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groundtruth collection for remotesensing support

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groundtruth collection for remotesensing support

  1. 1. Ground Truth Collection For Remote Sensing Support Presented by : P.Thiruvengadam M.Tech Geoinformatics
  2. 2. Remote Sensing Definition: The science and art of obtaining information about an object, area, or phenomenon through the analysis of data acquired by a device that is not in contact with the object, area, or phenomenon under investigation (L&K,1994) Example : Human Visual system
  3. 3. Principles Of Remote sensing • Detecting and recording of radiant energy reflected or emitted by objects or surface material • Different objects return different amount of energy in different bands of the electromagnetic spectrum, incident upon it. • Reflection or emmitance of electromagnetic spectrum depends on • Property of material (structural, chemical, and physical). • Surface roughness. • Angle of incidence. • Intensity. • Wavelength of radiant energy.
  4. 4. Stages In Remote Sensing
  5. 5. Electromagnetic Energy • Energy propagated in the form of an advancing interaction between electric and magnetic fields (Sabbins, 1978) • The electromagnetic is normally used as an information carrier in remote sensing. • Travels with the velocity of light. • The electromagnetic spectrum ranges from the shorter wavelengths (including gamma and x rays) to the longer wavelengths (including microwaves and broadcast radio waves) • Most of the remote sensing systems operate in visible, infrared (IR) and microwave regions
  6. 6. • Visible region EMR Spectrum ‒ Small region in the range 0.4 - 0.7 μm ‒ Blue : 0.4 – 0.5 μm ‒ Green: 0.5-0.6 μm ‒ Red: 0.6-0.7 μm. ‒ Ultraviolet (UV) region adjoins the blue end ‒ Infrared (IR) region adjoins the red end • Microwave region ‒ Longer wavelength intervals ‒ Ranges from 0.1 to 100 cm ‒ Includes all the intervals used by radar systems.  Infrared (IR) region ‒ Spanning between 0.7 and 100 μm ‒ 4 subintervals of interest for remote sensing (1) Reflected IR (0.7 - 3.0 μm) (2) Photographic IR (0.7 - 0.9 μm) (3) Thermal IR at 3 - 5 μm (4) Thermal IR at 8 - 14 μm
  7. 7. Remote Sensing Platforms • Ground level remote sensing – Very close to the ground (e.g., Hand held camera) – Used to develop and calibrate sensors for different features on the Earth’s surface • Aerial remote sensing – Low altitude aerial remote sensing – High altitude aerial remote sensing • Space-borne remote sensing – Space shuttles – Polar orbiting satellites – Geo-stationary satellites
  8. 8. Real Remote Sensing System Energy Source • Ideal system: Constant, high level of output over all wavelengths • Real system:  Usually non-uniform over various wavelengths  Energy output vary with time and space  Affects the passive remote sensing systems – The spectral distribution of reflected sunlight varies both temporally and spatially – Earth surface features also emit energy in varying degrees of efficiency  A real remote sensing system needs calibration for source characteristics.
  9. 9. The Atmosphere Ideal system: A non-interfering atmosphere Real system:  Atmosphere modifies the spectral distribution and strength of the energy transmitted through it  The effect of atmospheric interaction varies with the wavelength associated, sensor used and the sensing application  Calibration is required to eliminate or compensate these atmospheric effects
  10. 10. The Energy/Matter Interactions at the Earth's Surface • Ideal system: A series of unique energy/matter interactions • Real system:  Spectral signatures may be similar for different material, making the differentiation difficult  Lack of complete understanding of the energy/matter interactions for surface features The Sensor • Ideal system: A super sensor • Real system:  Fixed limits of spectral sensitivity i.e., they are not sensitive to all wavelengths.  Limited spatial resolution (efficiency in recording spatial details).  Sensor selection requires a trade-off between spatial resolution and spectral sensitivity. – For example, photographic systems have very good spatial resolution , but poor spectral sensitivity. Non-photographic systems have poor spatial resolution.
  11. 11. Advantages of Remote Sensing • Major advantages of remote sensing are  Provides data for large areas  Provide data of very remote and inaccessible regions  Able to obtain imagery of any area over a continuous period of time – Possible to monitor any anthropogenic or natural changes in the landscape  Relatively inexpensive when compared to employing a team of surveyors  Easy and rapid collection of data  Rapid production of maps for interpretation
  12. 12. Limitations of Remote Sensing • Some of the drawbacks of remote sensing are  The interpretation of imagery requires a certain skill level  Needs cross verification with ground (field) survey data  Data from multiple sources may create confusion  Objects can be misclassified or confused  Distortions may occur in an image due to the relative motion of sensor and source
  13. 13. Ground Truth • Ground truth is simply observations or measurements made at or near the surface of the earth in support of an air or space-based remote sensing survey (UCSC). • It may also be referred to as ancillary data or reference data. • Ground truth may consist of several types of data acquired before, during, and after an image acquisition
  14. 14. Sources of Ground Truth • Field observations. • In situ spectral measurements. • Aerial reconnaissance and photography. • Descriptive reports. • Inventory tallies. • Maps
  15. 15. Examples of Ground Truth • Field-based spectroscopic measurements of representative materials of interest such as trees, shrubs, rock outcrops, soils, water, and manmade objects such as roads and buildings • Meteorological conditions at time of over flight (including temperature, wind speed and direction, precipitation, etc). • Chemical and biochemical measurements such as chlorophyll content of tree canopies or chemical constituent identification within waterways.
  16. 16. • Rock and mineral analysis and collection including such things as permeability tests, grain size estimates, and simple hand sample identification • Field mapping of both biological and geological materials and their distributions, including gross species and lithological identification • Collection of previous work such as maps other chemical analyses, GIS information and any other remotely sensed data
  17. 17. Ground Truth Collection for RS • Correlate surface features and localities as known from familiar ground perspectives with their expression in satellite imagery • Provide input and control during the first stages of planning for analysis, interpretation, and application of remote sensing data (landmark identification, logistics of access. etc.) • Reduce data and sampling requirements (e.g., areas of needed coverage) for exploration, monitoring, and inventory activities
  18. 18. •Select test areas for aircraft and other multistage support missions (e.g., under flights simultaneous with spacecraft passes) •Identify classes established by unsupervised classification •Select and categorize training sites for supervised classification •Verify accuracy of classification (error types and rates) by using quantitative statistical techniques •Obtain quantitative estimates relevant to class distributions (e.g. field size; forest acreage)
  19. 19. • Collect physical samples for laboratory analysis of phenomena detected from remote sensing data (e.g., water quality; rock types; insect-induced disease) • Acquire supplementary (ancillary) non-remote sensing data for interpretive model analysis or for integration into Geographic Information Systems • Develop standard sets of spectral signatures by using ground-based instruments • Measure spectral and other physical properties needed to stipulate characteristics and parameters pertinent to designing new sensor systems
  20. 20. Source:http://ces.iisc.ernet.in/
  21. 21. Multi Approach Ground truth activities are an integral part of the “Multi" approach: • Multistage: Data should be procured whenever possible from different platforms • Multilevel : Data collected at various distances from Earth’s surface. • Multispectral : Data collected over various regions of the spectrum. • Multi temporal :Data obtained at different times. • Multi phase: some data correlate with one another and also with other remote sensing data.

Notes de l'éditeur

  • Rayleigh scattering occurs when particles are very small compared to the wavelength of the radiation. These could be particles such as small specks of dust or nitrogen and oxygen molecules. Rayleigh scattering causes shorter wavelengths of energy to be scattered much more than longer wavelengths. Rayleigh scattering is the dominant scattering mechanism in the upper atmosphere. The fact that the sky appears "blue" during the day is because of this phenomenon. As sunlight passes through the atmosphere, the shorter wavelengths (i.e. blue) of the visible spectrum are scattered more than the other (longer) visible wavelengths. At sunrise and sunset the light has to travel farther through the atmosphere than at midday and the scattering of the shorter wavelengths is more complete; this leaves a greater proportion of the longer wavelengths to penetrate the atmosphere.
    Mie scattering occurs when the particles are just about the same size as the wavelength of the radiation. Dust, pollen, smoke and water vapour are common causes of Mie scattering which tends to affect longer wavelengths than those affected by Rayleigh scattering. Mie scattering occurs mostly in the lower portions of the atmosphere where larger particles are more abundant, and dominates when cloud conditions are overcast.
    The final scattering mechanism of importance is called nonselective scattering. This occurs when the particles are much larger than the wavelength of the radiation. Water droplets and large dust particles can cause this type of scattering. Nonselective scattering gets its name from the fact that all wavelengths are scattered about equally. This type of scattering causes fog and clouds to appear white to our eyes because blue, green, and red light are all scattered in approximately equal quantities (blue+green+red light = white light).
    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.
    Ozone serves to absorb the harmful (to most living things) ultraviolet radiation from the sun. Without this protective layer in the atmosphere our skin would burn when exposed to sunlight.

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