Measure spectral similarity using spectral angle mapper
measures the spectral similarity between the spectra of each pixel in the hyperspectral data
score = sam(
inputData and the specified reference spectra
refSpectra by using the spectral angle mapper (SAM) classification
algorithm. Use this syntax to identify different regions or materials in a hyperspectral
measures the spectral similarity between the specified test spectra
score = sam(
testSpectra and reference spectra
using the SAM classification algorithm. Use this syntax to compare the spectral signature of
an unknown material against the reference spectra or to compute spectral variability between
two spectral signatures.
This function requires the Image Processing Toolbox™ Hyperspectral Imaging Library. You can install the Image Processing Toolbox Hyperspectral Imaging Library from Add-On Explorer. For more information about installing add-ons, see Get and Manage Add-Ons.
Distinguish Hyperspectral Regions Using Spectral Angle Mapper
Distinguish different regions in a hyperspectral data cube by computing the spectral angle distance between each pixel and the endmember spectra of the data cube.
Read hyperspectral data into the workspace.
hcube = hypercube('jasperRidge2_R198.hdr');
Identify the number of spectrally distinct bands in the data cube by using the
numEndmembers = countEndmembersHFC(hcube)
numEndmembers = 13
Extract the endmember spectral signatures from the data cube by using the NFINDR algorithm.
endmembers = nfindr(hcube,numEndmembers);
Plot the spectral signatures of the endmembers. The result shows the 14 spectrally distinct regions in the data cube.
figure plot(endmembers) legend('Location','Bestoutside')
Compute the spectral angular distance between each endmember and the spectrum of each pixel in the data cube.
score = zeros(size(hcube.DataCube,1),size(hcube.DataCube,2),numEndmembers); for i = 1:numEndmembers score(:,:,i) = sam(hcube,endmembers(:,i)); end
Compute the minimum score value from the distance scores obtained for each pixel spectrum with respect to all the endmembers. The index of each minimum score identifies the endmember spectrum to which a pixel spectrum exhibits maximum similarity. An index value, n, at the spatial location (x, y) in the score matrix indicates that the spectral signature of the pixel at spatial location (x, y) in the data cube best matches the spectral signature of the nth endmember.
[~,matchingIndx] = min(score,,3);
Estimate an RGB image of the hyperspectral data cube by using the
colorize function. Display both the RGB image and the matrix of matched index values.
rgbImg = colorize(hcube,'Method','RGB'); figure('Position',[0 0 1100 500]) subplot('Position',[0 0.15 0.4 0.8]) imagesc(rgbImg) axis off title('RGB Image of Hyperspectral Data') subplot('Position',[0.45 0.15 0.4 0.8]) imagesc(matchingIndx) axis off title('Indices of Matching Endmembers') colorbar
Determine Similarity of Endmember Spectra Using SAM
Read hyperspectral data into the workspace.
hcube = hypercube('indian_pines.dat');
Find ten endmembers of the hyperspectral data.
numEndmembers = 10; endmembers = nfindr(hcube,numEndmembers);
Consider the first endmember as the reference spectrum and the rest of the endmembers as the test spectrum. Compute the SAM score between the reference and test spectrum.
score = zeros(1,numEndmembers-1); refSpectrum = endmembers(:,1); for i = 2:numEndmembers testSpectrum = endmembers(:,i); score(i-1) = sam(testSpectrum,refSpectrum); end
Find the test spectrum that exhibit maximum similarity (minimum distance) to the reference spectrum. Then find the test spectrum that exhibit minimum similarity (maximum distance) to the reference spectrum.
[minval,minidx] = min(score); maxMatch = endmembers(:,minidx); [maxval,maxidx] = max(score); minMatch = endmembers(:,maxidx);
Plot the reference spectrum, the maximum similarity and the minimum similarity test spectrum. The test spectrum with the minimum score value indicates highest similarity to the reference endmember. On the other hand, the test spectrum with the maximum score value has the highest spectral variability and characterises the spectral behaviour of two different materials.
figure plot(refSpectrum) hold on plot(maxMatch,'k') plot(minMatch,'r') xlabel('Band Number') ylabel('Data Values') legend('Reference spectrum','Minimum match test spectrum','Maximum match test spectrum',... 'Location','Southoutside') title('Similarity Between Spectra') annotation('textarrow',[0.25 0.25],[0.4 0.5],'String',['Max score: ' num2str(maxval)]) annotation('textarrow',[0.6 0.55],[0.6 0.45],'String',['Min score: ' num2str(minval)])
inputData — Input hyperspectral data
hypercube object | 3-D numeric array
Input hyperspectral data, specified as a
object or a 3-D numeric array containing the data cube. If the input is a
hypercube object, the data is read from the
DataCube property of the object.
testSpectra — Test spectra
Test spectra, specified as a C-element vector. The test spectra is the spectral signature of an unknown region or material.
refSpectra — Reference spectra
Reference spectra, specified as a C-element vector. The reference spectra is the spectral signature of a known region or material. The function matches the test spectra against these values.
score — SAM score
scalar | matrix
SAM score, returned as a scalar or matrix. The output is a
scalar — If you specify the
testSpectrainput argument. The function matches the test spectral signature against the reference spectral signature and returns a scalar value. Both the test and the reference spectra must be vectors of same length.
matrix — If you specify the
inputDatainput argument. The function matches the spectral signature of each pixel in the data cube against the reference spectral signature and returns a matrix. If the data cube is of size M-by-N-by-C and the reference spectra is a vector of length C, the output matrix is of size M-by-N.
Each element of the SAM score is a spectral angle in radians in the range [0, 3.142]. A smaller SAM score indicates a strong match between the test signature and the reference signature.
Spectral angle mapper
Given the test spectra t and a reference spectra r of length C, the SAM score α is calculated as
 Kruse, F.A., A.B. Lefkoff, J.W. Boardman, K.B. Heidebrecht, A.T. Shapiro, P.J. Barloon, and A.F.H. Goetz. “The Spectral Image Processing System (SIPS)—Interactive Visualization and Analysis of Imaging Spectrometer Data.” Remote Sensing of Environment 44, no. 2–3 (May 1993): 145–63. https://doi.org/10.1016/0034-4257(93)90013-N.
Introduced in R2020a