WIA-ENE-051 | Greenhouse Gas Monitoring Standard v1.0
Monitoring greenhouse gases from space - the global perspective
Satellite remote sensing revolutionized GHG monitoring by providing capabilities impossible from the ground:
| Advantage | Description | Impact |
|---|---|---|
| Global Coverage | Monitor entire planet, including oceans and remote areas | No geographic blind spots |
| Consistency | Single instrument, standardized methodology | Comparable data across borders |
| Independence | Objective data not controlled by individual nations | Verify self-reported emissions |
| Systematic Sampling | Regular revisit patterns | Track temporal trends globally |
| Emission Detection | Identify large point sources and plumes | Find unreported emissions |
Satellites excel at: Spatial coverage, source detection, regional budgets
Ground stations excel at: Precision, long-term trends, validation
Optimal approach: Combine both for comprehensive monitoring
Most GHG satellites use passive spectrometers measuring reflected or emitted radiation:
Key concept: More absorption → less light reaching satellite → higher GHG concentration
| Spectral Region | Wavelength | Gases | Advantages | Challenges |
|---|---|---|---|---|
| Near-Infrared (NIR) O₂ A-band | ~0.76 μm | O₂ | Reference for surface pressure and light-path (cloud/aerosol) correction | Requires sunlight |
| Shortwave IR (SWIR) | 1.6-2.4 μm (CO₂ 1.61 and 2.06 μm, CH₄ 1.65 and 2.3 μm) | CO₂, CH₄, CO, H₂O | Strong absorption bands with sensitivity down to the surface | Requires sunlight and surface reflection |
| Thermal IR (TIR) | ~4-15 μm | CO₂, CH₄, N₂O, O₃ | Day/night operation, vertical profiles | Reduced sensitivity near the surface |
| Agency | NASA (USA) |
| Launch | July 2, 2014 |
| Status | Operational |
| Orbit | Sun-synchronous, 705 km altitude |
| Target Gas | CO₂ |
| Measurement | Column-averaged XCO₂ |
| Spectral Bands | 0.765 μm (O₂ A-band), 1.61 μm, 2.06 μm (CO₂) |
| Footprint | 1.29 × 2.25 km |
| Precision Goal | < 0.5 ppm XCO₂ (achieved: ~0.5-1 ppm) |
| Swath | ~10 km |
Key Achievement: NASA's first dedicated CO₂ observing satellite, which opened the era of dense, high-precision XCO₂ observations. Its successor instrument, OCO-3, has performed urban observations (Snapshot Area Map mode) from the International Space Station (ISS) since 2019
Observing Modes:
| Agency | JAXA, National Institute for Environmental Studies (NIES), and Ministry of the Environment (Japan) |
| Launch | January 23, 2009 |
| Nickname | "Ibuki" (breath) |
| Status | Operational |
| Orbit | Sun-synchronous, 666 km |
| Target Gases | CO₂, CH₄ |
| Instrument | TANSO-FTS (Fourier Transform Spectrometer) |
| Spectral Range | 0.76-14.3 μm (SWIR and TIR) |
| Footprint | 10.5 km diameter |
| Precision | < 2 ppm XCO₂, < 10 ppb XCH₄ |
Historical Significance: First dedicated GHG monitoring satellite
Successors: GOSAT-2 launched in October 2018, and the Global Observing SATellite for Greenhouse gases and Water cycle (GOSAT-GW) launched in June 2025
| Agency | ESA / EU Copernicus (Europe) |
| Launch | October 13, 2017 |
| Orbit | Sun-synchronous, 824 km |
| Target Gases | CH₄, NO₂, CO, O₃, SO₂, HCHO |
| Instrument | TROPOMI (TROPOspheric Monitoring Instrument) |
| Spectral Range | 270-2385 nm (UV-VIS-NIR-SWIR) |
| Resolution (CH₄, SWIR) | 7 × 7 km² (value in specification); 5.5 × 7 km² since August 2019 |
| Swath | 2600 km |
| Coverage | Daily global |
Breakthrough: Unprecedented spatial resolution for methane detection
Impact: Used to detect large methane emission events worldwide from oil and gas facilities, coal mines, landfills, and other sources
| Operator | GHGSat Inc. (Canada) |
| First Launch | 2016 (GHGSat-D demo) |
| Constellation | Commercial constellation of multiple small satellites |
| Target Gas | CH₄ (primary), CO₂ |
| Resolution | ~25 m (facility-scale) |
| Model | Commercial service (subscription-based) |
Business Model: On-demand monitoring for oil & gas companies and regulators
Advantage: Ultra-high resolution enables facility-level attribution
Definition: Total column amount of gas divided by total column of dry air
XCO₂ = (Total CO₂ column) / (Total dry air column)
Units: ppm (parts per million)
Example:
Total CO₂ column: 8.8 × 10²¹ molecules/cm²
Dry air column: 2.12 × 10²⁵ molecules/cm²
XCO₂ = (8.8 × 10²¹) / (2.12 × 10²⁵) × 10⁶ ≈ 415 ppm
Why use XCO₂ vs. surface concentration?
| Level | Description | Contents | Users |
|---|---|---|---|
| L0 | Raw data | Instrument digital counts, engineering data | Mission teams |
| L1B | Calibrated radiances | Geolocated, calibrated spectra | Algorithm developers |
| L2 | Geophysical retrievals | XCO₂, XCH₄ with quality flags and errors | Scientists, advanced users |
| L3 | Gridded products | Spatial/temporal averages, gap-filled | General users, modelers |
| L4 | Model outputs | Flux inversions, forecasts | Policy makers, public |
Converting measured spectra to GHG concentrations is complex and non-trivial:
Key challenges:
| Algorithm | Mission | Approach | Key Features |
|---|---|---|---|
| ACOS | OCO-2/3 | Optimal estimation | Full physics, aerosol scattering |
| RemoTeC | TROPOMI | Phillips-Tikhonov | Fast processing, operational |
| FOCAL | OCO-2 | Fast iterative | Independent retrieval to cross-validate ACOS results |
| NIES L2 | GOSAT | Optimal estimation (full physics) | Operational algorithm of Japan's National Institute for Environmental Studies (NIES) |
Satellites can now detect individual emission plumes from large sources:
Detection threshold (approximate): TROPOMI can detect CH₄ sources on the order of several tonnes per hour; high-resolution satellites such as GHGSat can detect sources on the order of several hundred kg per hour
Detection algorithm:
1. Calculate anomaly: ΔCH₄ = Observed - Background
2. Identify contiguous enhanced pixels
3. Apply statistical threshold (e.g., > 3σ)
4. Compute integrated mass enhancement (IME)
5. Estimate emission rate using wind speed
Emission rate (kg/hr) ≈ IME × U_eff / L
(U_eff = effective wind speed, L = plume length scale (square root of plume area))
Major sources detected:
| Resolution | Satellite | Attribution Capability | Typical Use Case |
|---|---|---|---|
| 25 m | GHGSat | Individual facility | Specific well pad, plant |
| ~5-7 km | TROPOMI | Cluster of facilities | Oil field, industrial zone |
| 10 km | GOSAT | City or region | Urban emissions, large basin |
| Source | Typical Magnitude | Mitigation |
|---|---|---|
| Instrument noise | ~0.5 ppm XCO₂ | Averaging, better SNR |
| Aerosol scattering | 0.5-2 ppm bias | Simultaneous aerosol retrieval |
| Cloud contamination | Variable bias | Strict cloud screening |
| Surface reflectance | 0.3-1 ppm | Improved surface models |
| Spectroscopy | ~0.2 ppm | Laboratory measurements |
| Calibration drift | 0.1-0.5 ppm/year | On-board calibration, vicarious calibration |
Satellite observations are used in inverse models to estimate surface fluxes:
Forward problem: Fluxes → Concentrations (atmospheric transport)
Inverse problem: Concentrations → Fluxes (infer sources/sinks)
Basic equation:
y = H × x + ε
where:
y = observations (satellite XCO₂)
x = state vector (fluxes at surface)
H = observation operator (transport model)
ε = observation error
Goal: Find x that best fits y
Solution approach (Bayesian):
x̂ = xb + BH^T(HBH^T + R)^-1(y - Hxb)
where:
xb = prior fluxes (best guess)
B = prior error covariance
R = observation error covariance
x̂ = optimized (posterior) fluxes
| Agency | ESA / EU Copernicus / EUMETSAT (Europe) |
| Launch | 2027 or later (planned; delayed from 2025 in the specification's Phase 4 roadmap) |
| Mission Type | Operational constellation (multiple satellites) |
| Orbit | Sun-synchronous |
| Gases | CO₂, CH₄, NO₂ (co-emitted tracer) |
| Resolution | ~2 × 2 km² |
| Precision Goal | < 0.7 ppm XCO₂ |
Objective: Monitor fossil fuel CO₂ emissions from cities and power plants
Innovation: Aims to be an operational (not research) CO₂ monitoring system
| Agency | NASA (USA) |
| Status | Cancelled by NASA in November 2022 (cost growth and schedule delays) |
| Planned Orbit | Geostationary (over Americas) |
| Planned Gases | CO₂, CH₄, CO, solar-induced fluorescence |
Significance: Introduced the concept of observing the same region several times a day from geostationary orbit to track the diurnal evolution of emissions and biospheric fluxes
Relation to the Specification: The specification's Phase 4 roadmap plans GeoCarb integration in 2026, but because the mission was cancelled, this item must be replaced by another geostationary mission
| Agency | CNES (France) |
| Launch | July 2025 |
| Gas | CO₂ |
| Platform | Small satellite |
| Resolution | 4.5 × 9 km² |
Innovation: Europe's first dedicated CO₂ observing satellite, demonstrating CO₂ monitoring with a small satellite
Data ingestion API: The SDK call below is an example that wraps the specification's Phase 3 §8 REST endpoint GET /api/v1/ghg/concentration.
// Fetch satellite XCO2 data for region
const satelliteData = await wia.satellite.query({
mission: 'OCO-2',
gas: 'CO2',
product: 'XCO2',
level: 'L2',
bbox: [lon_min, lat_min, lon_max, lat_max],
date_range: ['2025-01-01', '2025-12-31'],
quality_filter: 'good'
});
// Returns standardized GeoJSON with metadata
{
type: 'FeatureCollection',
mission: 'OCO-2',
processing_version: 'v10r',
features: [...]
}
Multi-mission fusion:
Quality assurance: