Environmental Remote Sensing: Fundamentals, Radiation, Spectral Signatures, and Image Processing

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Description and Tags

Comprehensive vocabulary flashcards covering the core concepts of environmental remote sensing: electromagnetic radiation principles, spectral signatures, digital data formats, image enhancement, and geometric correction.

55 Terms

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Remote Sensing

The science and art of deriving information about the Earth's land and water surfaces without touching them, using images acquired from an overhead perspective via electromagnetic radiation reflected or emitted from the Earth's surface.

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Spatial Resolution

A measure of the smallest ground area that can be separately recorded or resolved by a remote sensor, typically defined by the instantaneous field of view and the pixel dimension (e.g., 10×10 m10 \times 10\,\text{m}).

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Spectral Resolution

The specific wavelength interval or width across the electromagnetic spectrum that a remote sensing instrument detects, along with the number of discrete spectral bands it records.

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Radiometric Resolution

The sensitivity of a remote sensing detector to differences in signal strength, determined by the number of discrete quantization levels (bit depth) used to record brightness values (e.g., 8-bit records 28=2562^8 = 256 levels, from 0 to 255).

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Temporal Resolution

The revisit schedule or time interval between successive image acquisitions over the exact same geographic area by a satellite sensor platform (e.g., 16 days for Landsat).

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<p>AVIRIS Datacube</p>

AVIRIS Datacube

A 3-dimensional dataset produced by the Airborne Visible Infrared Imaging Spectrometer consisting of contiguous two-dimensional spatial coordinate layers recorded across 224 spectral bands with a 10 nm10\,\text{nm} nominal bandwidth from 400 nm400\,\text{nm} to 2500 nm2500\,\text{nm}.

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<p>Electromagnetic Radiation (EMR)</p>

Electromagnetic Radiation (EMR)

A dynamic form of energy that exhibits both wave and particle properties, propagating through space at the speed of light (c≈3×108 m/sc \approx 3 \times 10^8\,\text{m/s}) as mutually perpendicular oscillating electric and magnetic fields.

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Wave Equation of EMR

The fundamental mathematical expression relating the speed of light (cc), wavelength (λ\lambda), and frequency (ν\nu): c=λνc = \lambda \nu, demonstrating that wavelength and frequency are inversely related.

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Radiant Energy

The total capacity to do work emitted, transferred, or received in the form of electromagnetic waves, quantified in Joules (J\text{J}).

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Radiant Flux

The rate at which radiant energy passes through or is emitted from a surface per unit time, quantified in Joules per second (J/s\text{J/s}) or Watts (W\text{W}).

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Irradiance

The radiant flux density incident onto a flat surface from all hemispherical directions per unit surface area, quantified in W m−2\text{W}\,\text{m}^{-2} or J/(m2⋅s)\text{J}/(\text{m}^2 \cdot \text{s}).

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Exitance

The radiant flux density leaving or emitted from a flat surface in all directions per unit surface area, quantified in W m−2\text{W}\,\text{m}^{-2} or J/(m2⋅s)\text{J}/(\text{m}^2 \cdot \text{s}).

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Radiance

The radiant flux density emitted, reflected, or transmitted from a surface per unit projected area per unit solid angle in a specified direction, quantified in W/(m2⋅sr)\text{W}/(\text{m}^2 \cdot \text{sr}).

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<p>Steradian</p>

Steradian

The standard unit of solid angle in three dimensions, defined as the central angle subtended at the center of a sphere by an area on the surface equal to the square of the radius (r2r^2); the entire sphere subtends 4π steradians4\pi\,\text{steradians}.

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Radiant Energy Conservation Law

The principle stating that all incident radiant energy must be absorbed, reflected, or transmitted: α+ρ+τ=1\alpha + \rho + \tau = 1, where α\alpha is absorptivity, ρ\rho is reflectivity, and τ\tau is transmissivity.

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Blackbody

An idealized physical body that absorbs 100% of incident electromagnetic radiation at all wavelengths (α=1\alpha = 1) and re-emits the maximum possible thermal radiation for an object at that temperature.

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Wien's Displacement Law

A radiation law defining the inverse relationship between blackbody temperature (TT in Kelvin) and the peak emission wavelength (λmax⁡\lambda_{\max}): λmax⁡=2897.8T\lambda_{\max} = \frac{2897.8}{T}, showing that hotter objects peak at shorter wavelengths.

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Stefan-Boltzmann Law

A physical law stating that total radiant exitance (WW) from a blackbody is directly proportional to the fourth power of its absolute temperature: W=σT4W = \sigma T^4, where σ=5.6697×10−8 W m−2 K−4\sigma = 5.6697 \times 10^{-8}\,\text{W}\,\text{m}^{-2}\,\text{K}^{-4}.

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Emissivity (ε\varepsilon)

The ratio of the radiant exitance (MM) emitted by a real object (greybody) to that emitted by a perfect blackbody (MbM_b) at the identical kinetic temperature, expressed as ε=MMb\varepsilon = \frac{M}{M_b} with values ranging from 0 to 1.

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Cosine's Law of Illumination

The geometric relationship determining solar irradiance on a surface based on incoming solar beam irradiance (EinE_{\text{in}}) and solar zenith angle (θ\theta): Es=Eincos⁡(θ)E_s = E_{\text{in}} \cos(\theta).

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Rayleigh Scattering

Atmospheric scattering that occurs when particle diameters (such as N2N_2 and O2O_2 molecules) are much smaller than the radiation wavelength, where scattering intensity is inversely proportional to the fourth power of wavelength (∝λ−4\propto \lambda^{-4}).

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Mie Scattering

Atmospheric scattering occurring when particle diameters (such as smoke, dust, and pollen) are roughly equal to the wavelength of radiation, exhibiting a weak wavelength dependence.

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Nonselective Scattering

Atmospheric scattering caused by particles (such as water droplets and large airborne dust) that are much larger than the incident radiation wavelength, scattering all wavelengths equally and appearing white or light grey.

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Atmospheric Windows

Spectral regions of the electromagnetic spectrum where the atmosphere absorbs little to no radiation, allowing transmitted radiant energy to pass freely between the ground and airborne or spaceborne sensors.

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Lambertian Surface

An ideal perfectly diffuse reflecting surface that scatters incident light equally in all directions, yielding uniform radiance (RR) irrespective of viewing angle according to the relation I=πRI = \pi R.

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Bidirectional Reflectance Distribution Function (BRDF)

A mathematical formulation describing how surface reflectance varies with both illumination angle (solar zenith and azimuth) and viewing geometry (sensor zenith and azimuth), largely influenced by canopy architecture and shadowing.

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Spectral Reflectance

The ratio of reflected radiant energy to total incoming incident energy measured as a function of specific wavelength intervals across the electromagnetic spectrum.

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Albedo

The total hemispherical reflectivity of a surface calculated across the broad shortwave solar spectrum ranging from 0.3 μm0.3\,\mu\text{m} to 4.0 μm4.0\,\mu\text{m}.

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Vegetation Spectral Signature

The characteristic reflectance curve of healthy green vegetation, governed by photosynthetic pigments in the visible spectrum (380–720 nm380\text{–}720\,\text{nm}), spongy mesophyll cell structure in the near-infrared (720–1300 nm720\text{–}1300\,\text{nm}), and water absorption in the mid-infrared (1300–2500 nm1300\text{–}2500\,\text{nm}).

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Thermal Diurnal Signature

The characteristic daily cycle of radiant temperature variation of surface materials, in which water bodies maintain relatively stable temperatures due to high thermal capacity while dry soils, rocks, and sands fluctuate sharply between day and night.

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Active vs. Passive Sensors

Passive sensors record natural electromagnetic radiation emitted or reflected from terrestrial targets (e.g., optical scanners), whereas active sensors emit their own electromagnetic pulses and measure the backscattered return signal (e.g., RADAR and LiDAR).

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Landsat TM Band 1

The blue-green spectral band (0.45–0.52 μm0.45\text{–}0.52\,\mu\text{m}) on Landsat Thematic Mapper designed for water body penetration, coastal mapping, and discriminating soil from vegetation.

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Landsat TM Band 4

The near-infrared band (0.76–0.90 μm0.76\text{–}0.90\,\mu\text{m}) on Landsat Thematic Mapper responsive to leaf cellular structure, used to determine vegetation biomass, health, and water-land interfaces.

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Landsat TM Band 5

The mid-infrared band (1.55–1.75 μm1.55\text{–}1.75\,\mu\text{m}) on Landsat Thematic Mapper sensitive to vegetation moisture, soil moisture, and effective at discriminating between clouds and snow.

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Landsat TM Band 6

The thermal infrared channel (10.4–12.5 μm10.4\text{–}12.5\,\mu\text{m}) on Landsat Thematic Mapper measuring surface brightness temperature, vegetation stress, and thermal urban heat patterns.

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Digital Number (DN)

An integer value assigned to an individual image pixel that quantifies the intensity of detected electromagnetic radiation within a given band, typically scaled to bit ranges such as 0 to 255 (8-bit).

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ASCII File Format

A text-based data format where every character, decimal digit, delimiter, or space consumes 1 byte of storage, commonly used to record human-readable imagery metadata headers.

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Binary File Format

A compact numerical file structure that stores raw byte values directly without conversion to ASCII text, enabling smaller memory consumption and faster input/output operations.

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<p>Multispectral Storage Formats (BSQ, BIL, BIP)</p>

Multispectral Storage Formats (BSQ, BIL, BIP)

Three distinct methods to organize multi-band raster data: Band Sequential (BSQ) writes complete single bands sequentially, Band Interleaved by Line (BIL) stores scans line-by-line across all bands, and Band Interleaved by Pixel (BIP) stores spectral channel values pixel-by-pixel.

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Image Histogram

A graphic frequency distribution plot displaying the total number of pixels or percentage frequency occurring at each discrete digital number value within a single band of imagery.

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Min-Max Linear Contrast Stretch

A radiometric enhancement method that linearly expands the original narrow range of digital numbers to use the full display display range (0–2550\text{–}255 for 8-bit) using: Screen DN=pixel DN−DNmin⁡DNmax⁡−DNmin⁡×255\text{Screen DN} = \frac{\text{pixel DN} - \text{DN}_{\min}}{\text{DN}_{\max} - \text{DN}_{\min}} \times 255.

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Histogram Equalization

A nonlinear contrast enhancement technique that redistributes pixel brightness values to create a uniform, flattened histogram, allocating maximum visual contrast to the most frequently occurring digital numbers.

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Directional First Differencing

A spatial filtering technique for edge enhancement that computes the difference between adjacent pixel values horizontally (DNA−DNH\text{DN}_A - \text{DN}_H), vertically (DNA−DNV\text{DN}_A - \text{DN}_V), or diagonally, commonly offset by adding 127 for 8-bit display.

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Geometric Correction

The preprocessing operation that removes geometric distortions caused by sensor motion, platform velocity/altitude variations, Earth rotation, and curvature to register the image to a defined coordinate space.

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Nonsystematic Image Distortions

Random, unpredictable geometric errors induced by external factors during data acquisition, including variations in platform altitude, spacecraft velocity, Earth rotation, and attitude instabilities (roll, pitch, yaw).

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Systematic Image Distortions

Predictable geometric aberrations caused by internal sensor scanning mechanics, such as scan skew, cross-track scale variation, and scan mirror velocity variation, which can be corrected using known optical formulas.

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Ground Control Point (GCP)

A distinct, recognizable geographic feature with known map or GPS coordinates (such as road intersections or sharp water-body boundaries) used to geometrically align and register unrectified imagery.

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Root Mean Square Error (RMSE)

A quantitative statistical metric measuring the magnitude of residual positioning error between estimated transformed ground control point coordinates and their true map coordinates.

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Polynomial Order GCP Requirements

The mathematical threshold defining the minimum number of GCPs required to compute coordinate transformation models: 3 GCPs for 1st-order, 6 GCPs for 2nd-order, and 10 GCPs for 3rd-order transformations.

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<p>Nearest Neighbour Resampling</p>

Nearest Neighbour Resampling

A spatial resampling method that assigns the digital number of the closest input pixel directly to the transformed output grid location, preserving original radiometric values without smoothing.

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<p>Bilinear Interpolation Resampling</p>

Bilinear Interpolation Resampling

A resampling technique that calculates the output pixel value using a distance-weighted average of the four nearest surrounding input pixels, producing a smoothed appearance.

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<p>Cubic Convolution Resampling</p>

Cubic Convolution Resampling

The most widely used advanced resampling method that calculates output brightness values by computing a distance-weighted average of the surrounding 4×44 \times 4 (16 total) input pixels.

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Lambert Conformal Conic (LCC)

A conic map projection used widely for mid-latitude countries like Canada, using standard parallels at 49∘ N49^\circ\,\text{N} and 77∘ N77^\circ\,\text{N} and a central meridian at 95∘ W95^\circ\,\text{W}.

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<p>Mercator Projections</p>

Mercator Projections

A family of conformal cylindrical projections including standard Mercator (accurate east-west), Transverse Mercator (accurate along a north-south meridian), and Oblique Mercator (aligned along a satellite ground track).

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Universal Transverse Mercator (UTM)

A global standardized grid coordinate system dividing the Earth into 60 zones of 6∘6^\circ longitudinal width, spanning from latitude 84∘ N84^\circ\,\text{N} to 80∘ S80^\circ\,\text{S}, where Zone 1 begins at 180∘–174∘ W180^\circ\text{–}174^\circ\,\text{W}.