Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 56 min ago
PreprintCC BY 4.0arXiv

A Study of the 30 May 2026 Meteor Event Employing Data from Raspberry Boom Infrasound Sensors in the Boston Area

Abstract

Infrasound signals of one and a half cycles of a 0.4 Hz pressure pulse were detected from the 30 May 2026 meteor over Cape Cod Bay at several university and private Raspberry Boom sensors in the Greater Boston area. Our analyses of these signals demonstrate the ability to define directivity to the source of the event based on differences in the timing of the signals, to determine its identity and location by analysis of the relationship between event distance and sensor event timing, and event acoustical power by the infrasonic pressures measured at the sensor sites. The infrasound event is determined to be the atmospheric fireball blast at between 40 and 50 km in altitude with acoustic energy on the order of 5% to 14% of the total fireball energy.

Related

  1. Revisiting the 2014 Camelopardalids Outburst using a Meteor Radar Chain in the Northern Hemisphere
    Maolin Lu, Wen Yi, Xianghui Xue +7
    The Astrophysical JournalPeer-reviewedCC BY 4.0Full textSolar & stellar physicsIOP/AASCrossref
  2. The role of source geometry and atmospheric propagation in global bolide infrasound detectability
    Miro Ronac Giannone, Elizabeth A. Silber
    IcarusPeer-reviewedLicence not statedFull text6 citedPlanetary science & exoplanetsOpenAlex
  3. Cross-Validation of Infrasound Detections and Fireball Observations from the Global Fireball Observatory
    Iona Clemente, Eleanor K. Sansom, Hadrien A. R. Devillepoix +6
    arXivPreprintCC BY 4.0Full textInstrumentation & methodsPlanetary science & exoplanetsarXiv
  4. Radar and Infrasound Observations of the 2026 May 30 Cape Cod Bay Superbolide
    Juha Vierinen, Ryan Volz, Marc Fries +10
    arXivPreprintCC BY 4.0Full textInstrumentation & methodsPlanetary science & exoplanetsarXiv
  5. Period-Inverted Blast-Radius Normalization for a Non-Ablating Hypersonic Reentry Source Using OSIRIS-REx Capsule Infrasound
    Elizabeth A. Silber
    arXivPreprintCC BY 4.0Full textPlanetary science & exoplanetsAtmospheric science & meteorologyarXiv
BibTeX
@misc{africk2026study,
  title = {{A Study of the 30 May 2026 Meteor Event Employing Data from Raspberry Boom Infrasound Sensors in the Boston Area}},
  author = {S. Africk and A. Loeb},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.31742},
  eprint = {2610.31742},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.31742},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - A Study of the 30 May 2026 Meteor Event Employing Data from Raspberry Boom Infrasound Sensors in the Boston Area
AU  - S. Africk
AU  - A. Loeb
PY  - 2026
DA  - 2026/10/22
PB  - arXiv
DO  - 10.48550/arxiv.2610.31742
UR  - https://arxiv.org/abs/2610.31742
AB  - Infrasound signals of one and a half cycles of a 0.4 Hz pressure pulse were detected from the 30 May 2026 meteor over Cape Cod Bay at several university and private Raspberry Boom sensors in the Greater Boston area. Our analyses of these signals demonstrate the ability to define directivity to the source of the event based on differences in the timing of the signals, to determine its identity and location by analysis of the relationship between event distance and sensor event timing, and event acoustical power by the infrasonic pressures measured at the sensor sites. The infrasound event is determined to be the atmospheric fireball blast at between 40 and 50 km in altitude with acoustic energy on the order of 5% to 14% of the total fireball energy.
ER  -