FOR 353: Air Photo Interpretation and Photogrammetry. Lecture 2. Electromagnetic Energy/Camera and Film characteristics

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FOR 353: Air Photo Interpretation and Photogrammetry Lecture 2 Electromagnetic Energy/Camera and Film characteristics

Lecture Outline Electromagnetic Radiation Theory Digital vs. Analog (i.e. film ) Systems

Lecture Outline Electromagnetic Radiation Theory Digital vs. Analog (i.e. film ) Systems

Electromagnetic Spectrum EMR is energy propagated through space in the form of tiny energy packets called photons that exhibit both wave-like and particle-like properties.

Electromagnetic Spectrum Fundamental Interactions Sun energy: is radiated by atomic particles at the source (the Sun) propagates through the vacuum of space at the speed of light interacts with the Earth s atmosphere interacts with the Earth s surface interacts with the Earth s atmosphere once again, and finally reaches the remote sensor, where it interacts with various optical systems, filters, film emulsions, or detectors

Electromagnetic Radiation Energy Source and Measurement Units The Sun is the most common energy source - Sunlight travels at a speed of 186,000 m/s Wavelength (λ) is used to describe the spectrum of light. - Micrometer (μm) (1/1000 of a millimeter) - Nanometer (nm) (1 billionth of a meter) example: light in the visible portion of the spectrum ranges from 0.4 0.7 μm. In nanometers this would read: 400 700 nm

Electromagnetic Radiation Energy Source and Measurement Units Different sensors are required to capture and record the different wavelengths Photographic film (0.4-0.9 μm) Landsat satellite (0.45 2.35 μm optical; 10.4 12.5 μm thermal) MODIS satellite (0.62-14.38 μm) Human Eye (0.4-0.7 μm)

Electric field Wavelength and Frequency n = frequency Amplitude Transmission direction Units of wavelength: Nanometers: 1 nm = 10-9 m Micrometers: 1 μm = 10-6 m Angstroms: 1 Åm = 10-10 m c = λv where: λ = wavelength (m) V = frequency (cycles/second, Hz) c = speed of light (3x10 8 m/s)

Wavelength and Frequency c = λv Note: frequency is inversely proportional to wavelength def wavelength (λ) def frequency (V) - the mean distance between maximums of roughly periodic pattern the number of wavelengths that pass a point in time

ULTRA-VIOLET Electromagnetic Spectrum Frequency (MHz) 14 13 12 11 10 9 8 7 6 5 4 3 2 10 10 10 10 10 10 10 10 10 10 10 10 10 INFRARED MICROWAVES GAMMA RAYS X RAYS NEAR MIDDLE THERMAL RADAR RADIO, TV. UHF VHF 0.01 0.1 1 10 100 0.1 1 10 100 0.1 1 10 1 10 Wavelength ( l ) Angstroms Micrometers Centimetres Meters VISIBLE SPECTRUM BLUE GREEN RED 0.4 0.5 0.6 0.7 µ m

VIS Visible region 0.4-0.7 µm Electromagnetic Spectrum NIR Near-infrared (0.7 1.2 µm) - discriminate green vegetation MIR Mid-infrared (1.2 8 µm) [SWIR - Shortwave IR (1.2 3 µm)] *1.3-2.5 µm used for soil and vegetation moisture contents, *3-5 µm used for detecting high-temperature sources TIR Thermal infrared (8 14 µm) Helps to map surface temperatures, useful in detecting vegetation stress and clouds, and in assessments of environmental condition Microwave region (>1 mm)

Color White Light Composed of three primary additive colors: red, green, blue These colors can t be created by adding other colors together (Additive color model) Composed of three primary subtractive colors: cyan, magenta, yellow These are created by adding together two primary additives (Subtractive color model) Adding all three primary additive colors of light produces the color white

Electromagnetic Radiation Electromagnetic Energy EM energy only detected when it interacts with matter EM energy generally travels in a straight line from its source Once EM energy interacts with a medium, it may be altered (Reflection, Transmission, Absorption)

Electromagnetic Radiation Electromagnetic Energy: Reflection The ratio of energy reflected from an object to the energy incident upon the object Two types: 1. Specular 2. Diffuse Reflection

Electromagnetic Radiation Electromagnetic Energy: Reflection The ratio of energy reflected from an object to the energy incident upon the object Two types: 1. Specular 2. Diffuse Scattering

Electromagnetic Radiation Electromagnetic Energy: Absorption Incident energy does not bounce off an object, nor pass through it. Energy is converted to some other form, such as heat. Differences in absorptive qualities of objects result in color Absorption

Electromagnetic Radiation Electromagnetic Energy: Transmission The propagation of energy through a medium. The wavelengths are refracted when entering or leaving a medium (such as a glass window). Short wavelengths are refracted more than longer wavelengths. Transmission

Interactions of Solar energy with the Earth s surface f i f t f a f r f i f r f t f a Incident energy Reflected energy Transmitted energy Absorbed energy Law of the Conservation of Energy f i = f r f + + t f a

EMR Energy Budget

Transmission Atmospheric Windows Electromagnetic Spectrum Gamma and UV radiation filtered out by the atmosphere Human eye can resolve wavelengths between 0.4 and 0.7 μm, nearly 100% transmission through the atmosphere Photographic film records EM energy within the 0.4-0.9 μm range Wavelength

Atmospheric Scattering Rayleigh (air molecule scattering) -Blue Sky -Blue and Violet wavelengths scattered -Haze -Scattering by smaller particles Mie (aerosol scattering) -Scattering by larger particles -Red and orange wavelengths scattered -Reds and oranges in sunsets Non-selective - Atmospheric and particulate molecule scattering - Larger diameter than the wavelength striking them -Water droplets -Visible to IR equally scattered

Atmospheric Scattering Rayleigh (air molecule scattering) Rayleigh scattering refers to the scattering of light off of the molecules of the air, and can be extended to scattering from particles up to about a tenth of the wavelength of the light.

Atmospheric Scattering Mie (aerosol scattering) For particle sizes larger than a wavelength, Mie scattering predominates. This scattering produces a pattern like an antenna lobe, with a sharper and more intense forward lobe for larger particles.

Atmospheric Scattering Rayleigh and Mie Scattering

O 3 Absorbed Reflected Transmitted Photosynthesis- Leaf Pigments (Chlorophyll a, b, and β-carotene) ABSORB Blue and Red light

Oak InfraRed Pine Concrete G B R

Identify the Spectral Curves Grass Clear Water Fallow Field Sandy Loam Soil Shingles Concrete Artificial Turf Asphalt

Rank these colors from shortest to longest wavelength A. Green B. Purple C. Yellow D. Blue E. Orange Green Purple Yellow Blue Orange

What reflection-type is seen in this oblique satellite image of Australia? A. Specular B. Diffuse 0% 0% Specular Diffuse

What type of scattering is seen closest to the horizon? A. Mie B. Rayleigh C. Nonselective Mie 0% 0% 0% Rayleigh Non-selective

Lecture Outline Electromagnetic Radiation Theory Digital vs. Analog (i.e. film ) Systems

Lecture Outline Electromagnetic Radiation Theory Digital vs. Analog (i.e. film ) Systems

Camera Components A film camera is made of three basic elements: 1. Optical (the lens) 2. Chemical (the film) 3. Mechanical (the camera body)

Camera Components Exposure of film (amount of light that reaches film) is controlled by the f/stop and shutter speed f/stop = f / D

Analog Systems (i.e. film ) Energy Source and Measurement Units Different sensors are required to capture and record the different wavelengths Photographic film is used to capture energy in the 0.4-0.9 μm range Film Types: 1. Black and White - panchromatic (0.4 0.7 μm) - infrared (0.4 0.9 μm) 2. Color - normal color (0.4 0.7 μm) - color infrared (0.4 0.9 μm)

Energy Flow Energy flow within the camera Not all energy that reaches a sensor is recorded by the sensor. Cameras (and other sensors) use film (or CCD s, etc.) that only allow the capture and display of certain wavelengths of energy. Filters can be used to absorb specific quantities and qualities of energy, and affect the type of energy that finally reaches the film.

Camera Filters Filters Absorb unwanted rays of light before they reach the film Antivignetting filters Compensate for unequal light transmission with very wideangle lenses. Designed to allow as much light to the corners of an image as it does the center of the image Polarizing filters Designed to penetrate haze and to reduce reflections from the surfaces of water Haze-cutting filters Designed to remove the blue light in the atmosphere that is scattered by dust, moisture, smoke, or other air pollutants

Film Energy Source and Measurement Units Photographic film is used to capture energy in the 0.4-0.9 μm range Film Types: 1. Black and White - panchromatic (0.4 0.7 μm) - infrared (0.4 0.9 μm) 2. Color - normal color (0.4 0.7 μm) - color infrared (0.4 0.9 μm)

Film Energy Source and Measurement Units Photographic film is used to capture energy in the 0.4-0.9 μm range Film Types: 1. Black and White - panchromatic (0.4 0.7 μm) - infrared (0.4 0.9 μm) 2. Color - normal color (0.4 0.7 μm) - color infrared (0.4 0.9 μm) Blue Green Red IR Reflectance Blue Green Red Black Resulting colors

Film Energy Source and Measurement Units Photographic film is used to capture energy in the 0.4-0.9 μm range Film Types: 1. Black and White - panchromatic (0.4 0.7 μm) - infrared (0.4 0.9 μm) 2. Color - normal color (0.4 0.7 μm) - color infrared (0.4 0.9 μm) Blue Green Red IR Reflectance Black Blue Green Red Resulting colors

Film Comparisons of Film Types Advantages of panchromatic black and white and normal color over infrared: More natural to the eye Better resolution Better penetration of water Advantages of infrared over panchromatic black and white and normal color: Better penetration of haze Emphasizes water and wet areas Good differentiation between hardwood and conifers Good differentiation between healthy and diseased trees

Film Comparisons of Film Types Advantage of normal color over panchromatic black and white: Humans can discriminate 20,000-5 million shades of color, but only about 200 shades of gray. Advantages of panchromatic black and white over normal color: Color film is more expensive to process. Resulting images on color prints are usually not as sharp as on B&W prints.

Digital Systems The Mini-MCA12 System Includes: 12 channel Mini MCA camera 12 ea. 2 GB Certified CF Cards 12 ea. 9.6 mm lenses 12 ea. 1.3 MB image sensors (15.6 MB total) 12 ea. Bandpass Filter Set * - 490FS10-25 - 520FS10-25 - 550FS10-25 - 570FS10-25 - 671FS10-25 - 680FS10-25 - 700FS10-25 - 720FS10-25 - 800FS10-25 - 840FS10-25 - 900FS20-25 - 950FS40-25

Digital Systems Digital Cameras convert analog information (represented by a fluctuating wave) into digital information (represented by ones and zeros, or bits). Benefits of Digital Aerial Imagery Low noise and graininess compared to scanned film Enhanced radiometric resolution, 12 bit vs. 8 bit, for great detail in shadows. Improved tolerance for cloudy or less than ideal weather conditions. No geometric degradation effects related to film warping or distortion. Eliminates cost of film, film development, and digital scanning. Rapid turnaround and delivery, imagery available minutes after landing.