Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in...

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Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes Magnitude-scaling model Assumes Mw alone can explain large-magnitude scaling of ground motion Aspect ratio-scaling model: Assumes Mw and aspect ratio (AR) are needed to explain large-magnitude scaling of ground motion
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Transcript of Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in...

Page 1: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

Campbell-Bozorgnia

• Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes

• Magnitude-scaling model– Assumes Mw alone can explain large-magnitude

scaling of ground motion

• Aspect ratio-scaling model:– Assumes Mw and aspect ratio (AR) are needed to

explain large-magnitude scaling of ground motion

Page 2: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

5.0 5.5 6.0 6.5 7.0 7.5 8.0Moment Magnitude

10-1

100

101

102

Asp

ect

Rat

io (

L/W

)STRIKE SLIP

N. Cal. - Type ASo. Cal. - Type ANGAWC94 (W = 10)HB02 (W = 10)EL02 (W = 10)

Page 3: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

5.0 5.5 6.0 6.5 7.0 7.5 8.0Moment Magnitude

10-1

100

101

102

Asp

ect

Rat

io (

L/W

)STRIKE SLIP

N. Cal. - Type ASo. Cal. - Type ANGAWC94 (W = 15)HB02 (W = 15)EL02 (W = 15)

Page 4: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

5.0 5.5 6.0 6.5 7.0 7.5 8.0Moment Magnitude

10-1

100

101

102

Asp

ect

Rat

io (

L/W

)STRIKE SLIP

N. Cal. - Type ASo. Cal. - Type ANGAWC94 (W = 20)HB02 (W = 20)EL02 (W = 20)

Page 5: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

Magnitude-Scaling Model

Page 6: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

PGA, All Faults

4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0M

-3

-2

-1

0

1

2

3R

ES

IDU

AL

Page 7: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

PGA, All Faults

0 2 4 6 8 10 12 14LW

-3

-2

-1

0

1

2

3R

ES

IDU

AL

Page 8: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

With Surface Slip, Strike-Slip Faults

4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0M

-3

-2

-1

0

1

2

3R

ES

IDU

AL

Page 9: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

PGA, W/O Surface Slip, Strike-Slip Faults

4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0M

-3

-2

-1

0

1

2

3R

ES

IDU

AL

Page 10: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

Atten373 (Model 1), Resid stages 1 & 2 (combined), PGA

0 10 20 30 40 50 60RRUP

-3

-2

-1

0

1

2

3

RE

S1_

2_P

GA

Page 11: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

Atten373 (Model 1), Resid stages 1 & 2 (combined), PGA

4 5 6 7 8M

-3

-2

-1

0

1

2

3

RE

S1_

2_P

GA

Page 12: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

1 10 100Horizontal Distance to Fault (km)

10-2

10-1

100A

ccel

erat

ion

(g

)PGA

Campbell & Bozorgnia (2003)Campbell & Bozorgnia (Prelim NGA)

PARAMETERS:

M = 6.5, 7.0, 7.5, 8.0

Fault = Strike Slip

Dip = 90

Vs30 = 600 (C)

Page 13: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0

Moment Magnitude

10-2

10-1

100A

ccel

erat

ion

(g

)PGA

Campbell & Bozorgnia (2003)Campbell & Bozorgnia (Prelim NGA)

PARAMETERS:

Rjb = 0, 5, 10, 25

Fault = Strike Slip

Dip = 90

Vs30 = 270 (D)

Page 14: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

0 10 20 30 40 50 60 70 80 90

Dip (degrees)

0.0

0.4

0.8

1.2

1.6

2.0

Fau

ltin

g F

acto

rSTYLE OF FAULTING

PGA - ReversePSA (1s) - ReversePGA - NormalPSA (1s) - Normal

Page 15: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

Aspect Ratio-Scaling Model

Page 16: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

PGA, All Faults

4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0M

-3

-2

-1

0

1

2

3

RE

SID

UA

L

Page 17: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

PGA, All Faults

0 2 4 6 8 10 12 14LW

-3

-2

-1

0

1

2

3R

ES

IDU

AL

Page 18: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

PGA, With Surface Slip, Strike-Slip Faults

4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0M

-3

-2

-1

0

1

2

3

RE

SID

UA

L

Page 19: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

PGA, W/O Surface Slip, Strike-Slip Faults

4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0M

-3

-2

-1

0

1

2

3

RE

SID

UA

L

Page 20: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0

Moment Magnitude

10-2

10-1

100

Acc

eler

atio

n (

g)

PGA

Campbell & Bozorgnia (NGA AR-Scaling)Campbell & Bozorgnia (NGA M-Scaling)

PARAMETERS:

Rjb = 0, 5, 10, 25

Fault = Strike Slip

Dip = 90

Vs30 = 600 (C)

Page 21: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0

Moment Magnitude

10-2

10-1

100

Ac

ce

lera

tio

n (

g)

PGA

Campbell & Bozorgnia (NGA AR-Scaling)Campbell & Bozorgnia (NGA M-Scaling)

PARAMETERS:

Rjb = 0, 5, 10, 25

Fault = Strike Slip

Dip = 90, W = 20

Vs30 = 600 (C)

Page 22: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

Basin Effects: Influence of Depth to

Vs = 1.5 km/sec

Page 23: Campbell-Bozorgnia Two candidate models are currently being considered to capture the change in magnitude scaling of ground motion at large magnitudes.

0 1000 2000 3000 4000Z1_5

-3

-2

-1

0

1

2R

ES

1_2 _

T1