Publication

Measurement of Satellite Emissions in the 1400 MHz to 1427 MHz Radio Astronomy Protected Band

Publication Info

Publication

2026 IEEE International Symposium on Spectrum Innovation (DySPAN)

Abstract

We present dual polarization and flux calibrated measurements of Radio Frequency Interference (RFI) in the radio astronomy protected band between 1400 and 1427 MHz. These observations suggest that a subset of satellites observed likely produce ground level RFI in excess of ITU thresholds for interference to radio astronomy. They also highlight the effects and challenges associated with modeling and measuring RFI. Such challenges include limitations in measurement timing from errors in predicted satellite orbits using publicly available ephemeris information, the difficulty of distinguishing individual satellites in an increasingly crowded orbital environment, dynamic satellite platform behaviors such as beamforming, and contributions from other signals reflecting off of the satellites being observed.

CiTation

D. Sheen, S. Thé and F. D. Lind, "Measurement of Satellite Emissions in the 1400 MHz to 1427 MHz Radio Astronomy Protected Band," 2026 IEEE International Symposium on Spectrum Innovation (DySPAN), Washington, DC, USA, 2026, pp. 1-8, doi: 10.1109/DySPAN69846.2026.11571115.

Contributors

Info

Date:
June 24, 2026
Type:
Conference Paper
DOI:
10.1109/DySPAN69846.2026.11571115