Master’s in SAR/Optical/Hyperspectral Payloads Engineering
Online master's programme of 1,900 hours in SAR, optical and hyperspectral payload engineering: 12 modules covering remote sensing fundamentals, optical, infrared and hyperspectral instruments, SAR fundamentals and payload design, SAR and optical image processing, on-board processing, calibration and validation, and applications, with an assigned technical tutor.
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What you will be able to do
Understand the fundamentals of space remote sensing.
Design optical and infrared instruments.
Analyse hyperspectral spectrometers.
Design SAR payloads.
Process SAR, optical and hyperspectral images.
Plan instrument calibration and validation.
Develop Earth observation applications and services.
Who it's for
- Payload engineers who want to cover optical, hyperspectral and SAR instruments in one programme.
- Optical instrument engineers designing telescopes and focal planes.
- SAR radar engineers working on payload design or processing.
- Remote sensing specialists who want to understand the instrument behind the data.
- Image processing engineers working with Sentinel and commercial data.
- Calibration and validation engineers responsible for product quality.
- Engineering or science graduates aiming to enter the space sector.
What you'll work with
- ECSS-E-ST-10C (system engineering general requirements)
- ECSS-E-ST-10-03C (testing)
- CCSDS 123.0-B-2 (low-complexity lossless and near-lossless multispectral and hyperspectral image compression)
- CCSDS 121.0-B-3 (lossless data compression)
- ISO 19115-2 (geographic information metadata for imagery and gridded data)
- ISO 19159-1 (calibration and validation of remote sensing imagery sensors)
- CEOS Analysis Ready Data for Land (ARD specifications for land products)
- Regulation (EU) 2021/696 (Union Space Programme)
- ESA SNAP
- ENVI
- Zemax OpticStudio
- MATLAB
- Google Earth Engine
12 modules · 1900 h
1.1Electromagnetic spectrum and atmospheric windows1.2Interaction of radiation with surfaces1.3Spatial, spectral, radiometric and temporal resolution1.4Passive versus active sensors1.5Pushbroom and whiskbroom acquisition geometry1.6Earth observation orbits1.7The Copernicus programme and Sentinel missions1.8Product processing levels1.9Commercial observation market1.10Case study: user requirements for agricultural monitoring
2.1Cassegrain and Korsch reflecting telescopes2.2Optical quality and the modulation transfer function2.3Instrument signal-to-noise ratio2.4CCD and CMOS TDI detectors2.5Focal planes and filters2.6Thermal and structural stability2.7On-board radiometric calibration2.8Design of optical payloads for small satellites2.9Very high resolution and its diffraction limit2.10Lab: MTF and SNR calculation for a camera
3.1VNIR, SWIR, MWIR and TIR bands3.2HgCdTe and InGaAs detectors3.3Cryocoolers for detectors3.4MSI-type multispectral instruments3.5Brightness temperature and emissivity3.6Calibration with black bodies3.7Thermal wildfire monitoring applications3.8Atmospheric sounding instruments3.9Noise and NETD3.10Practical exercise: radiometric budget of a thermal channel
4.1Grating and prism spectrometers4.2Offner and Dyson spectrometers4.3Fourier transform spectral imaging4.4EnMAP, PRISMA and CHIME missions4.5Spectral resolution and SNR4.6Spectral calibration and smile4.7Data volume and compression4.8Applications in mining and vegetation4.9Hyperspectral imaging on small satellites4.10Lab: analysis of a PRISMA hyperspectral cube
5.1The radar equation5.2Range resolution and pulse compression5.3Synthetic aperture and azimuth resolution5.4X, C, L and P bands5.5Stripmap, ScanSAR and spotlight modes5.6Ambiguities and PRF5.7Speckle and radar statistics5.8Slant geometry: layover and shadow5.9SAR polarimetry and decompositions5.10Practical exercise: parameter design for an X-band SAR
6.1Active aperture antennas and reflectors6.2Solid-state transmit-receive modules6.3Chirp generation and digitisation6.4Power and thermal budget6.5SAR on microsatellites6.6Commercial SAR constellations6.7Internal and external calibration6.8System NESZ sensitivity6.9Data volume and downlink6.10Case study: sizing a SAR for a microsatellite
7.1Range-Doppler focusing algorithm7.2Chirp scaling and omega-k algorithms7.3Focusing and autofocus7.4Radiometric calibration of SAR images7.5Geometric correction and orthorectification7.6InSAR interferometry and digital models7.7Differential interferometry and deformation7.8Coherence and change detection7.9ESA's SNAP tool7.10Lab: interferogram with Sentinel-1 data
8.1Atmospheric correction of optical images8.2Orthorectification and RPC models8.3Pansharpening band fusion8.4Calculation of spectral indices8.5Linear spectral unmixing8.6Supervised land cover classification8.7Deep learning on satellite imagery8.8Multitemporal change detection8.9Cloud processing8.10Practical exercise: land cover classification with Sentinel-2
9.1On-board processing architecture9.2CCSDS 121 and 123 compression9.3On-board mass memory9.4On-board artificial intelligence9.5Cloud-free scene selection9.6X- and Ka-band downlinks9.7Optical data links9.8Product latency9.9Ground processing chains9.10Workshop: data budget for a hyperspectral mission
10.1Pre-launch laboratory calibration10.2In-flight calibration10.3Vicarious calibration sites10.4Corner reflectors for SAR10.5Product validation10.6Inter-calibration between sensors10.7CEOS calibration standards10.8Metrological traceability of measurements10.9Degradation monitoring10.10Case study: cal/val plan for an optical instrument
11.1Agriculture and food security11.2Emergency management11.3Ground deformation monitoring11.4Maritime surveillance and ship detection11.5Climate change and the cryosphere11.6Urban planning and urban growth11.7Water resource management11.8Insurance and finance11.9Operational Copernicus services11.10Practical exercise: subsidence monitoring service
12.1User and mission requirements12.2Selection of sensor type12.3Payload design12.4Instrument radiometric budgets12.5Platform and orbit12.6Processing chain12.7Calibration and validation plan12.8Demonstrator application with real data12.9Master's Thesis: written report12.10Master's Thesis: defence before a panel
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 each intake, so it fits around your job.
Each module combines theory, guided reading of the original standard and applied exercises. The working software is ESA SNAP, ENVI, Zemax OpticStudio, MATLAB and Google Earth Engine, in free, academic or evaluation versions. Testing is studied through real procedures for Sentinel-1 SAR data processing, hyperspectral cube analysis and instrument radiometric budgets. Assessment is continuous by module, plus the final Master's Thesis.
Standards covered: ECSS-E-ST-10C, ECSS-E-ST-10-03C, CCSDS 123.0-B-2, CCSDS 121.0-B-3, ISO 19115-2, ISO 19159-1, CEOS Analysis Ready Data for Land, Regulation (EU) 2021/696.
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
- A university degree in engineering, science or architecture, or equivalent demonstrable professional experience.
- An 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 1,900 hours over 12–14 months. You set your own pace within each intake, and your tutor helps you plan the workload around your job.
You work with ESA SNAP, ENVI, Zemax OpticStudio, MATLAB and Google Earth Engine, using free, academic or evaluation versions. Your tutor indicates the free alternative wherever one exists.
A SEIUM Institute diploma, awarded on passing the continuous assessment and the Master's Thesis. 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 in a course or postgraduate diploma in the same area are recognised in the higher programme. Ask about the recognition policy when you enrol.
A university degree in engineering, science or architecture (or equivalent professional experience), 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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