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dc.contributor.authorMaterna, Kathryn
dc.contributor.authorBürgmann, Roland
dc.contributor.authorLindsay, Danielle
dc.contributor.authorBilham, Roger
dc.contributor.authorHerring, Thomas
dc.contributor.authorCrowell, Brendan
dc.contributor.authorSzeliga, Walter
dc.date.accessioned2026-04-27T21:46:24Z
dc.date.available2026-04-27T21:46:24Z
dc.date.issued2024-06-19
dc.identifier.urihttps://hdl.handle.net/1721.1/165703
dc.descriptionArticle relates to: Vavra, E. J., Fialko, Y., Rockwell, T., Bilham, R., Štěpančíková, P., Stemberk, J., et al. (2024). Characteristic slow-slip events on the Superstition Hills Fault, Southern California. Geophysical Research Letters, 51, e2023GL107244. https://doi.org/10.1029/2023GL107244en_US
dc.description.abstractShallow creep events provide opportunities to understand the mechanical properties and behavior of faults. However, due to physical limitations observing creep events, the precise spatio‐temporal evolution of slip during creep events is not well understood. In 2023, the Superstition Hills and Imperial faults in California each experienced centimeter‐scale slip events that were captured in unprecedented detail by satellite radar, sub‐daily Global Navigation Satellite Systems, and creepmeters. In both cases, the slip propagated along the fault over 2–3 weeks. The Superstition Hills event propagated bilaterally away from its initiation point at average velocities of ∼9 km/day, but propagation velocities were locally much higher. The ruptures were consistent with slip from tens of meters to ∼2 km depths. These slowly propagating events reveal that the shallow crust of the Imperial Valley does not obey purely velocity‐strengthening or velocity‐weakening rate‐and‐state friction, but instead requires the consideration of fault heterogeneity or fault‐frictional behaviors such as dilatant strengthening.en_US
dc.language.isoen
dc.publisherAmerican Geophysical Unionen_US
dc.relation.isversionof10.1029/2023gl108089en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceAmerican Geophysical Unionen_US
dc.titleShallow Slow Slip Events in the Imperial Valley With Along‐Strike Propagationen_US
dc.typeArticleen_US
dc.identifier.citationMaterna, K., Bürgmann, R., Lindsay, D., Bilham, R., Herring, T., Crowell, B., & Szeliga, W. (2024). Shallow slow slip events in the Imperial Valley with along-strike propagation. Geophysical Research Letters, 51, e2023GL108089.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Geology and Geophysicsen_US
dc.relation.journalGeophysical Research Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2026-04-27T21:41:03Z
dspace.orderedauthorsMaterna, K; Bürgmann, R; Lindsay, D; Bilham, R; Herring, T; Crowell, B; Szeliga, Wen_US
dspace.date.submission2026-04-27T21:41:05Z
mit.journal.volume51en_US
mit.journal.issue12en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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