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When to Use Fast Radio Bursts 3D Explorer - Best Sessions and Limits

Last reviewed: 2026-07-23

Open Fast Radio Bursts 3D Explorer when you want to see why a fast radio burst's dispersion sweep proves it travelled across intergalactic space, and to compare Lorimer Burst, FRB 121102, and FRB 180916.J0158+65 side by side by their published figures - not to run a dedispersion pipeline or watch a live CHIME data feed.

A dispersion-sweep lesson

A lesson starts by playing the Lorimer Burst first (the original 2007 discovery), then switching to FRB 121102 to see the same sweep shape repeat from the first confirmed repeating source, then FRB 180916.J0158+65 to read its 16.35-day activity cycle in the facts panel.

Sessions this explorer does not fit

Sessions this page does not fit are studying a rotating neutron star's steady lighthouse-beam timing - use the Neutron Star Pulsar 3D Explorer for that - or a magnetar's steady-state magnetic field strength - use the Magnetar 3D Explorer. Walk the controls in the step-by-step guide.

← Back to Space 3D

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Last updated: Jul 23, 2026

Reviewed by the Free Tool Online editorial team · Tested in the current versions of Chrome, Firefox, Safari, and Edge before publishing. No account is needed to use any tool. Report a bug - we triage within 72 hours. · Last refreshed April 2026.

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