Skip to main content

Hybrid classification and Post-classification smoothing


Hybrid classification is a combined classification approach that uses both supervised and unsupervised classification techniques together.
It is designed to take advantage of the strengths of each method and to overcome their weaknesses.

What Is Hybrid Classification?

Hybrid classification blends:

  • Unsupervised classification (e.g., ISODATA, K-means)

  • Supervised classification (e.g., Maximum Likelihood, SVM)

✔ Concept

  1. First, an unsupervised algorithm groups pixels into spectral clusters without prior knowledge.

  2. These clusters are then labeled or merged into meaningful land-cover classes using supervised training data.

✔ Why use hybrid methods?

  • Unsupervised classification captures natural spectral groupings.

  • Supervised classification improves accuracy by using reference samples.

  • Together, they reduce errors caused by poor training data or complex landscapes.

✔ Key Terminology

  • Cluster: a group of pixels with similar spectral characteristics.

  • Signature training: giving labels to clusters.

  • Spectral homogeneity: similarity within a cluster.

  • Class merging: combining multiple clusters into one land-cover type.

Hybrid Classification

Step 1: Unsupervised Clustering

Algorithms like ISODATA or K-means group pixels into 20–50 clusters based only on spectral properties.

Step 2: Assign Clusters to Land-Cover Classes

Use training samples, field data, or expert knowledge to assign each cluster to:

  • water

  • forest

  • agriculture

  • built-up

  • soil
    (or other classes)

Step 3: Supervised Refinement

Run a supervised classifier (e.g., Maximum Likelihood) using the cluster-based signatures.

Step 4: Merge & Edit Classes

Check for:

  • confused clusters

  • isolated patches

  • mixed clusters
    Clusters are merged or adjusted.

Step 5: Final classified image

A clean, corrected classification map is produced.

Advantages of Hybrid Classification

  • Improves accuracy in heterogeneous landscapes

  • Handles mixed pixels better

  • Reduces reliance on perfect training samples

  • Captures subtle spectral differences

  • Reduces spectral confusion between similar classes

✔ Suitable for:

  • complex landscapes

  • urban environments

  • vegetation mosaics

  • large areas with limited training data

Limitations

  • More interactive and time-consuming

  • Requires expertise for cluster labeling

  • Too many clusters can make interpretation difficult

Post-Classification Smoothing

After classification, the resulting land-cover map often has:

  • salt-and-pepper noise

  • scattered small patches

  • isolated mislabeled pixels

Post-classification smoothing removes these artifacts to produce a cleaner, generalized map.

What Is Post-Classification Smoothing?

It is the process of cleaning and refining a classified image by applying spatial filters or majority rules to reduce noise and improve map readability.

✔ Why smoothing is needed?

Because pixel-based classifiers classify each pixel individually, ignoring spatial relationships.
This results in:

  • random noisy pixels

  • speckled appearances

  • unrealistic boundaries

Smoothing creates spatially coherent regions.

Common Smoothing Techniques

A. Majority (Mode) Filter

  • A moving window (3×3, 5×5) scans the classified image.

  • Each pixel is replaced by the most common class in the window.

  • Removes small patches and isolated noise.

B. Median Filter

  • Similar to majority filter but uses median instead of majority.

  • Preserves edges better.

C. Morphological Operations

  • Opening: removes small isolated pixels.

  • Closing: fills gaps in homogeneous regions.

D. Region Growing

  • Groups contiguous pixels belonging to the same class into larger coherent regions.

E. Elimination of Small Patches

  • Removes polygons smaller than a defined threshold (e.g., <1 hectare).

Results of Smoothing

  • More realistic class shapes

  • Reduced classification noise

  • Better readability for maps

  • Improved accuracy for urban and natural landscapes

  • Cleaner boundaries between classes


Comments

Popular posts from this blog

Thermal Infrared Remote Sensing

1. Principles Thermal Infrared Remote Sensing is based on the detection of naturally emitted electromagnetic radiation from objects, rather than reflected solar energy. According to Planck's Radiation Law , all objects with a temperature above absolute zero (0 K) emit electromagnetic radiation. For Earth surface features, the peak emission lies in the Thermal Infrared (TIR) region of 3–14 μm of the electromagnetic spectrum. The amount of radiation emitted is primarily a function of surface temperature and emissivity . Sensors measure the radiant energy flux density (W/m²) , which is later converted to surface temperature using Stefan-Boltzmann's Law . 2. Radiation Properties in TIR Emissivity (ε): Ratio of radiation emitted by a surface to that emitted by a perfect blackbody at the same temperature. Natural surfaces like water (ε ≈ 0.98) have high emissivity, while bare soils and metals have lower values. Blackbody: An idealized object th...

Atmospheric Window

The atmospheric window in remote sensing refers to specific wavelength ranges within the electromagnetic spectrum that can pass through the Earth's atmosphere relatively unimpeded. These windows are crucial for remote sensing applications because they allow us to observe the Earth's surface and atmosphere without significant interference from the atmosphere's constituents. Key facts and concepts about atmospheric windows: Visible and Near-Infrared (VNIR) window: This window encompasses wavelengths from approximately 0. 4 to 1. 0 micrometers. It is ideal for observing vegetation, water bodies, and land cover types. Shortwave Infrared (SWIR) window: This window covers wavelengths from approximately 1. 0 to 3. 0 micrometers. It is particularly useful for detecting minerals, water content, and vegetation health. Mid-Infrared (MIR) window: This window spans wavelengths from approximately 3. 0 to 8. 0 micrometers. It is valuable for identifying various materials, incl...

Radar Remote Sensing SAR

1. Radar and Radar Remote Sensing RADAR stands for Radio Detection and Ranging . It is an active remote sensing system that transmits microwave energy toward the Earth's surface and records the energy that is returned to the sensor as an echo or backscatter . Unlike passive optical remote sensing, radar does not depend on sunlight. Therefore, it can operate day and night and, at suitable wavelengths, can acquire data through clouds, haze and light rain. Hence, radar is widely described as an all-weather, day-and-night remote sensing technology . Basic principle Microwave pulse → transmission → interaction with surface → backscatter/echo → antenna receives signal → signal processing → radar image 2. Microwave Energy Radar systems use microwave electromagnetic radiation , generally in wavelength ranges from approximately 1 mm to 1 m . Important radar bands include: Band Approx. wavelength Common applications ...

Radar image. Polarization in Remote Sensing

L band radars operate on a wavelength of 15-30 cm and a frequency of 1-2 GHz. L band radars are mostly used for clear air turbulence studies. S band radars operate on a wavelength of 8-15 cm and a frequency of 2-4 GHz. Because of the wavelength and frequency, S band radars are not easily attenuated. . Polarization refers to the direction of travel of an electromagnetic wave vector's tip: vertical (up and down), horizontal (left to right), or  circular (rotating in a constant plane left or right). . a synthetic aperture radar (SAR) for high-resolution imaging. a radar altimeter, to measure the ocean topography. echo amplitude a wind scatterometer to measure wind speed and direction. Other types of radars have been flown for Earth observation missions: precipitation radars such as the  Tropical Rainfall Measuring Mission, or cloud radars like the one used on Cloudsat. . RISAT-1 (SAR, ISRO India, 2012) RORSAT (SAR, Soviet Union, 1967-1988) Seasat (SAR, altimeter, scatterometer, US, 19...

Discrete Detectors and Scanning mirrors Across the track scanner Whisk broom scanner.

Multispectral Imaging Using Discrete Detectors and Scanning Mirrors (Across-Track Scanner or Whisk Broom Scanner) Multispectral Imaging:  This technique involves capturing images of the Earth's surface using multiple sensors that are sensitive to different wavelengths of electromagnetic radiation.  This allows for the identification of various features and materials based on their spectral signatures. Discrete Detectors:  These are individual sensors that are arranged in a linear or array configuration.  Each detector is responsible for measuring the radiation within a specific wavelength band. Scanning Mirrors:  These are optical components that are used to deflect the incoming radiation onto the discrete detectors.  By moving the mirrors,  the sensor can scan across the scene,  capturing data from different points. Across-Track Scanner or Whisk Broom Scanner:  This refers to the scanning mechanism where the mirror moves perpendicular to the direction of flight.  This allows for t...