Radio Spectrum Codexery

Equivalent power flux density

A regulatory metric for NGSO-to-GSO interference in shared satellite spectrum.

Equivalent power flux density

Equivalent power flux density (EPFD) measures the total radio frequency interference that a constellation of non-geostationary orbit (NGSO) satellites creates at a receiving station in geostationary orbit (GSO). It extends the basic idea of spectral flux density to systems where many transmitters are visible at once. Each satellite’s contribution is scaled by the receiving antenna’s gain in that satellite’s direction, and the results are added together across all satellites in view. EPFD is defined in Article 22 of the International Telecommunication Union’s Radio Regulations and in corresponding national rules, such as those from the U.S. Federal Communications Commission. Historically, it has been used to decide whether an NGSO fixed-satellite service (FSS) system can share frequencies with GSO satellites without needing individually negotiated coordination agreements.

The ordinary power flux density from a single transmitter follows the inverse-square law, depending on the transmitter’s effective isotropic radiated power in the direction of interest and the distance to the receiver. But a GSO receiving station is rarely affected by just one interferer. An NGSO constellation can place dozens of satellites above the horizon at once, each at a different distance, transmit angle, and angle relative to the receiving antenna’s boresight. EPFD handles this by scaling each contributor’s power flux density by the receiving antenna’s gain toward that satellite, relative to the antenna’s peak gain, then summing the linear-power results before converting back to a logarithmic value.

Formally, as described in RR Article 22.5C.1 and mirrored in U.S. regulation at 47 CFR § 25.103, EPFD in dB(W/m²) in a specified reference bandwidth is calculated using: the number of transmitting stations in the NGSO system visible from the GSO station; the radio-frequency power of each transmitter in the reference bandwidth; the off-axis angle between that transmitter’s boresight and the direction of the GSO station; the transmitting antenna’s gain in that direction; the distance between the transmitter and the GSO station; the off-axis angle at the GSO receiving antenna toward that transmitter; the receiving antenna’s gain in that direction; and the receiving antenna’s peak gain.

Defined in
Article 22 of the ITU Radio Regulations
Reference bandwidth for ku band
40 kHz
Reference bandwidth for ka band
40 kHz or 1 MHz
Ku-band epfd trigger level for ngso sate
−202 dBW/m²/40 kHz
Assumed effective number of co-frequency
3.5
Date of fcc replacement of epfd rules
April 30, 2026

Lore & Background

The EPFD concept emerged from a regulatory dispute in the 1990s over how non-geostationary broadband constellations could share spectrum already used by geostationary systems. The 1995 Radio Regulations obliged non-GSO systems to 'cease or reduce to a negligible level' any emissions found to cause unacceptable interference to GSO networks, without specifying what threshold of interference that meant in quantitative terms. The issue came to a head around proposed non-GSO constellations such as Alcatel SkyBridge and Teledesic, which sought to reuse Ku- and Ka-band spectrum already allocated to GSO fixed-satellite systems. At the 1997 World Radiocommunication Conference, European administrations proposed resolving the ambiguity by defining quantitative interference limits, expressed as EPFD, that a non-GSO system could meet in order to be deemed compliant without negotiating individually with every GSO operator. These provisional limits were refined using a set of reference GSO links, rain fade statistics, and unavailability criteria, and were formally incorporated into Article 22 of the Radio Regulations at WRC-2000. Limits have subsequently been applied to portions of the Ku, Ka, and C bands.

Three related quantities are defined: EPFDdown (interference from NGSO satellite downlinks into a GSO earth station's downlink reception), EPFDup (interference from NGSO earth stations into a GSO satellite's uplink reception), and EPFDis (inter-satellite interference, in which an NGSO satellite's downlink emissions fall into bands where GSO satellites receive uplink signals). Because EPFD depends on constellation geometry that changes continuously, verifying compliance requires simulation rather than a single closed-form calculation. Recommendation ITU-R S.1503 sets out the standardized methodology used by the ITU Radiocommunication Bureau to check whether a filed non-GSO system meets the Article 22 limits, based on parameters an administration submits describing its system's technical envelope.

Reader's Guide

EPFD's fixed technical limits have drawn sustained criticism as broadband satellite constellations have grown far larger and more capable than the systems the framework was designed around in the 1990s. The International Telecommunication Union itself noted in 2023 that the existing Ku- and Ka-band EPFD provisions are 'spectrally inefficient' and unnecessarily constrain non-GSO systems without providing additional protection to GSO operators, calling for the limits to be revisited. When the ITU studied a comparable sharing problem for the higher-frequency Q band and V band ahead of a 2019 conference, it deliberately chose not to replicate the EPFD approach, instead developing a different framework subsequently addressed under Resolution 770. In the United States, the Federal Communications Commission moved unilaterally away from EPFD for domestic purposes in 2026, voting on April 30, 2026 to replace its EPFD-based satellite spectrum-sharing rules with a performance-based framework that instead relies on voluntary coordination between operators, backed by specific throughput-degradation and service-unavailability backstops, along with a minimum avoidance angle from the GSO arc. Proponents, including non-geostationary operators, argued the decades-old EPFD limits were based on outdated technical assumptions and constrained the throughput of modern low-Earth-orbit systems. Geostationary operators generally opposed the change, warning that relaxed limits could cause new interference to their in-service satellites. The FCC's action applies only within United States jurisdiction, and EPFD continues to apply internationally.

Did You Know?

Regulatory Purpose: Enabling Constellation-Scale Spectrum Sharing

EPFD exists to solve a practical regulatory problem: how to let large constellations of non-geostationary satellites coexist with geostationary satellites on the same frequencies without requiring bilateral coordination deals between every pair of operators. The International Telecommunication Union codified this concept in Article 22 of its Radio Regulations, and national authorities such as the U.S. Federal Communications Commission adopted it into their own rulebooks, specifically at 47 CFR § 25.103. Under this framework, an NGSO fixed-satellite service system can demonstrate compliance by showing that its aggregate interference at a protected GSO receiving station stays within a defined EPFD limit. This approach replaces the older, more cumbersome method of individually negotiated coordination agreements for each satellite-to-satellite pair, effectively scaling the regulatory burden to match the operational reality of constellations containing dozens or more active transmitters simultaneously visible from a single protected station.

From Single-Transmitter PFD to a Constellation-Wide Metric

The starting point is the familiar power flux density of a single transmitter, which follows directly from the inverse-square law: the effective isotropic radiated power in a given direction divided by four pi times the distance squared. For a lone interferer this is straightforward. A geostationary receiving station in practice, however, sees an entirely different picture. A non-geostationary constellation can place dozens of satellites above the horizon at any instant, each at a different slant range, each radiating at a different off-axis angle relative to its own boresight, and each arriving at the GSO antenna from a different direction. EPFD generalizes the single-source PFD by treating every visible transmitter as a contributor, scaling each one's flux density by the receiving antenna's gain in that particular direction relative to the antenna's peak gain, summing all contributions in linear power, and then converting the total back to a logarithmic expression in decibels per square meter within a specified reference bandwidth.

The Formal Summation and Its Governing Variables

The formal expression, as set out in ITU Radio Regulations Article 22.5C.1 and mirrored in U.S. regulation, sums over every transmitting station in the NGSO system that is visible from the protected GSO station. For each contributor, the formula incorporates the transmitter's radio-frequency power in the reference bandwidth, the transmitting antenna's gain evaluated at the specific off-axis angle between that satellite's boresight and the direction toward the GSO station, the slant distance between the two, and the receiving antenna's gain at the off-axis angle toward that particular transmitter, normalized by the receiving antenna's maximum gain. The result of each per-satellite term is a linear-power quantity; all such terms are added together, and the final sum is converted to a logarithmic value expressed in dB(W/m²). This structure ensures that satellites closer to the boresight of either antenna contribute more heavily, while those far off-axis are naturally attenuated by the antenna-pattern terms.

Why Antenna Geometry and Distance Shape the Result

A critical feature of the EPFD formulation is that it is not simply a sum of raw radiated powers. Each satellite's contribution is modulated by two antenna-pattern factors: the transmitting antenna's gain in the direction of the GSO station, evaluated at the off-axis angle between the transmitter's boresight and the receiver, and the receiving antenna's gain toward that satellite, evaluated at the off-axis angle at the GSO station and normalized by the antenna's peak gain. This means a satellite radiating strongly but pointing well off the GSO station's direction contributes little, while one in a favorable geometric alignment contributes more. The inverse-square distance term further weights nearer satellites more heavily. Together, these geometric and pattern-dependent factors ensure that EPFD reflects the actual electromagnetic environment at the receiving aperture rather than an abstract total of transmitted power, making it a physically meaningful interference metric for spectrum-sharing decisions.

Frequently Asked Questions

What is Equivalent Power Flux Density (EPFD)?

EPFD is a regulatory metric that captures the total RF interference a non-geostationary orbit (NGSO) satellite constellation produces at a geostationary orbit (GSO) receiving station. It generalizes the single-transmitter spectral flux density concept to situations where many satellites are visible simultaneously.

Where does EPFD come from in the rules?

It is defined in Article 22 of the ITU Radio Regulations. The FCC is set to replace its own EPFD rules on April 30, 2026.

How is EPFD calculated across a constellation?

Each satellite's interference contribution is scaled by the receiving antenna's gain in that satellite's direction, and all visible satellites' weighted contributions are then summed into a single flux-density figure.

What reference bandwidths apply to EPFD?

Ku band uses a 40 kHz reference bandwidth, while Ka band can use either 40 kHz or 1 MHz depending on the scenario.

What's the Ku-band EPFD trigger level for NGSO satellites?

The threshold is −202 dBW/m² per 40 kHz, and the calculation assumes an effective number of 3.5 co-frequency interferers.

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