introduction_to_remote_sensing GIS.pptx

Remote sensing briefly explained

1. Introduction to Remote Sensing

2. What is REMOTE SENSING ? REMOTE SENSING includes all methods and techniques used to gain qualitative and quantitative information about distant objects without coming into direct contact with these objects. Look-Look, NO Touch

3. What is REMOTE SENSING ? Remote Sensing (RS) methods try to answer four basic questions: HOW MUCH of WHAT is WHERE? What is the SHAPE and EXTENT of ... ? (Area, Boundaries, Lineaments, ...) Has it CHANGED? What is the MIX of Objects

4. What is REMOTE SENSING ? HOW MUCH of WHAT is WHERE? WHAT: Type, Characteristic and Properties of Object. Eg. Water, Vegetation, Land; Temperature, Concentration, State of Development; Subtype, Species, Use of ... ; Includes determination of generic object type, character and property as well as it’s abstract meaning. => DATA INTERPRETATION

5. What is REMOTE SENSING ? HOW MUCH of WHAT is WHERE? HOW MUCH: determine by simple COUNTING, measuring AREA covered or percentage of total area coverage. WHERE: Relate locations and area covered to either a standard map or to the actual location on the ‘ground’ where the object occurs. NOTE: WHERE also refers to a moment in time

6. What is REMOTE SENSING ? What is the SHAPE and EXTENT of ... ? (Area, Boundaries, Lineaments, ...) This extends the ‘WHERE’ to be a completely GEOMETRIC problem. MAP PRODUCTION methods are to be applied to the analysis of RS information. These include: Photogrammetric Methods : Identification and Delineation of Boundaries and Lineaments (Roads, Rivers, Fault Lines)

7. What is REMOTE SENSING ? Has it CHANGED? CHANGE may occur with progress of TIME. Change may be detected through comparison of observed states at different moments in time. => CHANGE DETECTION

8. What is REMOTE SENSING ? What is the MIX of Objects? The surface of the Earth is covered by objects like Soil, Water, Grass, Trees, Houses, Roads and so on. These are ‘GENERIC OBJECTS’. We know these well, but we also know objects like Open Forest, Residential and Industrial Estates, etc. Each of these ABSTRACT OBJECTS are made up of a typical collection of Generic Objects.

9. What is REMOTE SENSING ? What is the MIX of Objects? One important task for Remote Sensing is to identify GENERIC OBJECTS as well as ABSTRACT OBJECTS within areas of interest The following lessons will be devoted to techniques and methods as well as to the logistic for finding answers to the four basic questions.

10. What is REMOTE SENSING ? Remote Sensing (Look-Look, No Touch) is a much wider field than we will discuss in this lecture series. We will concentrate on that part of RS dealing with EARTH LAND RESOURCES Vision Medical Imaging Sound and Radio Wave Detection

11. What is REMOTE SENSING ? What makes it tick ??? (1) RS requires a CARRIER of information, which can bridge distances. (2) RS requires a SENSOR which can detect changes in the carried Signal. (3) RS requires RECORDING, ANALYSIS, INTERPRETATION and REPRESENTATION of the sensed information in a purposeful way.

12. What is REMOTE SENSING ? (1) RS requires a CARRIER of information, which can bridge distances. These Carriers of Information are FIELDS of FORCES: * Pressure Wave Fields of Sound, * Gravity Force Fields, * Magnetic Force Fields and * Electro-magnetic Force Fields. The latter are of our main interest, since they include visible and invisible LIGHT.

13. What is REMOTE SENSING ? (2) RS requires a SENSOR which can detect changes in the carried Signal. Apart from our own eyes and ears, technology has provided us with a multitude of sensors operating in the detection of force fields: microphones, geophones, photographic film, video cameras and photo detectors, radio wave receivers, gravimeters and magnetometers.

14. What is REMOTE SENSING ? (3) RS requires RECORDING, ANALYSIS, INTERPRETATION and REPRESENTATION of the sensed information in a purposeful way. This is a technique based topic. It is essential for the success or failure of RS in respect of it’s anticipated purpose. This topic will be dealt with in it’s main aspects (but not completely) in the following lessons.

15. What is REMOTE SENSING ? Source of Force Field Object (generic) Reflection Sensor System eg. Camera Resulting RS Data Set eg. Image DATA ACQUISITION

16. What is REMOTE SENSING ? Object(s) RS Data Set eg. Image DATA PROCESSING Interpretation (secondary) Measurements Data Processing & Mapping (geometric) Presentation of Processing Results Explaining deduced OBJECT INFORMATION

17. ER, the Physical Basis of RS Fraunhofer, Joseph (1877-1826), German optician and physicist, Spectroscopy Wien, Wilhelm (1864-1928), German physicist, 1911 Nobel Prize in Physics, Wien’s Displacement Law Planck, Max Karl Ernst Ludwig (1858-1947), German physicist, 1918 Nobel Prize in Physics, laid basis to Quantum Physics, developed Planck’s Law Einstein, Albert (18779-1955), German(?) physicist, 1921 Nobel Prize in Physics, General Theory of Relativity, and E = m c^2 Serious, Jahoo (still alive), son of Tasmanian apple grower,, How to put bubbles into beer: E = m c^2

18. ER, the Physical Basis of RS Fraunhofer discovered ‘black lines’ in the spectrum of light emitted by various superheated chemical elements. These lines were as typical for each of the elements as fingerprints for humans. Chemical Composition of objects effects emitted ER in a unique way for each element. Fraunhofer Lines (found empirically by observation)

19. ER, the Physical Basis of RS In Einstein's formula E = mc^2 E = Energy m = mass (of matter/object) c = propagation velocity of light What does that tell us ? There is a well defined relationship between MATTER, ENERGY and ELECTROMAGNETIC RADIATION (eg. light) Fraunhofer Lines E = mc 2

20. ER, the Physical Basis of RS The basic building blocks of all matter are ATOMS The basic building blocks of Atoms are the NUCLEUS (Neutrons and Protons) and several ELECTRONS. Electrons are thought to be spinning around the Nucleus at orbits of different, but well pre-defined discrete sequential radii.

21. ER, the Physical Basis of RS Neutrons are thought to carry NO Energy charge. Protons are thought to carry a charge of energy defined as being positive. Electrons are thought to carry a charge of energy defined as being negative. Because of the dual polarity (positive <=> negative) an energy potential exists between Nucleus and Electrons

22. ER, the Physical Basis of RS An equal number of Electrons and Protons exist in all atoms (isotopes excluded). A balance exists quasi mechanical between the attraction forces of opposite charges and centrifugal forces of the spinning Electrons. This balance is an intricate compromise of these forces and the actual energy level inherent to each atom.

23. ER, the Physical Basis of RS The energy level contained in an atom can be changed (eg. by heating or cooling). The balance of forces inside the atom will automatically adept to energy level changes by moving electrons to higher or lower orbits.

24. ER, the Physical Basis of RS To have an electron move from it’s current orbit to the next outer orbit, an energy amount equal to one Planck’s Quantum has to be added to the atom (eg. by heating). To have an electron drop back from an outer orbit to the next inner one, the same amount of energy has to be extracted from the atom.

25. ER, the Physical Basis of RS It is this EXTRACTION of energy from an atom when electrons drop back to lower orbits which is of interest to us. One widely accepted theory says, that atoms lose energy in form of Electromagnetic Radiation Energy differential = 1 Planck’s Quantum

26. ER, the Physical Basis of RS Electromagnetic Radiation One theory explains ER as a WAVE field, another as a field of a stream of PHOTONS, particles so small that they have no mass. Both are said to propagate at light speed. Energy differential = 1 Planck’s Quantum E = mc^2 Photon Wave

27. ER, the Physical Basis of RS Electromagnetic Radiation Some atoms may have been charged to a higher energy level; pushing electrons further than one orbital level. In turn they can drop back over more than one orbit level: more energy than one Quantum Energy differential = 1 Planck’s Quantum E = mc^2 Photon Wave c = const ~ 300000 km/sec

28. ER, the Physical Basis of RS Electromagnetic Radiation Gerd’s interpretation: Since c is constant, all photons travel about 300,000 km/sec Those with a higher energy charge will use a ‘more wiggly’ (thus, longer) wave path than those with lesser charge. Energy differential = 1 Planck’s Quantum E = mc^2 Photon Wave c = const ~ 300000 km/sec 2 Quantum charge

29. ER, the Physical Basis of RS Electromagnetic Radiation Wave characteristics:  = Wave length = distance between consecutive wave peaks (measured in  m) f = frequency = number of wave peaks (wiggles) in the wave train propagating for 1 sec (measured in Hz)  = c / f c = const ~ 300000 km/sec 

30. ER, the Physical Basis of RS Electromagnetic Radiation Summing up: High Energy Radiation proceeds at higher frequencies (shorter wavelength compared to low energy radiation. Radiation wave length mix depends on amount of (heat) energy contain in an atom PLANCK’s LAW c = const ~ 300000 km/sec 

31. ER, the Physical Basis of RS PLANCK’s LAW c = const ~ 300000 km/sec  Wave Length  Total Radiation Energy emitted Radiation Energy Curve for an object (BLACK BODY) at constant temperature. short long peak

32. ER, the Physical Basis of RS WIEN’s DISPLACEMENT LAW 0K = -273 degree Celsius 300K = 27 degree Celsius  Wave Length  Total Radiation Energy emitted Radiation Energy Curves for an object (BLACK BODY) at various constant temperatures. short long 300K 1000K 3000k 6000K

33. ER, the Physical Basis of RS Using Fraunhofer’s Observations A Black Body is a theoretical, not a real object. Real Objects will produce somewhat different radiation output pattern. c = const ~ 300000 km/sec  Wave Length  Radiation Energy Curve for an object at constant temperature. short long Gerd’s real object

34. ER, the Physical Basis of RS Using Fraunhofer’s Observations The variation in Radiation output from a REAL OBJECT depends on it’s chemical composition. Water has a different SPECTRAL SIGNATURE than soil or chlorophyll containing leaf matter, etc. Wave Length  Radiation Energy Curve for an object at constant temperature. short long Gerd’s real object QUESTIONS: Can we use these facts to measure object temperatures? Can we use these facts to identify the chemical composition of objects and can we use the latter to identify the object itself?

35. ER, the Physical Basis of RS WIEN’s DISPLACEMENT LAW Wave Length  Total Radiation Energy emitted Radiation Energy Curves for an object (BLACK BODY) at constant temperatures. short long 300K 1000K 3000k 6000K The Average Temperature of Earth’s Surface rarely exceeds 300 K, an object temperature to low to provide for EMITTED RADIATION of sufficient strength to register on most of the available sensors (except in thermal IR). (Even warm nights can be pitch black)

36. ER, the Physical Basis of RS WIEN’s DISPLACEMENT LAW Wave Length  Total Radiation Energy emitted Radiation Energy Curves for an object (BLACK BODY) at constant temperatures. short long 300K 1000K 3000k 6000K The surface of the Sun’s outer atmosphere (photosphere) has a temperature of about 5800K, hot enough to provide adequate radiation energy. (Peak output in GREEN of visible light). Most RS systems utilise reflected sun light.

37. ER, the Physical Basis of RS WIEN’s DISPLACEMENT LAW Wave Length  Total Radiation Energy emitted Radiation Energy Curves for an object (BLACK BODY) at constant temperatures. short long 300K 1000K 3000k 6000K QUESTION: Does incident sun light interact in a similar way with matter as described is the case for emitted radiation? ANSWER: YES! ER (including light) is a form of energy (as is heat). Matter (atoms) can absorb as well as emit energy.

38. ER, the Physical Basis of RS WIEN’s DISPLACEMENT Wave Length  Total Radiation Energy emitted Radiation Energy Curves for an object (BLACK BODY) at constant temperatures. short long 300K 1000K 3000k 6000K Objects under illumination by sun light will partially absorb radiation. Absorption level varies with wave length depending on chemical composition of the object Radiation not absorbed is mostly reflected and available for RS. Spectral Signatures

39. ER, the Physical Basis of RS Examples of Spectral Signatures (not to exact scale; see Textbook) 50 0.4 (blue) 0.8 0.6 (red) 0.5 (green) 0.7 (IR=>) 1.0  m  Reflectance (of Sun Light) Bare Soil (Grey/Brown) Vegetation (green) Water (clear) (<= UV)

40. ER, the Physical Basis of RS The Electromagnetic Spectrum (not to exact scale; see Textbook) 10^-6 10^-3 1 100 0.1 10^5 10^8  -Rays  Sound X-Ray UV Visible 0.4 0.5 0.6 0.7  m  m TV/Radio Micro- Wave Thermal Infrared Near & Mid Infrared Wave Length not part of ER) Note: outside the visible Range, no colours or shades will be perceived. Blue Green Red

41. ER, the Physical Basis of RS The General Remote Sensing Model I R A T A Sensor Radiation Source I = R + A + T Simplified Radiation- Balance R = I - A - T I = Incident ER R = Reflected A = Absorbed T = Transmitted S = Scattering S

42. ER, the Physical Basis of RS A bright Idea for RS 50 0.4 (blue) 0.8 0.6 (red) 0.5 (green) 0.7 (IR=>) 1.0  m  Reflectance (of Sun Light) Bare Soil (Grey/Brown) Vegetation (green) (<= UV) G R IR Veg. Soil G med med R low high IR high+ high Truth Table

43. ER, the Physical Basis of RS A bright Idea for RS G R IR Truth Table Veg. Soil G med med R low high IR high+ high

44. Landsat 7