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3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault system Andrea Bistacchi , Matteo Massironi & Luca Menegon

3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

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Page 1: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault system

Andrea Bistacchi, Matteo Massironi & Luca Menegon

Page 2: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

1. How to build a computer model of fault-zone architecture?to model geometry and properties

topology of the model should reflect fault-zone architecture

geomodelling technology from the oil industry gOcadgeom

odel

ling

> overview

Page 3: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

1. How to build a computer model of fault-zone architecture?need to model geometry and propertiestopology of the model should reflect fault-zone architecture geomodelling technology from the oil industry gOcad

2. Case studied: the Pusteria and Sprechenstein-Mules fault systemdataset: field geology and boreholes (from a deep tunnelling project)dextral (reverse) fault system with contractional stepovers

PF

-SM

F s

yste

mge

omod

ellin

g> overview

borehole data: > 2000 mcontinuous core and geophysical

log data across the fault zone

contractional stepover

Page 4: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> overview

1. How to build a computer model of fault-zone architecture?

need to model geometry and properties

topology of the model should reflect fault-zone architecture

geomodelling technology from the oil industry gOcad

2. Case studied: the Pusteria and Sprechenstein-Mules fault system

dataset: field geology and boreholes from a tunnelling project

strike slip fault system with contractional stepovers

3. Why a computer model of fault-zone architecture could be useful?visualization, understand complex structures, …

output realistic quantitative geometry and properties to mechanical models, fluid flow models, etc.

geom

odel

ling

PF

-SM

F s

yste

mco

nclu

sion

Page 5: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> how to build a computer model of fault-zone architecture?

gOcad topology and interpolation (CAD and geostats coupled)

PF

-SM

F s

yste

mco

nclu

sion

geom

odel

ling

[Mallet, 2002]

n functions φn(α), ∀ α∈Ω

graph Ģ(Ω,N) linear constrains C

discrete model Mn(Ω,N,φ,C)

Page 6: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

P(A)

A

> how to build a computer model of fault-zone architecture?

gOcad topology and interpolation (CAD and geostats coupled)

PF

-SM

F s

yste

mco

nclu

sion

geom

odel

ling

discrete model Mn(Ω,N,φ,C)

n functions φn(α), ∀ α∈Ω

graph Ģ(Ω,N) linear constrains C

topology of a natural object A is approximated using a cellular partition model P(A) based on the GMaps algebraic structure

hierarchical embedded objects lines (n=1), surfaces (n=2), solids (n=3) [Mallet, 2002]

nodes neighborhood

Page 7: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> how to build a computer model of fault-zone architecture?

gOcad topology and interpolation (CAD and geostats coupled)

PF

-SM

F s

yste

mco

nclu

sion

geom

odel

ling

discrete model Mn(Ω,N,φ,C)

n functions φn(α), ∀ α∈Ω

graph Ģ(Ω,N) linear constrains C

first three components of φn(α) define spatial coordinates at all nodes α of the discrete model: φx(α), φy(α), φz(α)

other n-3 components define any other continuousor categorical property: attitude of a surface (gradient), degree of fracturing, porosity, seismic impedance, density, lithology, age, etc.

any property can be calculated at any point by linear interpolation ( similar to FEM mesh) [Mallet, 2002]

Page 8: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> how to build a computer model of fault-zone architecture?

gOcad topology and interpolation (CAD and geostats coupled)

PF

-SM

F s

yste

mco

nclu

sion

geom

odel

ling

discrete model Mn(Ω,N,φ,C)

n functions φn(α), ∀ α∈Ω

graph Ģ(Ω,N) linear constrains C

property functions φn are simultaneously interpolated based on available data (constraints)

C= hard equality constraints - to be honoured strictly

C≈ soft equality constraints – to be honoured in a least square sense

C> (hard) inequality constraints

Discrete Smooth Interpolator (DSI) interpolates φn based on

C = C= U C≈ U C> and “minimum local roughness” criterion [Mallet, 2002]

Page 9: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> how to build a computer model of fault-zone architecture?

gOcad topology and interpolation (CAD and geostats coupled)

PF

-SM

F s

yste

mco

nclu

sion

geom

odel

ling

discrete model Mn(Ω,N,φ,C)

n functions φn(α), ∀ α∈Ω

graph Ģ(Ω,N) linear constrains C

discrete fault zone architecture model (DFZAM) fault surface network and surrounding volume (damage zone), modelled with hierarchical fully coupled topology, integrating all data from field and subsurface geology

Page 10: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> the Pusteria (PF) & Sprechenstein-Mules (SMF) fault systemP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

PF is the eastern segment of the Periadriatic lineament, one of the largest (>600 km) faults in the Alps. SMF is a younger dextral lineament, connecting the PF to the Brenner detachment

PFPF

SMFSMF

Bre

nner

Bre

nner

[Bigi, 1992; Castellarin, 2004]

Page 11: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> the Pusteria (PF) & Sprechenstein-Mules (SMF) fault systemP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

PF is the eastern segment of the Periadriatic lineament, one of the largest (>600 km) faults in the Alps. SMF is a younger dextral lineament, connecting the PF to the Brenner detachment

PFPF

SMFSMF

Bre

nner

Bre

nner

[Bigi, 1992; Castellarin, 2004]

Page 12: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> the Pusteria (PF) & Sprechenstein-Mules (SMF) fault systemP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

PF is the eastern segment of the Periadriatic lineament, one of the largest (> 600 km) faults in the Alps. SMF is a younger dextral lineament, connecting the PF to the Brenner detachment

[Massironi, 2004]

Page 13: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> the Pusteria (PF) & Sprechenstein-Mules (SMF) fault systemP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

PF is the eastern segment of the Periadriatic lineament, one of the largest (> 600 km) faults in the Alps. SMF is a younger dextral lineament, connecting the PF to the Brenner detachment

[Massironi, 2004]

Page 14: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> the Pusteria (PF) & Sprechenstein-Mules (SMF) fault systemP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

PFPF

SMFSMFBrixen Granite (non-metamorphic footwall)Brixen Granite (non-metamorphic footwall)

Tonalitic “Lamella”(sheet-like pluton - 30Ma)

Tonalitic “Lamella”(sheet-like pluton - 30Ma)

Austroalpine Gneiss (Alpine metamorphism)Austroalpine Gneiss (Alpine metamorphism)SMFSMF

PFPF

PF is the eastern segment of the Periadriatic lineament, one of the largest (> 600 km) faults in the Alps. SMF is a younger dextral lineament, connecting the PF to the Brenner detachment

[Massironi, 2004]

hangingwallhangingwall

Page 15: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> the Pusteria (PF) & Sprechenstein-Mules (SMF) fault systemP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

Time & temperature constraints:

o Brixen Granite (footwall) always below 150-200°C in the Tertiary.

o Tonalitic Lamella emplaced at 30 Ma at about 450°C – 15 km, then exhumed with its host rock, the Austroalpine basement. The two hangingwall units cooled below ca. 250°C at 24 Ma. [Bistacchi, in prep.]

Page 16: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> the Pusteria (PF) & Sprechenstein-Mules (SMF) fault systemP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

Time & temperature constraints:

o Brixen Granite (footwall) always below 150-200°C in the Tertiary.

o Tonalitic Lamella emplaced at 30 Ma at about 450°C – 15 km, then exhumed with its host rock, the Austroalpine basement. The two hangingwall units cooled below ca. 250°C at 24 Ma. [Bistacchi, in prep.]

Kinematics: dextral with thrust component since 30 MaKinematics: dextral with thrust component since 30 Ma

Page 17: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> fault network (FN) and tectonic unit boundaries model: geometryP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

field geology & borehole data 8km x 4 km x 1.5 km 3D model

[Bistacchi, 2007]

Page 18: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> fault network (FN) and tectonic unit boundaries model: geometryP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

[Bistacchi, 2007]

field geology & borehole data 8km x 4 km x 1.5 km 3D model

Page 19: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> fault network (FN) and tectonic unit boundaries model: geometryP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

[Bistacchi, 2007]

field geology & borehole data 8km x 4 km x 1.5 km 3D model

topology of FNtopology of FNconstraintsconstraints

interpolationinterpolation

Page 20: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> fault network (FN) and tectonic unit boundaries model: geometryP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

field geology & borehole data 8km x 4 km x 1.5 km 3D model

[Bistacchi, 2007]

Page 21: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> properties: 1- fault cores (preliminary characterisation)P

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

fault core relatively thin layers (1-5 m?) of mature fault rocks, developed generally in correspondence of major tectonic boundaries and master faults, where much of the displacement is achieved

Brixen Granite Tonalitic Lamella &Austroalpine basement

5-10 m protocataclasite(ultra-) cataclasite along PSZs (dm-m)

thick greenschist facies phyllonites (pre-brittle faults) reactivated by frequent

PSZs (cm-m) with foliated ultracataclasite and polished SSs

Page 22: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> properties: 1- fault cores (preliminary characterisation)P

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

fault core relatively thin layers (1-5 m?) of mature fault rocks, developed generally in correspondence of major tectonic boundaries and master faults, where much of the displacement is achieved

Brixen Granite Tonalitic Lamella &Austroalpine basement

5-10 m protocataclasite(ultra-) cataclasite along PSZs (dm-m)

thick greenschist facies phyllonites (pre-brittle faults) reactivated by frequent

PSZs (cm-m) with foliated ultracataclasite and polished SSs

Page 23: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> properties: 1- fault cores (preliminary characterisation)P

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

fault core relatively thin layers (1-5 m?) of mature fault rocks, developed generally in correspondence of major tectonic boundaries and master faults, where much of the displacement is achieved

Brixen Granite Tonalitic Lamella &Austroalpine basement

5-10 m protocataclasite(ultra-) cataclasite along PSZs (dm-m)

thick greenschist facies phyllonites (pre-brittle faults) reactivated by frequent

PSZs (cm-m) with foliated ultracataclasite and polished SSs

Page 24: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> properties: 1- fault cores (preliminary characterisation)P

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

fault core relatively thin layers (1-5 m?) of mature fault rocks, developed generally in correspondence of major tectonic boundaries and master faults, where much of the displacement is achieved

Brixen Granite Tonalitic Lamella &Austroalpine basement

5-10 m protocataclasite(ultra-) cataclasite along PSZs (dm-m)

thick greenschist facies phyllonites (pre-brittle faults) reactivated by frequent

PSZs (cm-m) with foliated ultracataclasite and polished SSs

Page 25: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

5 µm

> properties: 1- fault cores (preliminary characterisation)P

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

fault core relatively thin layers (1-5 m?) of mature fault rocks, developed generally in correspondence of major tectonic boundaries and master faults, where much of the displacement is achieved

Brixen Granite Tonalitic Lamella &Austroalpine basement

5-10 m protocataclasite(ultra-) cataclasite along PSZs (dm-m)

thick greenschist facies phyllonites (pre-brittle faults) reactivated by frequent

PSZs (cm-m) with foliated ultracataclasite and polished SSs

Page 26: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> properties: 2- damage zonesP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

damage zone how to (semi-) quantitatively map “damage” (40 km2)?

1m x 1m square window1m x 1m square window

towards fault core

Page 27: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> properties: 2- damage zonesP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

damage zone how to (semi-) quantitatively map “damage” (40 km2)?

Fd = cumulative fracture length/areaNj = number of joint setsFd = cumulative fracture length/areaNj = number of joint sets

Fd = 11.263 m-1

Nj ≤ 3Class 1

Fd = 11.263 m-1

Nj ≤ 3Class 1

Fd = 13.118 m-1

Nj ≤ 3Class 1

Fd = 13.118 m-1

Nj ≤ 3Class 1

Fd = 18.511 m-1

Nj = 4÷5Class 2

Fd = 18.511 m-1

Nj = 4÷5Class 2

Fd = 23.653 m-1

Nj > 5Class 3

Fd = 23.653 m-1

Nj > 5Class 3

Fd = n.d.Nj = n.d.Class 4

Fd = n.d.Nj = n.d.Class 4

Fd = n.d.Nj = n.d.Class 4

Fd = n.d.Nj = n.d.Class 4

towards fault core

Page 28: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> properties: 2- damage zonesP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

damage zone how to (semi-) quantitatively map “damage”?

GISborehole

log

Nj class.

DSI interpolation

damagemodel

Nj class.

Interpolation on a 3D regular grid (voxet).Grid connectivity broken across faults

(topology of the model reflects fault zone architecture).

Page 29: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> properties: 2- damage zonesP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

damage zone how to (semi-) quantitatively map “damage”?

GISborehole

log

Nj class.

DSI interpolation

damagemodel

Nj class.

Interpolation on a 3D regular grid (voxet).Grid connectivity broken across faults

(topology of the model reflects fault zone architecture).

FAULT

Page 30: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> discrete fault zone architecture model (DFZAM)P

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

Page 31: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

> conclusionP

F-S

MF

sys

tem

conc

lusi

onge

omod

ellin

g

1. Discrete model of fault zone architecture:dependence of damage zone thickness from fault network geometry (curvature, stepovers) and lithology has been verified

a new framework for damage zone characterization has been proposed (need to be further verified)

damage zones around stepovers are highly fractured “columns” hydraulic conduits

2. Why a computer model of fault-zone architecture could be useful?visualization, understanding complex structures

quantitative analysis of geometry (e.g. differential geometry) made easy

build realistic model of geometry and propertiesthat can be output to, and quantitatively compared to mechanical models, fluid flow models, etc.

Page 32: 3D modelling of fault-zone architecture along a major ... · 3D modelling of fault-zone architecture along a major Alpine wrench lineament: the Pusteria and Sprechenstein-Mules fault

BBT SE is acknowledged for giving access to > 2000 m of continuous core and borehole logging data of the Brenner Basistunnel project

ASGA, Earth Decision Sciences and Paradigm are thanked for welcoming Padova and Milano Bicocca Universities in the gOcad Research Consortium

… thank you!