Seismic Travel Time Models T1-01 Thu 09:10 1D Seismic Velocity Model - - PowerPoint PPT Presentation

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Seismic Travel Time Models T1-01 Thu 09:10 1D Seismic Velocity Model - - PowerPoint PPT Presentation

Seismic Travel Time Models T1-01 Thu 09:10 1D Seismic Velocity Model with GT5 Events in Brazil and Tests of Crustal Thickness Corrections to Improve the RSTT Model for South America Marcelo Assumpo; Elder Marco; Jos Roberto Barbosa


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SLIDE 1

1D Seismic Velocity Model with GT5 Events in Brazil and Tests of Crustal Thickness Corrections to Improve the RSTT Model for South America

Marcelo Assumpção; Elder Marco; José Roberto Barbosa Geophysics Dept. University of São Paulo

Seismic Travel Time Models T1-01 Thu 09:10

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SLIDE 2

Status report on the RSTT project in Brazil

  • GT5 and Pseudo-GT

events in Brazil

  • Travel time database
  • Test of Crustal

Corrections

  • Proposed 1D

reference model for Brazil

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SLIDE 3

Brazil Network: 70 stations installed by four institutions

Project funded by

USP – São Paulo Rio de Janeiro Natal UnB – Brasília

LPAZ SAML PTGA RCBR CPUP BDFB SPB

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SLIDE 4

Feng et al., 2007; Assumpção et al., 2013

Lithospheric mantle in Brazil has higher than average velocity ~5% higher velocity,

  • n average.

But also, significant lateral variation. 3D models are needed to improve locations.

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SLIDE 5

Travel time database

distance, km

T – X/8.5

IASP91 Herrin

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SLIDE 6

Example of GT5 event: hypocenter with local network (± 1km).

Chimpliganond et al., 2010

Itacarambi,

MG, Mag=4,7 09-Dec-2007 USGS

NW SE

hypodd

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SLIDE 7

Pseudo GT: known hypocenter from aftershocks Origin time estimated with teleseismic stations (IASP91)

Porto dos Gauchos, MT, mag=5,0 23-Mar-2005 Barros et al., 2009

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SLIDE 8

Aseismic country – few GT events…

none up to 2012; four available now at ISC

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SLIDE 9

Residuals for Herrin’s (1968) model. Travel times corrected to 0 depth hypocenter.

distance, km Res = Observ-Model (sec)

No Crustal correction Residuals (s)

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SLIDE 10

Correcting for crustal thickness variation

Assumpção et al.(2013)

Travel times corrected to 40 km depth, at both epicenter and station.

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SLIDE 11

Residuals for Herrin’s (1968) model. Travel times corrected to 0 depth

distance, km Res = Observ-Model (sec)

No Crustal correction

Res = Observ-Model (sec)

Corrected to 40 km Crust

s s

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SLIDE 12

Residuals for RSTT model

(currently CRUST2.0 for S.America)

Res = Observ-Model (sec) distance, km

residual, sec

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SLIDE 13

Best 1D model for Brazil (New BR): Pc=6.1 km/s

H= 42 km

Pn= 8.1 km/s gradient = 1.57 m/s/km

T – X/8.2

GT5 pGT

distance, km Herrin BR model

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SLIDE 14

Fast and Slow Paths for New BR Model

FAST SLOW

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SLIDE 15

Fast and Slow Paths for New BR Model S-wave anomaly at 100 km depth

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Conclusions - 1

Crustal correction is relevant but reduces scatter only slightly

No correction Corrected

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Conclusions - 2

Preliminary RSTT (CRUST2.0) is better than Herrin and similar to new 1D BR model

residual, sec

1D Herrin, crustal corrected 3D

residual, sec

1D New BR crustal- corrected

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SLIDE 18

Conclusions - 3

  • Mantle variation is

more important than crustal correction,

  • Next steps:

a) Insert new crustal model into RSTT b) If enough data, do a tomography inversion (?)

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SLIDE 19

Thank you Vielen Dank!

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SLIDE 20

Annex

Fast, slow paths wrt New BR model P-wave anomaly at 150 km depth