Satellite Communications and Space Satellite Link Design Informational

How do I design a ground station receiver for a LEO satellite constellation like Starlink or OneWeb?

A LEO ground station for constellations like Starlink, OneWeb, or Kuiper must handle: fast satellite tracking (satellites cross the sky in 5-15 minutes, requiring track rates up to 3°/s), frequent handovers (switching from one satellite to the next every few minutes), simultaneous multi-satellite links (gateway stations may communicate with 4-8 satellites simultaneously), and wideband operation (user terminals: 250-1000 MHz bandwidth; gateway stations: 2-4 GHz). User terminal: flat-panel electronically steered antenna (phased array), 0.3-0.5 m aperture, 10-20W transmit power, self-aligning. Gateway station: 2-4 m dishes on tracking pedestals (8-16 antennas for multi-satellite access), or large phased arrays. Frequency bands: Ku-band (12/14 GHz) or Ka-band (20/30 GHz) for user terminals, Ka-band or V-band (40/50 GHz) for gateway links.
Category: Satellite Communications and Space
Updated: April 2026
Product Tie-In: LNBs, BUCs, Feeds, Antennas

LEO Ground Station

The handover process: as one satellite sets below the useful elevation angle (typically 25-40°), the ground terminal must acquire the next rising satellite and transfer the data session. For seamless handover: make-before-break (connect to the new satellite before disconnecting from the old one). This requires either two antenna beams or pre-acquisition of the new satellite's signal. Handover intervals: every 2-8 minutes for a 550 km constellation. The network manages handover centrally, providing the terminal with timing, frequency, and beam pointing information for the next satellite.

ParameterGEOMEOLEO
Altitude35,786 km2,000-35,786 km200-2,000 km
Latency (one-way)~270 ms50-150 ms1-20 ms
Coverage per SatFull hemisphereRegionalLocal footprint
HandoverNonePeriodicFrequent
Path Loss (Ku-band)~206 dB190-206 dB170-190 dB
  • Performance verification: confirm specifications against the application requirements before finalizing the design
  • Environmental factors: temperature range, humidity, and vibration affect long-term reliability and parameter drift
  • Cost vs. performance: evaluate whether the application demands premium components or standard commercial grades
  • Interface compatibility: verify impedance, connector type, and mechanical form factor match the system architecture
Common Questions

Frequently Asked Questions

Why phased array for user terminals?

Mechanical dishes cannot track LEO satellites fast enough (3°/s track rate) without expensive, heavy pedestals. Flat-panel phased arrays steer the beam electronically in microseconds, enabling: fast tracking, seamless handovers, and a form factor suitable for consumer installation (roof-mount flat panel). The Starlink Dishy uses a 0.5 m phased array with > 1,000 elements.

What about interference between constellations?

Multiple LEO constellations sharing the same frequency bands (Ku, Ka) must coordinate to avoid inter-system interference. ITU rules require coordination and may impose power flux density limits. Inline events (when two constellations' satellites align along the same path to a ground station) can cause significant interference. Frequency reuse planning and dynamic power control mitigate these issues.

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