Improved Sensitivity for Space Domain Awareness Observations with the Murchison Widefield Array
arXiv:2205.05868 · doi:10.1016/j.asr.2022.05.013
Abstract
Our previously reported survey of the Low Earth Orbit (LEO) environment using the Murchison Widefield Array (MWA) detected over 70 unique Resident Space Objects (RSOs) over multiple passes, from 20 hours of observations in passive radar mode. In this paper, we extend this work by demonstrating two methods that improve the detection sensitivity of the system. The first method, called shift-stacking, increases the statistical significance of faint RSO signals through the spatially coherent integration of the reflected signal along the RSO's trajectory across the sky. This method was tested on the observations used during our previous blind survey, and we obtained a increase in the total number of detections. The second method re-focuses the MWA to the near-field RSO's position (post-observation), by applying a complex phase correction to each visibility to account for the curved wave-front. The method was tested successfully on an MWA extended array observation of an ISS pass. However, the method is currently limited by signal de-coherence on the long-baselines (due to the hardware constraints of the current correlator). We discuss the sensitivity improvement for RSO detections we expect from the MWA Phase 3 correlator upgrade. We conclude the paper by briefly commenting on future dedicated Space Domain Awareness (SDA) systems that will incorporate MWA technologies.
arXiv commentAccepted in Advances in Space Research. 16 pages, 10 figures, and 1 Table
References in corpus (17)
- Astropy: A Community Python Package for Astronomy
- The NumPy array: a structure for efficient numerical computation
- The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
- The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
- WSClean: an implementation of a fast, generic wide-field imager for radio astronomy
- GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey I: A low-frequency extragalactic catalogue
- The Size Distribution of Trans-Neptunian Bodies
- An optimized algorithm for multi-scale wideband deconvolution of radio astronomical images
- The Phase II Murchison Widefield Array: Design Overview
- Parametrising Epoch of Reionization foregrounds: A deep survey of low-frequency point-source spectra with the MWA
- The High Time and Frequency Resolution Capabilities of the Murchison Widefield Array
- On the detection and tracking of space debris using the Murchison Widefield Array. I. Simulations and test observations demonstrate feasibility
- A survey of spatially and temporally resolved radio frequency interference in the FM band at the Murchison Radio-astronomy Observatory
- Limits on radio emission from meteors using the MWA
- The Development of Non-coherent Passive Radar Techniques for Space Situational Awareness with the Murchison Widefield Array
- A Low Frequency Blind Survey of the Low Earth Orbit Environment using Non-Coherent Passive Radar with the Murchison Widefield Array
- A Deep Search for Additional Satellites around the Dwarf Planet Haumea
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