Skip to content
DraconiticResearch
Search Sources API
203,203 studies31 sourcesUpdated 59 min ago
PreprintCC BY 4.0arXiv

A measurement-based approach to EPFD calculation, to quantify the impact of satellite mega-constellations on low-frequency radio astronomy

Abstract

Context: Satellite mega-constellations generate Unintended Electro-Magnetic Radiation (UEMR) impacting low frequency radio astronomy. The Radio Regulations of the International Telecommunications Union Radiocommunication Sector (ITU-R) contain the basis for addressing UEMR, but enforcement mechanisms are absent. Aims: To adapt compatibility study methods based on satellite constellation simulations, in particular the Equivalent Power Flux-Density (EPFD) framework, to radio telescope measurements. Methods: We adapt the ITU-R EPFD calculation framework to measurement data obtained from all-sky interferometric imaging. We address the conceptual differences between forward-model EPFD calculations and measurement-based approaches. In particular, we consider low frequency systems, which are typically wide field-of-view and interferometric instruments. Results: For the first time, we demonstrate that all-sky interferometric observations enable a direct adaptation of the EPFD formalism to measurement data. We thus confirm previous estimations (Di Vruno et al. 2023) that the resulting measurement-based EPFD distributions exceed the radio astronomy interference threshold levels defined in Recommendation ITU-R RA.769-2 in 50-70% of samples. These exceedance fractions are well above the 2% single-system data-loss criterion in Recommendation ITU-R RA.1513-2. Expressed using the conventional 2% compatibility margin, the corresponding margins are negative, ranging from -18.6 to -16.3 dB, equivalent to a required uniform attenuation of 16.3-18.6 dB. Conclusions: Measurement-based implementations provide a practical pathway toward verification and long-term monitoring at low radio frequencies, which could form an important component of enforceability. We suggest instrumentation approaches to support measurement.

Related

  1. A measurement-based approach to equivalent power flux density calculation, to quantify the impact of satellite mega-constellations on low-frequency radio astronomy
    S. J. Tingay, G. Hellbourg, D. Sheen +4
    Astronomy & AstrophysicsPeer-reviewedCC BY 4.0Full textSolar & stellar physicsCrossrefDOAJ
  2. Space Electric and Magnetic Sensor (SEAMS) Phase I: A Pathfinder Mission for Low-Frequency Radio Astronomy
    Atharva Kulkarni, Samruddhi Rohokale, Niketan Pawar +7
    arXivPreprintCC BY 4.0Full textInstrumentation & methodsarXiv
  3. Pushing the frontiers of low-frequency radio astronomy: An ultra-deep sub-arcsecond LOFAR image of ELAIS-N1
    J. M. G. H. J. de Jong, L. K. Morabito, R. J. van Weeren +11
    arXivPreprintCC BY 4.0Full textInstrumentation & methodsarXiv
  4. Real-Time Doppler-Frequency Measurement and Frequency-Pulling Suppression in Arm-locking
    Zheng-Rong Xiang, Jun Ke, Tian-Chi Zhu +3
    arXivPreprintarXiv licenceFull textInstrumentation & methodsGravitation & general relativityarXiv
  5. A frequency-resolved measurement of the scattering law in FRB 20210415C
    Victor Pop, Mohammed A. Chamma, Aishwarya Kumar +1
    arXivPreprintCC BY 4.0Full textHigh-energy astrophysicsInstrumentation & methodsarXiv
BibTeX
@misc{tingay2026measurementbased,
  title = {{A measurement-based approach to EPFD calculation, to quantify the impact of satellite mega-constellations on low-frequency radio astronomy}},
  author = {Steven J. Tingay and Gregory Hellbourg and Daniel Sheen and Dylan Grigg and Benjamin Winkel and Federico Di Vruno and Balthasar Indermuehle},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.01995},
  eprint = {2609.01995},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.01995},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - A measurement-based approach to EPFD calculation, to quantify the impact of satellite mega-constellations on low-frequency radio astronomy
AU  - Steven J. Tingay
AU  - Gregory Hellbourg
AU  - Daniel Sheen
AU  - Dylan Grigg
AU  - Benjamin Winkel
AU  - Federico Di Vruno
AU  - Balthasar Indermuehle
PY  - 2026
DA  - 2026/09/02
PB  - arXiv
DO  - 10.48550/arxiv.2609.01995
UR  - https://arxiv.org/abs/2609.01995
AB  - Context: Satellite mega-constellations generate Unintended Electro-Magnetic Radiation (UEMR) impacting low frequency radio astronomy. The Radio Regulations of the International Telecommunications Union Radiocommunication Sector (ITU-R) contain the basis for addressing UEMR, but enforcement mechanisms are absent. Aims: To adapt compatibility study methods based on satellite constellation simulations, in particular the Equivalent Power Flux-Density (EPFD) framework, to radio telescope measurements. Methods: We adapt the ITU-R EPFD calculation framework to measurement data obtained from all-sky interferometric imaging. We address the conceptual differences between forward-model EPFD calculations and measurement-based approaches. In particular, we consider low frequency systems, which are typically wide field-of-view and interferometric instruments. Results: For the first time, we demonstrate that all-sky interferometric observations enable a direct adaptation of the EPFD formalism to measurement data. We thus confirm previous estimations (Di Vruno et al. 2023) that the resulting measurement-based EPFD distributions exceed the radio astronomy interference threshold levels defined in Recommendation ITU-R RA.769-2 in 50-70% of samples. These exceedance fractions are well above the 2% single-system data-loss criterion in Recommendation ITU-R RA.1513-2. Expressed using the conventional 2% compatibility margin, the corresponding margins are negative, ranging from -18.6 to -16.3 dB, equivalent to a required uniform attenuation of 16.3-18.6 dB. Conclusions: Measurement-based implementations provide a practical pathway toward verification and long-term monitoring at low radio frequencies, which could form an important component of enforceability. We suggest instrumentation approaches to support measurement.
ER  -