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Satellite ground stationsGround stations, ready for every pass.
A satellite ground station has minutes for each pass and loses signal in heavy rain. Weather sensors at the antennas, condition monitoring on antenna drives, timing references and site security report to one record that schedules passes around the weather and catches faults between them.
Plan a deploymentHow it worksStation Builder- Industry
- Telecom
- Measurements
- 5
- Sources cited
- 4
Telecom · Satellite ground stations
Minutes per pass, lost to the rain
A satellite crosses the sky in minutes, and a heavy shower over the station can wash out the link at higher frequencies. Antennas stop in high wind, and a worn drive can fail mid-pass. Measuring rain, wind and drive health at every antenna lets operators plan each pass and catch faults between them.
What is measured
Rain, wind, drives and time
Rain gauges beside each large antenna measure rain rate, anemometers at antenna height measure wind, and vibration sensors on motors and gearboxes follow drive health during motion. GNSS-disciplined references keep station time, and cameras watch pads and gates. Every reading names its antenna.
- Instruments
- Rain gauges · Anemometers · Drive vibration · GNSS timing · Cameras
The base node
Fade predicted for every pass
The station node predicts rain fade for each coming pass from the rain rate and the link frequency, flags antennas to stow in high wind, detects drive faults from vibration during motion and time-stamps every pass log against the GNSS reference.
Radio and links
Fibre home, and the sky as a spare
Ground stations are connected by fibre to their networks, and monitoring rides that fibre. When terrestrial links fail, the station’s own antennas or a small terminal carry the alarms, and an out-of-band cellular path is used where coverage exists. Each path is supervised.
- Links
- Fibre · Satellite · Public cellular
How it works
From a shower to a moved pass
A heavy shower approaches the station before a critical pass. Rain gauges read the rate rising, the node predicts the fade at the link frequency and alerts the scheduler, who moves the pass to a station in clear weather. The pass log records the weather and the decision.
From order to operation · Order
Scope the station and its passes
The scope reads the antennas, frequencies, pass schedule, weather history, timing and security arrangements. Nexus Observatory Inc. returns the point plan per antenna, the rain fade prediction method, the integration with scheduling and a price per station and per year.
Plan a deploymentFrom order to operation · Survey
Survey around the antennas
Crews survey each antenna with the station engineer: gauge and anemometer sites clear of the dish, drive access for vibration sensors, timing references and camera views over pads and gates. They record fibre, power and lightning protection. Every candidate site is photographed for the design.
From order to operation · Permits
Licences and site rules
Nothing new may radiate or interfere with the station’s licensed operation. Work on antennas follows the station’s safety and outage rules, and every approval is kept with the station record. Sensors are checked so that nothing new radiates in the station’s bands. Work on antennas follows the station’s outage plan, so no pass is lost to installation.
From order to operation · Build
Build for the antenna pad
Rain gauges, anemometers, vibration sensors, cameras, the timing reference and nodes are built, tested together and enrolled with their identities. Each antenna’s frequencies and stow limits are configured, and every part is labelled by antenna. Configurations are tested on the bench with the scheduler interface before shipping.
Open the Station BuilderFrom order to operation · Install
Install between passes
Crews install between passes: gauges and anemometers beside each antenna, vibration sensors on drives, cameras over pads and gates and the timing reference in the equipment room. Cables are protected against lightning, and every point is photographed. Each antenna returns to service before its next pass.
From order to operation · Commission
Check against a real pass
Each node proves its identity. Gauges are checked with a measured volume, anemometers against a reference, drive vibration baselines are taken on healthy antennas, and rain fade predictions are compared with received signal on real passes. Results are kept with the antenna record.
From order to operation · Operate
Schedule around the weather
Schedulers see predicted rain fade for each pass and move critical passes to stations in clear weather. Antennas stow when wind limits are reached, drive faults are planned for repair between passes, and every pass log carries its weather and timing.
From order to operation · Maintain
Maintain in pass gaps
Sensors are checked during antenna maintenance windows, gauges cleaned, drive baselines updated after repairs, and the timing reference checked against GNSS. Every change is recorded with the antenna, so pass and availability records stay complete. Spares are kept on site for quick swaps between passes.
Book field servicesData products
For schedulers, operators and customers
Pass schedulers receive rain fade predictions; station operators receive wind stow alerts; maintenance engineers receive antenna drive health; operators and customers receive pass logs with weather and timing. Each product carries its antenna, frequency and time. Reports are dated and versioned.
See the data productsEvidence
Availability on record
Every reading, prediction, pass and fault is signed and kept. Rain fade follows the ITU propagation recommendations, rain characteristics follow the ITU precipitation model, weather follows WMO practice, and operation follows the radio regulations and the station’s licence. Records are open to customers.
- Drawn against
- ITU-R P.618 · ITU-R P.837 · WMO-No. 8 · ITU Radio Regulations
What you get
Ground segment hosting
Antenna sites, shelters, power and fibre for satellite operators, with downlink and processing at the edge. Delivered as managed service and infrastructure hosting, for satellite operators, EO companies, research missions. Scale: Multi-site, multi-mission. Service levels are written as numbers you can measure on your own dashboard.
Talk to salesNext step
Plan satellite ground stations with us
Tell us the site, the measurements and the rules it answers to. We reply with a survey proposal, a design and a scope for satellite ground stations. An engineer replies with a survey proposal and a scope, and the plan grows from one site to the network you need, at your pace.
Plan a deploymentOpen the Station BuilderOpen the Studio
01The place and its hazards
Where it runs, and what can go wrong.
Operating contextGround stations track satellites through passes, uplinking commands and downlinking data, often unattended and far from towns. Rain attenuates higher-frequency links, wind limits antenna operation, lightning threatens equipment, and timing must be accurate. Propagation prediction follows ITU recommendations, and stations operate under radio regulations and their licences.
Hazards
- Rain fade losing passes at higher frequencies
- High wind stopping antennas
- Lightning damage
- Antenna drive and bearing faults
- Unattended sites open to intrusion
02What must be measured
What, where, how often, and under which rules.
Each measurement names where it is taken, how often, and the public standard or regulation behind it. Numbers in the sources column open the cited source below.
| Measurement | Where | Cadence | Sources |
|---|---|---|---|
| Rain rate | Gauges beside each large antenna | Continuous, at short intervals | 12 |
| Wind speed and gusts | Anemometers at antenna height | Continuous | 3 |
| Antenna drive condition | Motors, gearboxes and bearings | Continuous during motion | 4 |
| Time and frequency reference | GNSS-disciplined references | Continuous | 4 |
| Site access and images | Gates, shelters and antenna pads | On event | 4 |
03The observation stack
From one base unit to a network.
The same blocks at every scale: instruments and a base node, a site with its radio, a fleet run as one, and a network federated on the open protocol.
- 01
Base unit
An antenna point: rain, wind and drive sensors with a camera, read by an edge node with a timing reference.
Build a station → - 02
Site
A ground station: every antenna, the timing reference and site security on the station’s fibre.
Plan a site → - 03
Fleet
Every station of an operator or a ground network run as one fleet, with one record.
Managed offers → - 04
Network
Ground station operators and their customers exchange pass, weather and availability records through open standards.
The open protocol →
- 01Compact weather station
- 02GNSS reference station (RTK)
- 03Vibration and condition monitor
- 04PTZ camera
- 05Edge node (Wedge)
- 06Fibre terminal
- 07Lattice tower
Radio and links
Fibre
Ground stations are connected by fibre to their networks; monitoring rides it.
Radio and links
Satellite
The station’s own antennas or a small terminal carry alarms when terrestrial links fail.
Radio and links
Public cellular
An out-of-band path for site alarms where coverage exists.
Edge computeThe station node predicts rain fade for each coming pass from rain rate and the link’s frequency, flags antennas to stow in high wind, detects drive faults from vibration during motion and keeps every pass log time-stamped against the GNSS reference.
PowerMonitoring runs on the station’s protected supply with batteries.
04How it works
From the instrument to the product.
One observation’s path, tier by tier, with the interface on every link and a bill of materials below; then how the one node grows to a site, a fleet and federated networks.
Satellite ground stations: data path
– of 06
01 Instruments Measurement with sensor identity andcalibration 02 Node – Wrap in an observation envelope with timequality– Measure quality and uncertainty, attachquality flags– Buffer locally (store-and-forward when thelink drops) 03 Backhaul Commit with transactional outbox andpublish, delivered at least once 04 Site Consumer inbox deduplicates and applieseach record once into governed data 05 Data store Governed product through API, map orexport, correction-aware 06 Products ITU-R P.618ITU-R P.837OGC SensorThings API 07 Power and structure 01 Compact weather station SDI-12 · RS-485 · Ethernet 02 GNSS reference station (RTK) Ethernet · GNSS antenna · RS-232 ·1PPS/10 MHz 03 Vibration and condition monitor Analogue I/O · RS-485 · Ethernet 04 PTZ camera Ethernet 05 Edge node (Wedge) Ethernet · Fibre · USB · RS-485 ·BMC 06 Fibre terminal Fibre · Ethernet Site MQTT 5 with Sparkplug B Governed data store Versioned, correction-aware Rain fade predictions per pass Wind stow alerts Antenna drive health Pass logs with weather and timing 07 Lattice tower RS-485 Ethernet RS-485 Ethernet Fibre Fibre| Item | Equipment | Data ports | Protocols | Power in |
|---|---|---|---|---|
| 01 | Compact weather stationAll-in-one or compact station for temperature, humidity, pressure, wind and rain at a site. | SDI-12RS-485Ethernet | SDI-12, Modbus, MQTT 5, OGC SensorThings API | 12 V DC |
| 02 | GNSS reference station (RTK)Multi-constellation GNSS base station that streams corrections for real-time kinematic positioning. | EthernetGNSS antennaRS-2321PPS/10 MHz | NMEA 0183, NTP with NTS | 12 V DC |
| 03 | Vibration and condition monitorAccelerometer-based vibration and temperature sensor for rotating machinery and structural condition monitoring. | Analogue I/ORS-485Ethernet | Modbus, OPC UA, MQTT 5 | 12 V DC |
| 04 | PTZ cameraPan-tilt-zoom camera for wide-area visual monitoring (wildfire, flood, traffic). | Ethernet | RTSP with ONVIF profiles | PoE, 24 V DC |
| 05 | Edge node (Wedge)Rugged edge node that boots from signed media, attests itself and establishes a site cell from little or no infrastructure. | EthernetFibreUSBRS-485BMC | MQTT 5, DMTF Redfish, IEEE 1588 PTP, NTP with NTS, OPC UA | 12 V DC, 24 V DC, 48 V DC, AC mains |
| 06 | Fibre terminalOptical network terminal or media converter that lands fibre backhaul at a site. | FibreEthernet | IEEE 1588 PTP | 12 V DC, 48 V DC, AC mains |
| 07 | Lattice towerSelf-supporting or guyed lattice tower for macro radios, links and instruments. | — | — | — |
How it scales
01 Instruments Arbitrary qualified sensors and instruments whosemeasurements are ingested with calibration, units,geometry, time, custody and uncertainty. ×n 02 Node The minimum useful deployable unit: server, ruggedappliance, radio node, sensor gateway, satelliteterminal, AI, scientific, vehicle or virtual node. Node Node agent 03 Site The minimum independently operable localgovernance and failure domain: one or more nodesplus local network, identity, policy, evidence,storage, products and operator surfaces.SITE
Node Node Node ×n 04 Cluster An optional scale or specialisation domain forscheduling, shared storage, accelerators or datalocality.CLUSTER
×n 05 Fleet Coordinates plans, acknowledgements,convergence evidence, update campaigns andcorrection propagation across nodes and sites.FLEET
Fleet controller ×n 06 Federation An exchange of products, capabilities, events orwork across approved, independently administeredtrust domains, using explicit trust, policy,data-locality, version and correction contracts.TRUST DOMAIN
TRUST DOMAIN
TRUST DOMAIN
×n Verifier Applications Data in the field Telemetry Control Data upstream Control Data upstream Control Exchange Evidence Events Exchange- Data in the field
- MQTT 5 with Sparkplug B; connectors for LoRaWAN, OPC UA and instrument buses.
- Telemetry
- OpenTelemetry OTLP.
- Control
- TLS 1.3 with mutual authentication; protobuf messages over gRPC or HTTP/2.
- Data upstream
- At-least-once publication with repeat-safe keys over the control channel or NATS JetStream; QUIC MAY be used on lossy links.
- Evidence
- DSSE-signed in-toto statements; SLSA provenance; SCITT transparency receipts.
- Events
- Event envelopes mapped to CloudEvents 1.0; channels described in AsyncAPI 3.
- Exchange
- OpenAPI 3.1; the OGC API family; SensorThings; STAC; WIS 2.0.
05From order to operation
Every step, from the first call to a running site.
The same crew and the same record carry the work from scope to maintenance.
- 01 Order
Scope the station and its passes
The scope reads the antennas, frequencies, pass schedule, weather history, timing and security arrangements. Nexus Observatory Inc. returns the point plan per antenna, the rain fade prediction method, the integration with scheduling and a price per station and per year. 2
- 02 Survey
Survey around the antennas
Crews survey each antenna with the station engineer: gauge and anemometer sites clear of the dish, drive access for vibration sensors, timing references and camera views over pads and gates. They record fibre, power and lightning protection. Every candidate site is photographed for the design.
- 03 Permits
Licences and site rules
Nothing new may radiate or interfere with the station’s licensed operation. Work on antennas follows the station’s safety and outage rules, and every approval is kept with the station record. Sensors are checked so that nothing new radiates in the station’s bands. Work on antennas follows the station’s outage plan, so no pass is lost to installation. 4
- 04 Build
Build for the antenna pad
Rain gauges, anemometers, vibration sensors, cameras, the timing reference and nodes are built, tested together and enrolled with their identities. Each antenna’s frequencies and stow limits are configured, and every part is labelled by antenna. Configurations are tested on the bench with the scheduler interface before shipping.
- 05 Install
Install between passes
Crews install between passes: gauges and anemometers beside each antenna, vibration sensors on drives, cameras over pads and gates and the timing reference in the equipment room. Cables are protected against lightning, and every point is photographed. Each antenna returns to service before its next pass.
- 06 Commission
Check against a real pass
Each node proves its identity. Gauges are checked with a measured volume, anemometers against a reference, drive vibration baselines are taken on healthy antennas, and rain fade predictions are compared with received signal on real passes. Results are kept with the antenna record.
- 07 Operate
Schedule around the weather
Schedulers see predicted rain fade for each pass and move critical passes to stations in clear weather. Antennas stow when wind limits are reached, drive faults are planned for repair between passes, and every pass log carries its weather and timing. 21
- 08 Maintain
Maintain in pass gaps
Sensors are checked during antenna maintenance windows, gauges cleaned, drive baselines updated after repairs, and the timing reference checked against GNSS. Every change is recorded with the antenna, so pass and availability records stay complete. Spares are kept on site for quick swaps between passes.
06Data products and integration
What it delivers, to whom, and into which systems.
Data products
- Rain fade predictions per passPass schedulers
- Wind stow alertsStation operators
- Antenna drive healthMaintenance engineers
- Pass logs with weather and timingOperators and customers
Integration
- Pass schedulingPredicted fade per pass feeds the scheduling system.
- Station controlStow alerts reach the antenna control system through its own interfaces.
- Customer reportingAvailability and pass logs are exported for customers.
Exchanged through ITU-R P.618, ITU-R P.837, OGC SensorThings API.
07Questions buyers ask
Before you scope it.
How is rain fade predicted?
From measured rain rate and the link frequency, using the ITU propagation methods.
Will sensors interfere with the antennas?
Nothing radiates in the station’s bands, and sites are chosen clear of the dish.
Can passes move to another station?
Yes, where the network has one in clear weather; the scheduler decides.
What timing is used?
GNSS-disciplined references at each station.
08Resources
The sources behind this page.
Public standards, regulations and guidance, cited where they apply. Each applies only where its jurisdiction or scope does.
- 1Recommendation ITU-R P.837: Characteristics of precipitation for propagation modellingInternational Telecommunication Union
- 2Recommendation ITU-R P.618: Propagation data and prediction methods for Earth-space telecommunication systemsInternational Telecommunication Union
- 3Guide to Instruments and Methods of Observation (WMO-No. 8)World Meteorological Organization
- 4ITU Radio RegulationsInternational Telecommunication Union
09Related
Use cases and solutions.
SolutionGround segment hosting
Antenna sites, shelters, power and fibre for satellite operators, with downlink and processing at the edge.Solutions for telecom →SolutionTiming and positioning integrity
PTP grandmasters with GNSS holdover, interference detection and timing monitoring for networks and instruments.Solutions for telecom →10Telecom: specialized fields
Other fields of this industry.
Specialized fieldMobile network sites
Power and batteries, shelter climate, tower movement, intrusion and site weather at every mobile site, with an out-of-band path that reports when the site itself is down.The full field →Specialized fieldFibre networks and outside plant
Distributed fibre sensing along routes, flooding and gas in chambers, and cabinet access and climate, on LoRaWAN and the fibre itself, so dig-ins and faults are found before the cable is cut.The full field →Specialized fieldEdge data centres
Power and energy, cooling and air, leaks and vibration in edge and regional data centres, on an industrial network behind a security gateway, with efficiency indicators to the standard.The full field →Specialized fieldSpectrum monitoring and interference
Fixed and mobile receivers that measure occupancy, find interference and locate its source by direction finding and time difference, with GNSS timing, so regulators and operators clear the bands they depend on.The full field →Bring us the site.
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