POES Satellite Data Guide
Polar Operational Environmental Satellites (POES) provide continuous high-latitude measurements of energetic particles, magnetic fields, and spacecraft position. This guide explains the unified POES endpoint, available satellites, and data fields.
Overview
Satellite Network: NOAA POES satellites operate in sun-synchronous polar orbits at approximately 840 km altitude, passing over the Earth's poles about 14 times per day. These satellites monitor energetic particles and magnetic fields in the auroral regions.
Data Coverage: 1998-present
Update Interval: 1-minute granularity; data typically available within 1-3 days after downlink
Total Records: >18 million measurements across 5 satellites
Active Satellites
| Satellite | Status | Orbit Type | Agency |
|---|---|---|---|
| NOAA-15 | Operational | Sun-synchronous (~840 km) | NOAA |
| NOAA-18 | Operational | Sun-synchronous (~840 km) | NOAA |
| NOAA-19 | Operational | Sun-synchronous (~840 km) | NOAA |
| MetOp-01 (MetOp-A) | Operational | Sun-synchronous (~840 km) | EUMETSAT |
| MetOp-03 (MetOp-B) | Operational | Sun-synchronous (~840 km) | EUMETSAT |
Data Fields
The unified POES endpoint returns comprehensive measurements organized into four categories:
1. Position Data (Geodetic Coordinates)
latitude- Satellite latitude in degrees (-90 to +90)longitude- Satellite longitude in degrees (-180 to +180)altitude_km- Satellite altitude above sea level (kilometers)
2. Magnetic Field Data (IGRF Model)
Measurements of Earth's magnetic field in two reference frames:
At Satellite Location
btot_sat- Total magnetic field magnitude (nanoTesla)bp_sat- Parallel (B_||) component (nanoTesla)br_sat- Radial (B_r) component (nanoTesla)bt_sat- Theta (B_θ) component (nanoTesla)
At Foot of Field Line (Earth's Surface)
btot_foot- Total field at footpoint (nanoTesla)bp_foot- Parallel component at footpoint (nanoTesla)br_foot- Radial component at footpoint (nanoTesla)bt_foot- Theta component at footpoint (nanoTesla)
Cartesian Coordinates (Satellite Frame)
bx_sat- X component (nanoTesla)by_sat- Y component (nanoTesla)bz_sat- Z component (nanoTesla)
3. Electron Flux Data (4 Energy Channels)
Energetic electron measurements across different energy levels:
elec_flux_e0- Electron flux in E0 channel (particles/cm²/s/sr)elec_flux_e1- Electron flux in E1 channel (particles/cm²/s/sr)elec_flux_e2- Electron flux in E2 channel (particles/cm²/s/sr)elec_flux_e3- Electron flux in E3 channel (particles/cm²/s/sr)elec_energy- Reference energy array for electron channels (keV) [E0, E1, E2, E3]
4. Proton Flux Data (8 Energy Channels)
Energetic proton measurements across multiple energy levels:
prot_flux_p1throughprot_flux_p8- Proton flux in P1-P8 channels (particles/cm²/s/sr)prot_energy- Reference energy array for proton channels (MeV) [P1, P2, ..., P8]
5. Alpha Particle Flux Data (4 Energy Channels)
Energetic alpha particle (He²⁺) measurements:
alpha_flux_a1throughalpha_flux_a4- Alpha flux in A1-A4 channels (particles/cm²/s/sr)alpha_energy- Reference energy array for alpha channels (MeV) [A1, A2, A3, A4]
6. Metadata
timestamp- Measurement time (ISO 8601 UTC)satellite- Satellite identifier (NOAA15, NOAA18, NOAA19, METOP01, METOP03)
API Usage
Get POES data for a date range
Code
Filter by satellite
Code
Paginate through results
Code
Response Example
Code
Common Use Cases
Monitoring Auroral Electron Precipitation
Query elec_flux_* fields during geomagnetic substorms to track electron precipitation at high latitudes.
Radiation Belt Studies
Track prot_flux_* and alpha_flux_* data to study radiation belt dynamics and particle acceleration.
Magnetic Field Analysis
Use btot_sat and component fields (bp_sat, br_sat, bt_sat) for magnetospheric studies and field-aligned current analysis.
Space Weather Alerts
Sudden increases in prot_flux_* can indicate solar energetic particle events. Monitor during solar activity.
Data Quality Notes
- Gaps may occur during satellite maintenance or data transmission issues
- Fields with
nullvalues indicate missing or excluded data for that measurement - All flux values are in particles/(cm² · s · sr) unless otherwise noted
- Energy values represent the geometric center of each channel's response function
- Timestamps are in UTC; convert to local time as needed for your analysis
API Parameters
| Parameter | Type | Required | Description | Example |
|---|---|---|---|---|
start_time | ISO 8601 | Yes | Start of time range | 2025-01-01T00:00:00Z |
end_time | ISO 8601 | Yes | End of time range | 2025-01-02T00:00:00Z |
satellite | String | No | Filter by satellite | NOAA19 |
limit | Integer | No | Records per page (default 1000, max 10000) | 5000 |
offset | Integer | No | Pagination offset | 0 |
See Also
- API Reference: /poes - Full endpoint documentation
- Geomagnetic Storms - Related space weather phenomena
- GOES Data - Complementary geostationary satellite measurements