1. Summer Session 12 July 2011

2. Basic Info Lecturer: Alyssa Whitcraft alyssakw@gmail.com Office Hours: by appointment TA: Sumalika Biswas Sumalika.biswas@gmail.com Office Hours: 4-6 pm, Tuesday/Thursday – ONLINE Grading Breakdown: ComponentPercentage of Grade 1 – 75 minute midterm exam25% 4 pop-quizzes8% 9 laboratory assignments (equally weighted)22% 1 – 120 minute comprehensive final exam40% Participation in discussion on online message board5%

3. Questions About You Introductions: Name? Major(s)/Minor(s)? Why are you taking this class? For many it is a requirement – but anything else? Any background relative to remote sensing? PLEASE POST TO THE DISCUSSION BOARD BY THURSDAY 14 JULY 2011

4. Today’s Topics Introduction to Online Interface - Questions Remote Sensing: What? and Why? Basics of Electromagentic (EM) Radiation Wave & Particle Theory Radiation Laws and Theories Lab 1 – Data Sources

5. Chat Box Yes or No (respond to questions) Raise your hand Change your “status” Click to talk, or hold down “ctrl” or “F8” You will see the slides here! Click to activate video camera Who is in the room, and what their status & capabilities are

6. A note about labs You do not have to “attend” online labs There are not enough Citrix licenses for everyone in the department of Geography to be online at once, unfortunately. Sumalika will be available for 8 hours a week Tuesday/Thursday 4-6 pm and 7:30-9:30 pm We may have to split groups into two and only allow access for half of the class at a time if it becomes an issue. Sumalika will review labs after lecture (~7:30 pm) so people are prepared to complete them on their own time If some students are repeatedly unable to login, then we (instructors) will have to take action Other options: Open lab: Monday-Friday, ~10 am – 4 pm (LEF 1136/8)

7. What is Remote Sensing? Remote sensing uses the radiant energy that is reflected, emitted, or scattered from the Earth and its atmosphere from various portions (“wavelengths”) of the electromagnetic (EM) spectrum Our eyes are only sensitive to the “visible light” portion of the EM spectrum – but there is MUCH more that remote sensing makes available/useful to us!

8. Why Remote Sensing? Electromagnetic energy being detected by remote sensors is dependent on the characteristic of the surface or atmosphere being sensed – Remote sensing provides unique information Many portions of the earth’s surface and atmosphere are difficult to sample and measure using in situ measurements Only way to systematically collect data in many regions Remote sensors can continuously collect data Reliable and consistent source of information

9. Definitions of remote sensing Our basic definition Definition 1 – Remote sensing is the acquiring of information about an object or scene without touching it through using electromagnetic energy. Issues? - we limit ourselves to electromagnetic energy, yet many systems use sound waves to acquire data. - includes smell, etc.

10. Elements of a Remote Sensing System 2. Area or scene of interest 3. Sensing Device 4. Data Recorder 5. Information Production System 6. Information Delivery System 1. Information User

11. Basic Remote Sensing System – Aerial Photography Sun Camera System - Used photographic film, paper products, and simple cartographic representations (we’ll learn more about this in Lecture 3).

12. Definitions of remote sensing Definition 2 – Remote sensing is the non-contact recording of information from the UV, visible, IR, and microwave regions of the EM spectrum by means of a variety of electro-optical systems, and the generation and delivery of information products based on the processing of these data

13. Categories of Remote Sensors Remote sensors are based on: 1. Specific regions of the EM spectrum 2. The types of EM energy being detected 3. The source of EM energy, e.g., passive versus active sensors

14. EM Spectrum Regions Used in Remote Sensing 1. Ultraviolet ( < 0.4  m) 2. Visible ( 0.4  m < < 0.7  m) 3. Reflected IR ( 0.7  m < < 2.8  m) 4. Emitted (thermal) IR ( 2.4  m < < 20  m) 5. Microwave ( 1 cm < < 1 m) = EM radiation wavelength VERY IMPORTANT!!

15. Thermal IR Sensors Thermal IR deals with the Far IR region of the EM spectrum, wavelengths between 2.4 and 20 µm Most Thermal IR scanners use wavelengths between 8 and 15 µm

16. Figure 1-18 from Elachi, C., Introduction to the Physics and Techniques of Remote Sensing, 413 pp., John Wiley & Sons, New York, 1987. Microwave remote sensing instruments operate at wavelengths greater than 1 mm

17. Categories of Remote Sensors Remote sensors are based on 1. Specific regions of the EM spectrum 2. The types of EM energy being detected 3. The source of EM energy, e.g., passive versus active sensors

18. Types of EM energy detected by remote sensors 1. Reflected energy 1. Reflected EM energy Atmosphere 2. Emitted EM energy 3. Scattered EM energy Earth surface

19. Passive vs. active systems Passive systems record energy that is emitted, scattered or reflected from natural sources (e.g., sunlight or based on the temperature of the surface or atmosphere being imaged) Active systems provide their own source of EM radiation, which is then reflected or scattered, and this signal detected by the system

20. 6000º K emitted 300º K emitted UV, Visible, Near IR Sensors Thermal IR, Microwave Sensors Active Sensors Microwave, Visible reflected emitted scattered

21. Definition of resolution Also referred to as resolving power Defined as the ability of a remote sensor to distinguish between signals that are similar Four types of resolution important in remote sensing – Spatial Spectral Radiometric Temporal  KNOW THESE!

22. Spatial Resolution The measure of the smallest distance (linear or angular separation) between objects that can be resolved by the sensor. e.g. Landsat 7  15-60 m resolution e.g. MODIS  250-1000 m resolution Figure 1-8 from Jensen

23. Spectral Resolution Refers to the dimensions (widths) and wavelength regions of the EM spectrum a specific sensor is sensitive to

24. Spectral Bands in a Visible and Near IR Remote Sensor Sensor has 6 different bands or channels Each band has a center wavelength Each band has a width

25. Spectral Resolution Most remote sensing systems collect data in 1 to 10 different wavelength regions or bands, each with broad width e.g. Landsat 7  7 visible/IR bands (including 1 thermal), and 1 panchromatic band e.g. MODIS  36 visible/IR bands Hyperspectral remote sensing systems have a large number of very narrow bands]

26. Radiometric Resolution The sensitivity of a remote sensing detector to variations in the intensity of the emitted, reflected or scattered EM energy that is being detected the precision of the system e.g. Landsat 7  8-bit system e.g. MODIS  12-bit system

27. How many different intensity levels can be discriminated by the remote sensor within a specific band? Radiometric Resolution

28. Temporal Resolution How often a remote sensor has the ability to record data over the same area e.g. Landsat 7  16 days e.g. MODIS  Daily

29. Examples of Remote Sensing Information Products Global land cover Global agricultural monitoring information – cropped area and crop production forecasts Active fire locations Ocean chlorophyll Flooding patterns in the Florida Everglades Gulf Stream flow El Nino sea surface temperature Global wind patterns Atmospheric trace gas/aerosol concentrations The Antarctic Ozone Hole Breakup of the Larsen Ice Sheet Arctic sea ice cover

31. Basic Energy Principles Energy is the ability to do work There are three ways to transfer energy from one place or object to another Conduction Convection Radiation – energy emitted into space by any object above 0 degrees K

32. Conduction – transfer of energy through collisions of atoms or molecules

33. Convection - physically moving the molecules/atoms from one place to another

34. Radiation – energy emitted into space by any object above 0° K

35. Models of EM Radiation 1. Wave Model of EM Energy – describes how EM radiation is propagated, e.g., how it moves through space 2. Particle Model of EM Energy – describes how EM radiation interacts with matter

36. The Electromagnetic Wave EM energy travels with the speed of light, c, Within a vacuum c = 3 x 10 8 m sec -1

37. The Electromagnetic Wave EM energy consists of two fluctuating fields perpendicular to each other and both perpendicular to the direction of energy movement 1. An electrical field 2. A magnetic field

39. Polarization Polarization refers to the relative orientation of the electrical field of an EM wave Horizontal polarization - an EM wave that is parallel to the earth’s surface Vertical polarization - an EM wave that is perpendicular to the earth’s surface  an important consideration in microwave remote sensing

40. Radar systems control the polarization of both the transmitted and received microwave EM energy Figure 9.6 from Jensen

41. Characteristics of EM radiation Created whenever an electrical charge is accelerated Two characteristics of EM waves Wavelength ( ) – depends on the length of time over which the electrical charge is accelerated Frequency ( ) depends on the number of accelerations per second

43. EM Frequency ( ) Frequency is expressed in hertz, where one hertz is one cycle or wavelength per second Shorter wavelengths have higher frequencies Longer wavelengths have lower frequencies

44. Relationship between c,, and  c = = c / - In visible, near IR, and thermal IR remote sensing, wavelength ( ) is used to describe a system In microwave remote sensing, frequency ( ) is often used to describe a system

45. Stefan-Boltzman Law* The total emitted radiation from a blackbody** (M) measured in Watts m -2 is proportional to the fourth power of its absolute temperature (T) measured in Kelvin (K), and is calculated: M =  T 4 where  is a constant (5.6697 x 10 -8 W m -2 K -4 ) *Know this formula and be able to describe what it represents ** a blackbody is a theoretical construct that absorbs and radiates energy at the maximum possible rate per unit area at each wavelength for a given temperature.

46. Planck’s formula** Spectral emittance – S( ) S( ) = 2  h c 2 / [ 5 (e ch /  kT – 1)] Where h is Planck’s constant And k is the Stephan-Boltzman constant **you do NOT have to know this formula

47. Planck’s formula gives basic shape of emittance curves Stephan Boltzman Law predicts how much total energy is emitted Note how total energy drops dramatically as temperature decreases

48. Wien Displacement Law* The wavelength with the highest level of emitted radiation ( max ) for an object of temperature T can be calculated as max = k / T where k = 2898  m ºK *know this formula and be able to describe what it represents

49. Examples of Wien’s Displacement Law T (sun) = 6000º K max = k / T = 2898/6000 = 0.483  m T (earth) = 300º K max = k / T = 2898/300 = 9.66  m

50. Wein Displacement Law shows that as temperature increases, the wavelength of maximum emission decreases

52. EM Spectrum Regions Used in Remote Sensing Ultraviolet – 0.3 to 0.4  m Visible – 0.4 to 0.7  m Near Infrared – 0.7 to 1.3  m Middle Infrared – 1.3 to 3.0  m Thermal Infrared – 3 to 14  m **note: TIR goes from 2.4-30  m, but only the region above is actually used. Microwave – 1 mm to 1 m

53. Radar systems operate in the microwave region of the EM spectrum Figure 9.2 from Jensen

54. EM Radiation Particle Model - Radiation from Atomic Structures Einstein discovered that when light (EM radiation) interacts with matter, it behaves like it is composed of photons Photons carry energy and momentum, i.e., particle like properties Thus, light is considered to be a unique type of matter

56. Sources of EM radiation used in remote sensing Sun and stars – (UV, visible, near and middle infrared) All bodies with temperature > 0 ºK (far or thermal IR and microwave) Radio transmitters (microwave region) Lasers (UV, visible)

57. Microwave Transmitter / Receiver Antenna Microwave EM energy pulse transmitted by the radar Microwave EM energy pulse reflected from a target that will be detected by the radar Target

58. Laser Device that emits a high-intensity, narrow-spectral- width, highly directional or near-zero-divergence beam of light by stimulating electronic, ionic, or molecular transitions to higher energy levels and allowing them to fall to lower energy levels

59. Notes on Lab 1 Purpose To show you the wealth of data available for free online To show you the steps to acquiring it. There are multiple online databases of free remotely sensed data. Dr. John Townshend (BSOS Dean) helped create the Global Land Cover Facility (GLCF)… you’ll be using this today to acquire Landsat ETM+ and TM data. Another data repository = WIST… you’ll be using that for MODIS. There are several other repositories – LAADS, GLOVIS…