Hyperspectral payloads course
Online course of 300 hours in hyperspectral payloads, structured in 6 modules covering imaging spectroscopy, spectrometer architecture, calibration and pre-processing, hyperspectral data analysis, thematic applications and a final project, with an assigned technical tutor.
Take the controls.
Run a real engineering trade-off from this field. Move the sliders, watch the model react in real time and beat the challenge.
What you will be able to do
Understand the fundamentals of imaging spectroscopy.
Analyse the architectures of space spectrometers.
Apply calibration and atmospheric correction to hyperspectral data.
Use spectral analysis and unmixing techniques.
Assess thematic applications of hyperspectral data.
Design the processing chain of a mission.
Produce the preliminary design of a hyperspectral payload.
Who it's for
- Hyperspectral remote sensing specialists.
- Payload engineers working on imaging spectrometers.
- Geospatial data scientists.
- Calibration engineers.
- Remote sensing geologists.
- Optical engineers moving into spectral instruments.
- Engineering or science graduates aiming to enter Earth observation.
What you'll work with
- CCSDS 123.0-B (low-complexity lossless and near-lossless multispectral and hyperspectral image compression)
- CEOS-ARD Surface Reflectance (analysis ready data specification for surface reflectance)
- ISO 19159-1 (calibration and validation of remote sensing imagery sensors: optical sensors)
- ISO 19115-2 (geographic information metadata for imagery and gridded data)
- ECSS-Q-ST-70-01C (cleanliness and contamination control)
- ISO 19130-1 (imagery sensor models for geopositioning)
- ENVI
- EnMAP-Box
- Spectral Python (SPy)
- MODTRAN
- Zemax OpticStudio
6 modules
1.1Spectral signature of materials1.2Differences between multispectral and hyperspectral1.3VNIR and SWIR range1.4Spectral resolution and sampling1.5The hyperspectral cube1.6Characteristic absorption features1.7EnMAP, PRISMA and CHIME missions1.8Main applications1.9Spatial versus spectral resolution1.10Workshop: analysis of spectral signatures of minerals
2.1Grating and prism spectrometers2.2Offner and Dyson configurations2.3Fourier transform spectrometers2.4Linear variable filters2.5HgCdTe detectors for SWIR2.6Smile and keystone2.7Spectral signal-to-noise ratio2.8Data volume and compression2.9On-board calibration with solar diffusers2.10Practical exercise: SNR calculation for a SWIR spectrometer
3.1Spectral calibration3.2Radiometric calibration3.3Correction of bad bands3.4Atmospheric correction with radiative transfer3.5Surface reflectance3.6Geometric correction3.7Noise reduction3.8Level 2 products3.9Smile effect correction3.10Lab: atmospheric correction with MODTRAN
4.1Dimensionality reduction: PCA and MNF4.2Spectral angle mapper (SAM)4.3Linear spectral unmixing4.4Endmember extraction4.5Specific spectral indices4.6Supervised classification4.7Deep learning for data cubes4.8USGS and ECOSTRESS spectral libraries4.9Classification quality indices4.10Case study: spectral unmixing of a PRISMA scene
5.1Geology and mining5.2Agriculture and vegetation stress5.3Water quality5.4Methane detection5.5Biodiversity5.6Soils and degradation5.7Environmental monitoring5.8Fusion with multispectral data5.9Products and distribution platforms5.10Case study: mineral mapping with EnMAP data
6.1Scientific requirements6.2Spectral range selection6.3Spectrometer design6.4SNR budget6.5Calibration plan6.6Processing chain6.7Analysis algorithms6.8Validation with real data6.9Report and presentation6.10Final project: final review with the tutor
How you'll learn
100% online training on the SEIUM campus, with downloadable material, recorded classes and an assigned technical tutor. There are no fixed timetables: you progress at your own pace within the intake, so the programme can be combined with work.
Each module combines theory, guided reading of the original standard and applied exercises. The working software is ENVI, EnMAP-Box, Spectral Python (SPy), MODTRAN and Zemax OpticStudio, in free, academic or evaluation versions. Testing is studied through real procedures: spectral unmixing of a hyperspectral scene, atmospheric correction with radiative transfer models and design of an Offner-type spectrometer. Assessment is continuous by module, plus the final integrating project.
Standards covered: CCSDS 123.0-B, CEOS-ARD Surface Reflectance, ISO 19159-1, ISO 19115-2, ECSS-Q-ST-70-01C, ISO 19130-1.
Build it end to end
Your final project follows the real engineering workflow, step by step, reviewed by your tutor.
Where this takes you
Requirements
- No prior qualification is required.
- Internet connection and a computer capable of running the programme software.
- English sufficient to read technical standards.
Ready to start?
Send your application today. Our admissions team replies within 72 hours with your study plan and funding options.
Frequently asked questions
The programme totals 300 hours over 3 months. You set your own pace within each intake, and your tutor helps you plan the workload around your job.
You work with ENVI, EnMAP-Box, Spectral Python (SPy), MODTRAN, Zemax OpticStudio, using free, academic or evaluation versions. Your tutor indicates the free alternative wherever one exists.
A SEIUM Institute certificate, awarded on passing the continuous assessment and the final project. It is SEIUM's own qualification, not an official state degree; its recognition depends on the programme completed and the regulations of each country.
Yes. Modules passed are recognised in a higher programme in the same area (postgraduate diploma or master's). Ask about the recognition policy when you enrol.
No prior qualification is required; you need an internet connection, a computer able to run the programme software and English sufficient to read technical standards.
Start dates are set by SEIUM's faculty for each intake. Our admissions team will confirm the next available date when you apply.
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