A Roadmap towards a Space-based Radio Telescope for Ultra-Low Frequency Radio Astronomy
M.J. Bentum, M.K. Verma, R.T. Rajan, A.-J. Boonstra, C.J.M. Verhoeven,, E.K.A. Gill, A.J. van der Veen, H. Falcke, M. Klein Wolt, B. Monna, S., Engelen, J. Rotteveel, and L.I. Gurvits

TL;DR
This paper proposes a roadmap for a space-based ultra-low frequency radio telescope, OLFAR, utilizing a satellite swarm to explore the universe at frequencies below 30 MHz, overcoming Earth's ionospheric limitations.
Contribution
It introduces the OLFAR concept, outlining the technological, scientific, and programmatic challenges of deploying a satellite swarm for ultra-low frequency radio astronomy.
Findings
NCLE experiment launched in 2018 provides initial data.
Key technologies for satellite swarm deployment are identified.
The roadmap outlines steps towards a functional space-based radio telescope.
Abstract
The past two decades saw a renewed interest in low frequency radio astronomy, with a particular focus on frequencies above 30 MHz. However, at frequencies below 30 MHz, Earth-based observations are limited due to a combination of severe ionospheric distortions, almost full reflection of radio waves below 10 MHz, solar eruptions and human-made radio frequency interference (RFI). A space or Lunar-based ultra-low-frequency (or ultra-long-wavelength, ULW) array would suffer significantly less from these limitations and hence would open up the last, virtually unexplored frequency domain in the electromagnetic spectrum. A roadmap has been initiated in order to explore the opportunity of building a swarm of satellites to observe at the frequency band below 30 MHz. This roadmap, dubbed Orbiting Low Frequency Antennas for Radio Astronomy (OLFAR), presents a space-based ultra-low frequency radio…
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