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The 2023 May 20 Queensland Superbolide: Multimodal Observations from Atmospheric Entry to Postdisruption Dust Cloud

  • Authors: Elizabeth A. Silber, Miro Ronac Giannone, Hadrien A. R. Devillepoix, Mark Boslough, Iona Clemente, Loring P. Schaible, Denis Vida, Damir Šegon, Yleana Ceballos, Eleanor K. Sansom, Leigh Tyers, Seamus L. Anderson, Hany S. Elbehiri, Masa-yuki Yamamoto, Claus Hetzer, Katherine R. Bermingham, Hely C. Branco, Hope Tornabene, Logan T. Scamfer, Randy Longenbaugh, Yasuhiro Nishikawa, Vedant Sawal

Elizabeth A. Silber et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 5.

Cardinal output for station I39PW. The panels provide an analysis of the signal’s characteristics over time. The vertical dashed lines (red, green, and blue) represent theoretical or predicted arrival windows based on different atmospheric propagation waveguides. Panels from top to bottom represent timeseries (the bandpass-filtered—0.05–3 Hz—waveform, showing a high-amplitude arrival between 4000 and 5000 s); back azimuth deviation (the consistency of the signal’s arrival direction; the focused cluster indicates a coherent point source); trace velocity; and semblance (a correlation metric where higher values—darker regions—identify the arrival of a coherent, nonrandom signal).

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