A numerical assessment of simple airblast models of impact airbursts

File Description SizeFormat 
Collins_et_al-2017-Meteoritics_&_Planetary_Science.pdfPublished version1.37 MBAdobe PDFDownload
Title: A numerical assessment of simple airblast models of impact airbursts
Author(s): Collins, GS
Lynch, E
McAdam, R
Davison, TM
Item Type: Journal Article
Abstract: Asteroids and comets 10–100 m in size that collide with Earth disrupt dramatically in the atmosphere with an explosive transfer of energy, caused by extreme air drag. Such airbursts produce a strong blastwave that radiates from the meteoroid's trajectory and can cause damage on the surface. An established technique for predicting airburst blastwave damage is to treat the airburst as a static source of energy and to extrapolate empirical results of nuclear explosion tests using an energy-based scaling approach. Here we compare this approach to two more complex models using the iSALE shock physics code. We consider a moving-source airburst model where the meteoroid's energy is partitioned as two-thirds internal energy and one-third kinetic energy at the burst altitude, and a model in which energy is deposited into the atmosphere along the meteoroid's trajectory based on the pancake model of meteoroid disruption. To justify use of the pancake model, we show that it provides a good fit to the inferred energy release of the 2013 Chelyabinsk fireball. Predicted overpressures from all three models are broadly consistent at radial distances from ground zero that exceed three times the burst height. At smaller radial distances, the moving-source model predicts overpressures two times greater than the static-source model, whereas the cylindrical line-source model based on the pancake model predicts overpressures two times lower than the static-source model. Given other uncertainties associated with airblast damage predictions, the static-source approach provides an adequate approximation of the azimuthally averaged airblast for probabilistic hazard assessment.
Publication Date: 17-Apr-2017
Date of Acceptance: 11-Mar-2017
URI: http://hdl.handle.net/10044/1/45588
DOI: https://dx.doi.org/10.1111/maps.12873
ISSN: 1086-9379
Publisher: Wiley
Start Page: 1542
End Page: 1560
Journal / Book Title: Meteoritics & Planetary Science
Volume: 52
Issue: 8
Copyright Statement: © 2017 The Authors. Meteoritics & Planetary Science published by Wiley Periodicals, Inc. on behalf of The Meteoritical Society. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
Sponsor/Funder: Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Funder's Grant Number: ST/J001260/1
Keywords: Science & Technology
Physical Sciences
Geochemistry & Geophysics
0201 Astronomical And Space Sciences
0402 Geochemistry
0403 Geology
Geochemistry & Geophysics
Publication Status: Published
Appears in Collections:Faculty of Engineering
Earth Science and Engineering

Items in Spiral are protected by copyright, with all rights reserved, unless otherwise indicated.

Creative Commons