NOIRE Study Report: Towards a Low Frequency Radio Interferometer in Space
arXiv:1710.10245 · doi:10.1109/AERO.2018.8396742
Abstract
Ground based low frequency radio interferometers have been developed in the last decade and are providing the scientific community with high quality observations. Conversely, current radioastronomy instruments in space have a poor angular resolution with single point observation systems. Improving the observation capabilities of the low frequency range (a few kHz to 100 MHz) requires to go to space and to set up a space based network of antenna that can be used as an interferometer. We present the outcome of the NOIRE (Nanosatellites pour un Observatoire Interférométrique Radio dans l'Espace / Nanosatellites for a Radio Interferometer Observatory in Space) study which assessed, with help of CNES PASO (Architecture Platform for Orbital Systems is CNES' cross-disciplinary team in charge of early mission and concept studies), the feasibility of a swarm of nanosatellites dedicated to a low frequency radio observatory. With such a platform, space system engineering and instrument development must be studied as a whole: each node is a sensor and all sensors must be used together to obtain a measurement. The study was conducted on the following topics: system principle and concept (swarm, node homogeneity); Space and time management (ranging, clock synchronization); Orbitography (Moon orbit, Lagrange point options); Telecommunication (between nodes and with ground) and networking; Measurements and processing; Propulsion; Power; Electromagnetic compatibility. No strong show-stopper was identified during the preliminary study, although the concept is not yet ready. Several further studies and milestones are identified. The NOIRE team will collaborate with international teams to try and build this next generation of space systems.
arXiv commentSubmitted to IEEEAeroconf 2018 proceedings
References in corpus (16)
- LOFAR: The LOw-Frequency ARray
- 21-cm cosmology
- Revisiting the radio interferometer measurement equation. I. A full-sky Jones formalism
- Probing the First Stars and Black Holes in the Early Universe with the Dark Ages Radio Explorer (DARE)
- Observing Neutral Hydrogen Above Redshift 6: The "Global" Perspective
- Science with a lunar low-frequency array: from the dark ages of the Universe to nearby exoplanets
- Revisiting the radio interferometer measurement equation. II. Calibration and direction-dependent effects
- LOFAR Sparse Image Reconstruction
- LOFAR tied-array imaging of Type III solar radio bursts
- Imaging Jupiter's radiation belts down to 127 MHz with LOFAR
- Spherical Harmonic Analyses of Intensity Mapping Power Spectra
- Revisiting the radio interferometer measurement equation. III. Addressing direction-dependent effects in 21 cm WSRT observations of 3C 147
- Statistical Survey of Type III Radio Bursts at Long Wavelengths Observed by the Solar TErrestrial RElations Observatory (STEREO)/Waves Instruments: Goniopolarimetric Properties and Radio Source Locations
- Spherical 3D Isotropic Wavelets
- Sparse representations and convex optimization as tools for LOFAR radio interferometric imaging
- Revisiting the radio interferometer measurement equation. IV. A generalized tensor formalism
Cited by in corpus (5)
- A Roadmap towards a Space-based Radio Telescope for Ultra-Low Frequency Radio Astronomy
- Discovering the Sky at the Longest wavelengths with a lunar orbit array
- The future of astronomy with small satellites
- A Space-based Decametric Wavelength Radio Telescope Concept
- Communication protocol for a satellite-swarm interferometer