Tutorial
About Hyperspectral Remote Sensing Data
Authors: Leah A. Wasser
Last Updated: Sep 27, 2023
Learning Objectives
After completing this tutorial, you will be able to:
- Define hyperspectral remote sensing.
- Explain the fundamental principles of hyperspectral remote sensing data.
- Describe the key attributes that are required to effectively work with hyperspectral remote sensing data in tools like R or Python.
- Describe what a "band" is.
Mapping the Invisible
About Hyperspectral Remote Sensing Data
The electromagnetic spectrum is composed of thousands of bands representing different types of light energy. Imaging spectrometers (instruments that collect hyperspectral data) break the electromagnetic spectrum into groups of bands that support classification of objects by their spectral properties on the earth's surface. Hyperspectral data consists of many bands -- up to hundreds of bands -- that cover the electromagnetic spectrum.
The NEON imaging spectrometer collects data within the 380nm to 2510nm portions of the electromagnetic spectrum within bands that are approximately 5nm in width. This results in a hyperspectral data cube that contains approximately 426 bands - which means big, big data.
Key Metadata for Hyperspectral Data
Bands and Wavelengths
A band represents a group of wavelengths. For example, the wavelength values between 695nm and 700nm might be one band as captured by an imaging spectrometer. The imaging spectrometer collects reflected light energy in a pixel for light in that band. Often when you work with a multi or hyperspectral dataset, the band information is reported as the center wavelength value. This value represents the center point value of the wavelengths represented in that band. Thus in a band spanning 695-700 nm, the center would be 697.5).

Spectral Resolution
The spectral resolution of a dataset that has more than one band, refers to the width of each band in the dataset. In the example above, a band was defined as spanning 695-700nm. The width or spatial resolution of the band is thus 5 nanometers. To see an example of this, check out the band widths for the Landsat sensors.
Full Width Half Max (FWHM)
The full width half max (FWHM) will also often be reported in a multi or hyperspectral dataset. This value represents the spread of the band around that center point.

In the illustration above, the band that covers 695-700nm has a FWHM of 5 nm. While a general spectral resolution of the sensor is often provided, not all sensors create bands of uniform widths. For instance bands 1-9 of Landsat 8 are listed below (Courtesy of USGS)
Band | Wavelength range (microns) | Spatial Resolution (m) | Spectral Width (microns) |
---|---|---|---|
Band 1 - Coastal aerosol | 0.43 - 0.45 | 30 | 0.02 |
Band 2 - Blue | 0.45 - 0.51 | 30 | 0.06 |
Band 3 - Green | 0.53 - 0.59 | 30 | 0.06 |
Band 4 - Red | 0.64 - 0.67 | 30 | 0.03 |
Band 5 - Near Infrared (NIR) | 0.85 - 0.88 | 30 | 0.03 |
Band 6 - SWIR 1 | 1.57 - 1.65 | 30 | 0.08 |
Band 7 - SWIR 2 | 2.11 - 2.29 | 30 | 0.18 |
Band 8 - Panchromatic | 0.50 - 0.68 | 15 | 0.18 |
Band 9 - Cirrus | 1.36 - 1.38 | 30 | 0.02 |
Explore Related Data Products
These data products are used in this tutorial: