Articles | Volume 38, issue 4
Ann. Geophys., 38, 861–879, 2020

Special issue: Special Issue on the joint 19th International EISCAT Symposium...

Ann. Geophys., 38, 861–879, 2020

Regular paper 15 Jul 2020

Regular paper | 15 Jul 2020

Radar observability of near-Earth objects using EISCAT 3D

Daniel Kastinen et al.


Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to technical corrections (15 Jun 2020) by Petr Pisoft
Short summary
We have applied three different methods to examine the observability, both tracking and discovery, of near-Earth objects (NEOs) by the EISCAT 3D radar system currently under construction. There are, to our knowledge, no previous studies on the expected discovery rates of NEOs using radar systems. We show that it is feasible to regularly track NEOs and mini-moons. We also show it is possible to discover new NEOs and mini-moons with EISCAT 3D, something never before done with radar systems.