de/  

(32)

•  Disadvantages

– Difficult radiometric calibration – Low spectral bandwidth

– Analog data

•  Advantages

– Relatively cheap – High resolution

– "Spontaneous"

recording of areas

9.2 Photographic Systems

hBp://saturn.unibe.ch/.../Fotogrammetrie-­‐Bildflug.pdf  

(33)

•  Optomechanical scanner

•  A rotating 45 degree scan

mirror continuously scans the Earth beneath the

platform perpendicular to the direction of flight

•   The system collects data one pixel at a time sequentially

•   A scan line (mirror rotation) is equivalent to the image swath

•  The forward motion of the platform used to acquire a scene with sequential scan lines

9.2 Whisk Broom Scanner

hBp://www.mikroelektronik.fraunhofer.de/  

(34)

9.2 Whisk Broom Scanner

scan  direc(on  

aperture  angle  

al(tude  

sensor   plaHorm  

flight  direc(on  

a:  geometric  resolu$on            >  ground  segment   s:  swath  width  

instantaneous  field  of  view    IFOV:  pixel  

hBp://www.uni-­‐potsdam.de/.../febasis/febasis06_04-­‐1206.pdf  

(35)

motor  

rota$ng   mirror  

radia$on  

op$cal  system   telescope  

beam  spliBer   dispersion  prism  

photodetectors   beam  spliBer  

interference  grid  

electronics  

amplifier,  converter  

streamer  

magne$c  tape   HDDT,  CCT  

•  Radiation imaging

–  Mirror rotates around an axis parallel to the flight direction –  The radiation is split into its various wavelengths and focused

onto detectors

–  Stored on magnetic tape (HDDT, CCT), remote data transmission

9.2 Whisk Broom Scanner

hBp://www.uni-­‐potsdam.de/.../febasis/febasis06_04-­‐1206.pdf  

(36)

•  Advantages

–  Precise spectral and radiometric measurements

–  Wide total field of view –  Digital data, remote data

transmission

•  Disadvantages

–  Relatively short dwell-time –  S-bend

–  Panoramic distortion

–  Low SNR limited radiometric resolution

9.2 Whisk Broom Scanner

hBp://landsat.gsfc.nasa.gov/images/archive/c0005.html  

(37)

•  Landsat

– American satellite series

•  Landsat 1: 1972-1978

•  Landsat 2: 1975-1981

•  Landsat 3: 1978-1983

•  Landsat 4: 1982-1993

•  Landsat 5: 1984-2013

•  Landsat 6: 1993 failure

•  Landsat 7: since1999

•  Landsat 8: since 2013

9.2 Whisk Broom Scanner

hBp://de.wikipedia.org/wiki/Landsat  

1-­‐3  

6,  7   4,  5  

(38)

– Orbit

•  Near polar, sun synchronous

•  Altitude: 907-913 km (Landsat 1-3), 705 km (Landsat 4-7 )

•  Inclination: 99.2° (Landsat 1-3),

98.2° (Landsat 4-7)

•  Orbital period:

approximately 100 minutes

→  14 circulations per day

•  Provide complete coverage

of the Earth every 18

(Landsat 1-3) respectively 16

days (Landsat 4-7)

9.2 Whisk Broom Scanner

ground  trace  for  Landsat1-­‐3  for  one  day    [AS14]                    

(39)

LANDSAT  4,5  (1-­‐3)   LANDSAT  4,5   LANDSAT  7   sensor   Mul$spectral  Scanner  

(MSS)   Thema$c  Mapper  (TM)   Enhanced  Thema$c  

Mapper  Plus  (ETM+)   pixel  size   79  x  79  m²   30  x  30  m²   30  x  30  m²  

spectral  

 channels   1  (4)  0,50  -­‐  0,60  µm,   green  

2  (5)  0,60  -­‐  0,70  µm,   red  

3  (6)  0,70  -­‐  0,80  µm,   near  infrared  

4  (7)  0,80  -­‐  1,10  µm,   near  infrared  

1  0,45  -­‐  0,52  µm,  blue-­‐

green  

2    0,52  -­‐  0,60  µm,  green   3    0,63  -­‐  0,69  µm,  red   4    0,76  -­‐  0,90  µm,  near   infrared  

5    1,55  -­‐  1,73  µm,  mid   infrared  

7    2,08  -­‐  2,35  µm  ,  mid   infrared  

1    0,45  -­‐  0,52  µm,  blue-­‐

green    

2      0,52  -­‐  0,60  µm,  green   3      0,63  -­‐  0,69  µm,    red   4      0,76  -­‐  0,90  µm,  near   infrared  

5      1,55  -­‐  1,73  µm,  mid   infrared  

7      2,08  -­‐  2,35  µm  ,  mid   infrared  

thermal  channel   6      10,4  -­‐  12,5  µm    

(120  x  120  m²)   6      10,4  -­‐  12,5  µm     (60  x  60  m²)  

panchroma(c  channel   8      0,52  -­‐  0,90  µm    

(15  x  15  m²)  

9.2 Whisk Broom Scanner

(40)

– Typical combination of channels

9.2 Whisk Broom Scanner

0,5-­‐0,6  μm   0,8-­‐0,9  μm  

false  colour  composite  

0,6-­‐0,7  μm  

true  colour  composite  

hBp://www.uni-­‐potsdam.de/.../febasis/febasis06_04-­‐1206.pdf  

infrared   red  

green  

(41)

9.2 Whisk Broom Scanner

hBp://landsat.gsfc.nasa.gov/images/lg_jpg/f0012_77-­‐89-­‐06.jpg  

(42)

•  Optoelectronical scanner

•  Employs a linear array of solid semi- conductive elements to acquire one entire line of spectral data

simultaneously

•   Scan lines perpendicular to the direction of flight

•   Forward motion of the platform to acquire a sequence of imaged lines to map a scene

•  CCDs (charge coupled device) to serialize parallel analog signals

9.2 Push Broom Scanner

hBp://www.fotos.docoer-­‐dig.de/  

(43)

9.2 Push Broom Scanner

hBp://www.uni-­‐potsdam.de/.../febasis/febasis06_04-­‐1206.pdf  

scan  direc(on  

:  aperture  angle  

al(tude  

sensor   plaHorm  

flight  direc(on  

a:  geometric  resolu$on            >  ground  segment   s:  swath  width  

(44)

focal     distance  

lens  

aperture  angle   sample  mirror  

CCD  sensors  

op$cal     system   radia$on  

•  Radiation imaging

–  Tilted mirror, sometimes fixed sometimes tiltable

–  CCD image sensors in the image plane of the lens: line scan camera

–  Data storage in parallel memory chips, remote data transmission

9.2 Push Broom Scanner

hBp://www.uni-­‐potsdam.de/.../febasis/febasis06_04-­‐1206.pdf  

(45)

•  Spot (Systeme Probatoire d'Oberservation de la Terre) – French satellite series

•  Spot-1: 1986-1990

•  Spot-2: 1990-2009

•  Spot-3: 1993-1997

•  Spot-4: since 1998

•  Spot-5: since 2002

•  Spot 6: since 2012

•  Spot 7: since 2014

– Two identical parallel sensors that can be operated independently

9.2 Push Broom Scanner

hBp://www.uni-­‐potsdam.de/...  

/febasis/febasis06_04-­‐1206.pdf  

hBp://www.fe-­‐lexikon.info/images/Spot5.jpg  

1-­‐3  

4  

5  

(46)

hBp://www.uni-­‐potsdam.de/.../febasis/febasis06_04-­‐1206.pdf  

angled  

 view   nadir-­‐  

looking  

– Pivoting of the sensors can be employed for stereoscopy and also for a higher repeat circle – Sensors are operated from the ground stations

9.2 Push Broom Scanner

hBp://www.terraengine.com/Dgroundsta$on.cfm  

(47)

– Orbit

•  Sun synchronous

•  Altitude: 822 km

•  Inclination 98,7°

•  Orbital period 101,4 min

approximately 14 circulations per day

9.2 Push Broom Scanner

SPOT  1-­‐3   SPOT  4   SPOT  5  

sensor   HRV  (Instrument  Haute  

Résolu$on  Visible)   HRVIR  (High  Resolu$on  

Visible  and  Infrared)   HRG  (High  Resolu-­‐

$on  Geometric)   geometric  

resolu(on  

20  m  (XS),     10  m  (PN)  

20  m  (XS),     10  m  (P)  

10  m  (VIS,  NIR),     2,5/5  m  (PAN),     20  m  (MIR)   radiometric  

resolu(on   0,5-­‐0,9  μm:                                        

3  VIS,  1  NIR   0,5-­‐1,75  μm:                                      

3  VIS,  1  NIR,  1  MIR   0,45-­‐1,75  μm:    

2  VIS,  2  NIR,  1  MIR      

hBp://spot5.cnes.fr/.../35.htm  

(48)

9.2 Push Broom Scanner

hBp://www.uni-­‐potsdam.de/.../febasis/febasis06_04-­‐1206.pdf  

Spot-1 HRV P-Modus

San Diego(USA),

panchromatic, resolution 20 m

Spot-1 HRV XS-Modus

Detroit(USA), false colour composite, resolution 30 m

(49)

Spot-5 HRG XS-Modus: stereo

9.2 Push Broom Scanner

hBp://www.uni-­‐potsdam.de/.../febasis/febasis06_04-­‐1206.pdf  

Dead sea (Jordan), panchromatic, 11/2002 resolution 2,5 m

(50)

•  Radio Detection And Ranging

•  Principle:

– Transmitting radar

pulses (microwaves)

and recording the

reflected radiation

→ active

– The transit time

and the strength

of the reflected

signal is measured

9.2 Radar

[LKC15]  

(51)

•  Nadir:

– The local vertical direction pointing in the direction of the force of gravity at that location

•  Range:

– Line of sight

•  Azimuth:

– Direction of flight

9.2 Radar

hBp://ladamer.org/Feut/studium/fe1/FE1-­‐06-­‐Radar.pdf  

(52)

•  Recording parameters

– Polarization

•  Direction of the electric field which is

perpendicular to the direction of

propagation in the transmitted radar

signal (H = horizontal, V = vertical)

4 possibilities: HH, VV, HV, VH

– Depression angle θd – Pulse length

– Wavelength is divided into 5 bands

9.2 Radar

hBp://ladamer.org/.../FE1-­‐06-­‐Radar.pdf  

     

K-­‐band   X-­‐band   C-­‐band   L-­‐band   P-­‐band   0,7-­‐1  cm   2,4-­‐4,5  cm   4,5-­‐7,5  cm   15-­‐30  cm   77-­‐136  cm  

(53)

B   GR2  

GR1  

R2   R1  

A  

A   β   B  

•  Azimuth resolution AR depends on beam width ( β ) and the ground range distance (GR)

→ Azimuth resolution is better in the near range

9.2 Radar

[LKC15]  

 and   L:  antenna  length  

λ:  wavelength   where  

(54)

•  Ground range resolution (GRR) depends on the pulse length ( τ ) and the depression angle ( θ )

– Distinction between

A and B only possible

if the pulse passed A

completely before

reaching B

→ Better ground range resolution in the far range

9.2 Radar

Pulse  length                      τ  

Front  of  return     wave  from  A  

Front  of  return     wave  from  B  

A   B    τ  

 2  

<  

Rear  of    

           outgoing  wave  

[LKC15]  

(55)

•  In order to improve the resolution

– Ground range

•  Decrease pulse length

– Azimuth

•  Decrease wavelength

•  Increase antenna length

•  The azimuth resolution

is unacceptably coarse

for systems operating at satellite altitudes

9.2 Radar

hBp://ladamer.org/Feut/studium/fe1/FE1-­‐06-­‐Radar.pdf  

(56)

•  Synthetic aperture radar (SAR)

–  Scene is illuminated over an interval of time →   history of reflections –  The further an object

the longer the time it is illuminated

–  As changes in frequency are systematic separate components of the

reflected signal can be assigned to their correct position

9.2 Radar

hBp://ladamer.org/Feut/studium/fe1/FE1-­‐06-­‐Radar.pdf  

(57)

•  Doppler-effect

– Approaching → increase in frequency

– Receding → decrease in frequency

•  Physical antenna as small as possible

•  Azimuth resolution

independent of GR and λ

9.2 Radar

hBp://ladamer.org/Feut/studium/fe1/FE1-­‐06-­‐Radar.pdf  

synthe$c  aperture  

radar  pulse     with  frequency  v2  

frequency  v2  

object  

v1  –  v2  >  0   v3  –  v2  <  0  

(58)

•  Comparison of the resolution between systems with real (a) and synthetic (b) aperture

9.2 Radar

hBp://ladamer.org/Feut/studium/fe1/FE1-­‐06-­‐Radar.pdf  

(59)

•  Interactions between radar signals and materials very complex as it depends on:

– Wavelength

– Incidence angle

– Electrical properties – Moisture

– Surface property

9.2 Radar

hBp://www.meteo.physik.uni-­‐muenchen.de/.../fe_boden_micro.html  

(60)

•  Penetration depths of microwaves

– Increases with decreasing wavelength – Decreases with increasing

conductivity, which is also influenced by moisture

– Is higher for smoother

surfaces

9.2 Radar

vegeta(on  

dry  alluvium  

glacier  

[AS14]  

(61)

•  Problem-oriented quantitative analysis of radar images is difficult as it relies mostly on hardly comprehensible interdependencies

9.2 Radar

C-­‐Band   L-­‐Band   P-­‐Band  

hBp://www.ccrs.nrcan.gc.ca/resource/tutor/gsarcd/pdf/bas_intro_e.pdf  

(62)

•  Sentinel-1

– SAR satellites in the Copernicus program

– Sentinel-1A launched on 3 April 2014, Sentinel-1B on 25 April 2016

– Orbit

•  Sun synchronous

•  693 km altitude

•  98.2° inclination

•  Orbital period 98.5 min

•  Repeat circle 6 days (two satellites)

9.2 Radar

hBp://104.131.251.97/copernicus/  

(63)

– Mass: 2300 kg (including 130 kg fuel)

– Size: 2.8 m long, 2.5 m wide, 4 m high

with 2×10 m-long solar arrays and a 12 m-long radar antenna

– Solar array average power: 5900 W

– Battery capacity: 324 Ah

– Azimuth resolution:

5, 20, 40 m

–  Ground range resolution: 5, 20 m

9.2 Radar

hBp://104.131.251.97/copernicus/  

(64)

•  Image of Ireland (May 2015)

–  Blue: strong changes in bodies of water or

agricultural activities within 12 days

–  Yellow: urban centers –  Green: vegetated fields

and forests –  Red and orange: bare

soil and rocks

9.2 Radar

hBps://directory.eoportal.org/  

(65)

•  Nepal earthquake displacement

– Image shows how and where the land uplifted and sank from the 7.8-

magnitude

earthquake that struck

Nepal on 25 April 2015

9.2 Radar

hBp://www.esa.int/  

(66)

•  Map of Greenland ice sheet velocity

– January–March 2015

– About 1200 radar scenes were used

– Colour scale in meters per day

9.2 Radar

hBp://www.esa.int/  

(67)

•  Light Detection and Ranging

•  Active sensor

•  Laser beams (UV, VIS near IR) to measure

– Distance – Speed

– Chemical composition and concentrations

•  Often imprecisely called "laser-radar"

9.2 LIDAR

(68)

•  Airborne Laserscanning

– The distance between the sensor and the surface to be measured is determined from the runtime of a light pulse

– By deflection of the laser beam and the forward movement of the aircraft a wide strip is scanned

9.2 LIDAR

ellip(cal  scanning   fibre  scanner   swiveling  mirror  

(69)

– Parameters

•  Sampling rate

•  Scan angle

•  Scan frequency

•  Altitude

•  Aircraft speed

– Recorded data

•  Position

•  Orientation of the aircraft

•  Angle of every emitted beam

•  Measured distance

9.2 LIDAR

hBps://www.e-­‐educa$on.psu.edu/geog481/  

(70)

Last  return   (DTM)  

Primary  return   (DOM)  

– One laser beam might be reflected at different heights, e.g. in presence of vegetation:

•  Primary return: originate from the first objects a lidar pulse encounters, often the upper surface of a vegetation canopy

•  Well suited to create a

digital object model (DOM)

9.2 LIDAR

hBp://www.zt-­‐stuBgart.de/.../gis_day2004_guelch.pdf  

(71)

•  Secondary returns: lower

vegetation layers and the ground surface

•  Last return provides data for a digital terrain model (DTM) if the vegetation is not too dense

9.2 LIDAR

hBp://publik.tuwien.ac.at/files/PubDat_166922.pdf  

emiZed  

         pulse   first  echo   last  echo  

$me  

$me  

$me   signal  

strength  

scrup   terrain  

discrete  echo  determina(on  

full  waveform  digi(sa(on   signal  

strength  

signal   strength  

(72)

– Coordinates of the reflection points:

•  Calculated from the

position and orientation of the sensor (by GPS and INS), the deflection angle of the beam and the distance between sensor and reflection point

– Result: 3D point set along the trajectory

9.2 LIDAR

hBp://www.photo.verm.tu-­‐muenchen.de/.../EFE03_Kap23.pdf  

(73)

– Advantages

•  Uniform, dense acquisition of points

•  Acquisition of height information for DOM (with vegetation), as well as for DTM (without vegetation)

•  Accuracy in height between 50 and 15 cm in position1m

•  Fast area-wide acquisition

•  Active measuring method, nearly independent of illumination

9.2 LIDAR

hBp://www.zt-­‐stuBgart.de/.../gis_day2004_guelch.pdf  

(74)

– Disadvantages

•  Arbitrary points, no structure elements (prominent terrain points, borders)

•  Only single points, interpolation necessary

•  Relatively noisy

9.2 LIDAR

hBp://www.zt-­‐stuBgart.de/{v/{vweb/veranstaltungen/GIS-­‐Day/Rueckblick/gis_day2004_guelch.pdf  

(75)

– Reconstruction of buildings from airborne LIDAR point clouds is still subject of research

•  Building polyhedral models by intersecting detected planes

•  Bottom-up reconstruction using a given number of building parts

•  Top-down statistical

reconstruction of building roofs

9.2 LIDAR

[HBS11]  

(76)

Comparison between remotely sensed images and topographic maps

9.3 Image Processing

Proper(es  

Remotely  sensed  image   Topographic  map   Mapping  not  true  to  scale,  

image  scales  are  only  approxima$ons,     addi$onal  errors  if  terrain  is  uneven  

Mapping  true  to  scale,  only  minor   changes  due  to  generaliza$on  

Mapping  not  posi$onal  accurate,  

influenced  by  sensor  alignment,  grade,   earth  curvature,  etc.  

Mapping  posi$onal  accurate,  only   minor  changes  due  to  generaliza$on   No  parallel  projec$on   Orthogonal  parallel  projec$on  of  the  

earth‘  s  surface  on  the  map  reference   plane  

(77)

9.3 Image Processing

Content  

Remotely  sensed  image   Topographic  map   Communica$ng  informa$on  in  

images   Informa$on  coded  by  graphic  symbols  

Content  defined  causally    by  

physical-­‐chemical  processes   Content  defined  conven$onally,  s$pulated   map  symbols,  explained  in  a  legend  

High  informa$on  density,  but  

irrelevant  data  included   Low  informa$on  density,  but  all   topographically  relevant  

Unlimited  diversity  of  forms   Limited  number  of  map  symbols  

Snap  shot,  contains  transient  data   Contains  only  topographically  stable  data   Content  scale  independent,  no  

selec$on   Content  scale  dependent,  reduc$on  of  

informa$on  by  generaliza$on  

Up  to  date  ,  short  produc$on  $me   Not  up  to  date,  long  produc$on  $me,   problem  of  revision  

(78)

9.3 Image Processing

Readability  and  interpreta(on  

Remotely  sensed  image   Topographic  map   Varying  image  quality   Uniform  map  quality  

No  readability,  objects  have  to  be  

interpreted   Objects  are  directly  readable  as  they   are  represented  by  clearly  defined   symbols    

Ambiguous,  as  interpreta$on  depends  

on  the  interpreter     Unambiguous  independent  of  the   user    

Real  3d  impression  possible,  if  third  

dimension  by  stereoscopy  captured   No  real  3d  impression,  third  

dimension  may  only  be  coded  by   symbols  

Interpreta$on  scale  dependent,  

resolu$on  determines  if  objects  can  be   recognized  

Readability  scale  independent,   granted  by  generaliza$on  

(79)

9.3 Image Processing

Visual  comparison  

Remotely  sensed  image   Topographic  map  

[AS14]  

(80)

•   Geometric errors, distortions

–  Inaccurate position and form of objects –  Causes

•  Recording techniques and system

•  Relief

•  Platform (instability, motion)

•   Radiometric errors

–  Faulty pixel values –  Causes

•  Atmospheric interference

•  Topographical effects

•  Technical defects (sensors, data transfer)

9.3 Image Processing

hBp://www.fas.org/irp/  

(81)

•  Goals of geometric corrections

– Represent objects in uniform scale and true geometry (system correction)

– Register overlapped images of a scene from different dates and views (image to image registration)

– Register the image to real world map coordinates (image to map registration)

•  The  planimetrically            

corrected  image                

is  called                

orthophoto  

9.3 Geometric Errors

[AS14]  

aerial  photo,  uncorrected    corrected  →  orthophoto  

(82)

•  Radial displacement

– Causes objects to be displaced outward from the nadir

– Increases with the height of the object and distance from the nadir

– E.g. tops of buildings are

displaced outward relative to the bases

9.3 Geometric Errors in Photographic Systems

(83)

9.3 Geometric Errors in Photographic Systems

[SX08]  

(84)

•   Varying scale

–  Mapping scale changes with variations in terrain

–  The scale of objects closer to the camera is larger than that of objects being further away

–  The mapping of a rectangle that covers a terrace is not a rectangle

9.3 Geometric Errors in Photographic Systems

higher  

lower   Map:  

constant  scale   Aerial  photo:  

varying  scale  

terrace  

hBp://homepage.univie.ac.at/thomas.engleder/  

(85)

•  Capturing a scene (image) takes a certain time

•  During the recording time the earth rotates

eastward, so that the starting point of the last scan line is further west than that of the first line

•  Displacement depends on the relative speed of the satellite, the earth rotation, and the size of the image

•   Example (Landsat 7):

–  33.8°S (Sidney)

–  Image size: 185 km

Offset: 10.82 km (~ 6%)

9.3 Geometric Errors in Scanners

pixel   satellite  

mo(on↓   earth  rota(on    →  

hBp://ladamer.org/Feut/pdf/Kursbegleitung/  

(86)

•  Whiskbroom scanner

– The distance between sensor and terrain increases towards the edges

– Size of scanning spots increases towards the edges

9.3 Geometric Errors in Scanners

[AS14]  

scan  direc(on   flight  

direc(on

↑  

hBp://ladamer.org/Feut/pdf/Kursbegleitung/  

dbv_vl/dbv_vl_kapitel3.pdf  

(87)

– If the angular speed is constant, the image seems to be increasingly compressed towards the edges

– More elevated surfaces are perpendicular moved away from the flight direction

9.3 Geometric Errors in Scanners

[AS14]  

hBp://homepage.univie.ac.at/.../lba_fe_28102004.pdf  

(88)

•  Image geometry depends on the depression angle and the terrain

•  Oblique perspective (i.e. side-looking) leads to relief displacement

– The type and degree

of relief displacement in the radar image is a

function of the angle at which the radar

beam hits the ground

9.3 Geometric Errors in Radar Systems

(89)

•  Foreshortening

– Compression of those features in the scene which are tilted toward the radar

– Foreshortening effects are

reduced with increasing

incident angles

9.3 Geometric Errors in Radar Systems

hBp://www.ccrs.nrcan.gc.ca/.../bas_intro_e.pdf   hBp://www.geoinforma$on.net/  

(90)

•   Radar shadow

–  Areas not illuminated by the radar

–  Caused by either concave or convex relief features if the slope on the opposite side of the antenna is larger than the depression angle

–  Typical in high relief

terrain

–  Occur in the down-

range direction

–  Most prominent

with large incidence

angle illumination

9.3 Geometric Errors in Radar Systems

hBp://www.ccrs.nrcan.gc.ca/resource/tutor/gsarcd/pdf/bas_intro_e.pdf  

(91)

•  Layover

– Occurs when the reflected energy from the upper

portion of a feature is received before the return from its lower

– The top of the feature will be

displaced, or "laid over"

relative to its base

9.3 Geometric Errors in Radar Systems

hBp://www.ccrs.nrcan.gc.ca/.../bas_intro_e.pdf   hBp://history.nasa.gov/  

(92)

•  Instability of the platform (aircraft)

9.3 Geometric Errors

change  of  flight   speed  

pitching   change  of  

al(tude   rolling  

yawing  

[AS14]  

hBp://wdc.dlr.de/data_products/SURFACE/LCC/diplomarbeit_u_gessner_2005.pdf  

(93)

•  Model-based correction algorithm

– Develop a model for a given recording technique and platform that considers all its

inherent causes for distortions

– Parameterize the model to fit the actual conditions under which the image was taken

– Suitable if the kind and cause of the distortion is known, as earth rotation, satellite orbit or positional parameters of the platform

9.3 Geometric Corrections

hBp://www.der-­‐schweighofer.at/  

(94)

•  Mathematical function to map the positions of

pixels on the coordinates of the same points in a map

– Independent of the sensor platform – Commonly used

– Uses ground control points (GCPs)

i.e. features visible on the image with

known ground coordinates

9.3 Geometric Corrections

corrected  image   raw  image   e  

n   e  =  f  (c,r)   r   c  

n  =  f  (c,r)  

(95)

– Assigns to each pixel a new position in the reference grid

– Needs 6 GCPs for two-dimensional second order

polynomials (12 unknowns)

– Involves the following steps:

I.  Choice of a suitable function

(mapping)

II.  Coordinate transformation III.  Resampling (interpolation)

9.3 Geometric Corrections

(96)

•  Example: image to image geocorrection

– Matching the coordinate systems or column and row systems of two digital images

– One image acting as a reference image and the other as the image to be rectified

•  Reverence image

– Satellite imagery from GoogleMaps

•  Input image

– Mathematically distorted reference image

9.3 Image Rectification

(97)

•  Reference image

9.3 Image Rectification

(98)

•  Mathematical distortions

– Central projection – Change of altitude – Pitching

– Rolling – Yawing

9.3 Image Rectification

(99)

•  Distorted image

9.3 Image Rectification

(100)

•  Ground control point (GCP)

– Need to be accurately located on the image, e.g.

highway crossings, building corners

– Should be well distributed on the reference and the distorted image

– Number of necessary GCPs depends on the function used for rectification

– Can be used to determine the quality of the rectification, if more GCPs than needed are defined

9.3 Image Rectification

+   +  

+  

+  

(101)

•  Reference image with ground

control points

9.3 Image Rectification

(102)

•  Distorted image with ground

control points

9.3 Image Rectification

(103)

•  Mapping functions

– Polynomials are often used

•  Degree 1 needs 3 GCPs

•  Degree 2 needs 6 GCPs

•  Degree 3 needs 10 GCPs

9.3 Image Rectification

hBp://en.wikipedia.org/wiki/Polynomial  

(104)

•  Polynomial of degree 1

9.3 Image Rectification

(105)

•  Polynomial of degree 2

9.3 Image Rectification

(106)

•  Polynomial of degree 3

9.3 Image Rectification

(107)

•  Reference image

9.3 Image Rectification

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