A roadmap towards a space-based radio telescope for ultra-low frequency radio astronomy

M.J. Bentum (Corresponding author), 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, L.I. Gurvits

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Uittreksel

The past two decades have witnessed a renewed interest in low frequency radio astronomy, with a particular focus on frequencies above 30 MHz e.g., LOFAR (LOw Frequency ARray) in the Netherlands and its European extension ILT, the International LOFAR Telescope. 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 the radio frequency interference (RFI) of human-made signals. Moreover, there are interesting scientific processes which naturally occur at these low frequencies. A space or Lunar-based ultra-low-frequency (also referred to as ultra-long-wavelength, ULW) radio 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 by astronomers and researchers in the Netherlands 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), a space-based ultra-low frequency radio telescope that will explore the Universe's so-called dark ages, map the interstellar medium, and study planetary and solar bursts in the solar system and search them in other planetary systems. Such a radio astronomy system will comprise of a swarm of hundreds to thousands of satellites, working together as a single aperture synthesis instrument deployed sufficiently far away from Earth to avoid terrestrial RFI. The OLFAR telescope is a novel and complex system, requiring yet to be proven engineering solutions. Therefore, a number of key technologies are still required to be developed and proven. The first step in this roadmap is the NCLE (Netherlands China Low Frequency Explorer) experiment, which was launched in May 2018 on the Chinese Chang'e 4 mission. The NCLE payload consists of a three monopole antenna system for low frequency observations, from which the first data stream is expected in the second half of 2019, which will provide important feedback for future science and technology opportunities. In this paper, the roadmap towards OLFAR, a brief overview of the science opportunities, and the technological and programmatic challenges of the mission are presented.

Originele taal-2Engels
Pagina's (van-tot)856-867
Aantal pagina's12
TijdschriftAdvances in Space Research
Volume65
Nummer van het tijdschrift2
Vroegere onlinedatum23 sep 2019
DOI's
StatusGepubliceerd - 15 jan 2020

Vingerafdruk

Radio astronomy
Radio telescopes
extremely low frequencies
radio astronomy
radio telescopes
astronomy
radio
low frequencies
Netherlands
Antennas
antenna
Telescopes
radio frequency interference
Earth (planet)
antennas
Satellites
Monopole antennas
Radio waves
Solar system
China

Citeer dit

Bentum, M. J., Verma, M. K., Rajan, R. T., Boonstra, A. J., Verhoeven, C. J. M., Gill, E. K. A., ... Gurvits, L. I. (2020). A roadmap towards a space-based radio telescope for ultra-low frequency radio astronomy. Advances in Space Research, 65(2), 856-867. https://doi.org/10.1016/j.asr.2019.09.007
Bentum, M.J. ; Verma, M.K. ; Rajan, R.T. ; Boonstra, A.J. ; Verhoeven, C.J.M. ; Gill, E.K.A. ; van der Veen, A.J. ; Falcke, H. ; Wolt, M. Klein ; Monna, B. ; Engelen, S. ; Rotteveel, J. ; Gurvits, L.I. / A roadmap towards a space-based radio telescope for ultra-low frequency radio astronomy. In: Advances in Space Research. 2020 ; Vol. 65, Nr. 2. blz. 856-867.
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abstract = "The past two decades have witnessed a renewed interest in low frequency radio astronomy, with a particular focus on frequencies above 30 MHz e.g., LOFAR (LOw Frequency ARray) in the Netherlands and its European extension ILT, the International LOFAR Telescope. 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 the radio frequency interference (RFI) of human-made signals. Moreover, there are interesting scientific processes which naturally occur at these low frequencies. A space or Lunar-based ultra-low-frequency (also referred to as ultra-long-wavelength, ULW) radio 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 by astronomers and researchers in the Netherlands 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), a space-based ultra-low frequency radio telescope that will explore the Universe's so-called dark ages, map the interstellar medium, and study planetary and solar bursts in the solar system and search them in other planetary systems. Such a radio astronomy system will comprise of a swarm of hundreds to thousands of satellites, working together as a single aperture synthesis instrument deployed sufficiently far away from Earth to avoid terrestrial RFI. The OLFAR telescope is a novel and complex system, requiring yet to be proven engineering solutions. Therefore, a number of key technologies are still required to be developed and proven. The first step in this roadmap is the NCLE (Netherlands China Low Frequency Explorer) experiment, which was launched in May 2018 on the Chinese Chang'e 4 mission. The NCLE payload consists of a three monopole antenna system for low frequency observations, from which the first data stream is expected in the second half of 2019, which will provide important feedback for future science and technology opportunities. In this paper, the roadmap towards OLFAR, a brief overview of the science opportunities, and the technological and programmatic challenges of the mission are presented.",
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Bentum, MJ, Verma, MK, Rajan, RT, Boonstra, AJ, Verhoeven, CJM, Gill, EKA, van der Veen, AJ, Falcke, H, Wolt, MK, Monna, B, Engelen, S, Rotteveel, J & Gurvits, LI 2020, 'A roadmap towards a space-based radio telescope for ultra-low frequency radio astronomy', Advances in Space Research, vol. 65, nr. 2, blz. 856-867. https://doi.org/10.1016/j.asr.2019.09.007

A roadmap towards a space-based radio telescope for ultra-low frequency radio astronomy. / Bentum, M.J. (Corresponding author); Verma, M.K.; Rajan, R.T.; Boonstra, A.J.; Verhoeven, C.J.M.; Gill, E.K.A.; van der Veen, A.J.; Falcke, H.; Wolt, M. Klein; Monna, B.; Engelen, S.; Rotteveel, J.; Gurvits, L.I.

In: Advances in Space Research, Vol. 65, Nr. 2, 15.01.2020, blz. 856-867.

Onderzoeksoutput: Bijdrage aan tijdschriftTijdschriftartikelAcademicpeer review

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AU - Bentum, M.J.

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AU - Rajan, R.T.

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AU - Verhoeven, C.J.M.

AU - Gill, E.K.A.

AU - van der Veen, A.J.

AU - Falcke, H.

AU - Wolt, M. Klein

AU - Monna, B.

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AU - Rotteveel, J.

AU - Gurvits, L.I.

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N2 - The past two decades have witnessed a renewed interest in low frequency radio astronomy, with a particular focus on frequencies above 30 MHz e.g., LOFAR (LOw Frequency ARray) in the Netherlands and its European extension ILT, the International LOFAR Telescope. 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 the radio frequency interference (RFI) of human-made signals. Moreover, there are interesting scientific processes which naturally occur at these low frequencies. A space or Lunar-based ultra-low-frequency (also referred to as ultra-long-wavelength, ULW) radio 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 by astronomers and researchers in the Netherlands 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), a space-based ultra-low frequency radio telescope that will explore the Universe's so-called dark ages, map the interstellar medium, and study planetary and solar bursts in the solar system and search them in other planetary systems. Such a radio astronomy system will comprise of a swarm of hundreds to thousands of satellites, working together as a single aperture synthesis instrument deployed sufficiently far away from Earth to avoid terrestrial RFI. The OLFAR telescope is a novel and complex system, requiring yet to be proven engineering solutions. Therefore, a number of key technologies are still required to be developed and proven. The first step in this roadmap is the NCLE (Netherlands China Low Frequency Explorer) experiment, which was launched in May 2018 on the Chinese Chang'e 4 mission. The NCLE payload consists of a three monopole antenna system for low frequency observations, from which the first data stream is expected in the second half of 2019, which will provide important feedback for future science and technology opportunities. In this paper, the roadmap towards OLFAR, a brief overview of the science opportunities, and the technological and programmatic challenges of the mission are presented.

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