Transcript
  • BASIN ARCHITECTURE AND LITHOSPHERIC STRUCTURE OF THE BARENTS SEA REGION FROM GEOPHYSICAL MODELLING

    L. Marello (1,2); J. Ebbing (1,2); L. Gernigon (1)1 Geological Survey of Norway (NGU), Trondheim. 2 Department for Petroleum Engineering and Applied Geophysics,

    Norwegian University of Science and Technology (NTNU), Trondheim.

    Part of:PETROBAR Project

    “Petroleum-related regional studies of the Barents Sea region" project funded by NFR and Statoil and includes participants from the University of Oslo, PGP, University of Bergen, International Re-search Institute of Stavanger, Geological Survey of Norway and Volcanic Basin Petroleum Re-search.

    Contact: [email protected]

    NGUNorges geologiske undersøkelseGeological Survay of Norway

    Magnetic model made by 6 layers with homogeneous properties

    Magnetic Basement blocks and geological implica-

    Svalbard : Magnetic lineaments are correlating with Caledonian structures

    West Barents Sea: anomaly trends represent Caledonian Thrust Front

    West Barents Sea: high magnetic block; high pseudogravity; shallowing of deep dense lowercrust could be a methamorphic core complex formed during the exumation of the lower crustalrocks by low-angle detachments

    Central Barents Sea High Anomalies:seems to be part of two different basement blocks

    E-Svalbar : Sill intrusions are related to the CretaceusMagmatic event

    NE-Barents Sea : pseudogravity coincident with Bouguer gravity

    Central-N Novaya Zemlya : susceptibility inversion and forward modelling not coinciding

    N and S East Barents Sea Basin:have different basement

    SW Barents Sea: Magnetic block: Early Proterozoic and Archeancomplexes are near the surfaceNon Magnetic block: thick turbidite succession

    SW Barents Sea: Anomaly trends coincide with Timanian trends

    S Novaya Zemlya : Anomaly trends coincide with Timaniantrends

    E-Svalbard : Small scale anomalies have shallower Euler solutions and are considered the effect of sill intrusion

    NE-Barents Sea 1:Lineaments are following Uralian setting

    4) INTEGRATION OF RESULTS

    Fendinsky High: lineaments seems to be the prolongations of Timanian linea-ments (e.g. BF: Baidaratsky Fault)

    The magnetic field analysis and the in-version results combined with the for-ward models give a regional overview of the Barents Sea basement and allow to organize the area in sub-domains with similar magnetic properties.The magnetic patterns in comparison with geological trends and the suscepti-bility distribution help to illustrate the tectonic setting.

    Bibliography- Blakely, R., 1995. Potential Theory in Gravity and Magnetic Applications. Cambridge University Press. , 461 pp.-Dimakis, P., Braathen, B.I., Faleide, J.I., Elverhoi, A. and Gudlaugsson, S.T., 1998. Cenozoic erosion and the preglacial uplift of the Svalbard-Barents Sea region. Tectonophysics, 300(1-4): 311-327.- Grad, M., Tiira, T. and Group, E.W., 2009. The Moho depth map of the European Plate. Geophys. J. Int., 176,(279-292).- Gramberg, I.S., Glebovsky, V.Y., Grikurov, G.E., Ivanov, V.L., Korago, E.A., Kos'ko, M.K., Maschenkov, S.P., Piskarev, A.L., Pogrebitsky, Y.E., Shipelkevitch, Y.V. and Suprunenko, O.I., 2001. Eurasian Arctic Margin: Earth Science Problems and Research Challenges. Polarforschung, 69: 3-25.-Jakobsson, M., Macnab, R., Mayer, L., Anderson, R., Edwards, M., Hatzky, J., Schenke, H.W. and Johnson, P., 2008. An improved bathymetric portrayal of the Arctic Ocean: Implications for ocean modeling and geological, geophysical and oceanographic analyses. Geophysical Research Letters, DOI: doi: 10.1029/2008gl033520.- Johansen, S.E., Ostisty, B.K., Birkeland, Ø., Fedorovsky, Y.F., Martirosjan, V.N., Christensen, O.B., Cheredeev, S.I., Ignatenko, E.A. and Margulis, L.S., 1992. Hydrocarbon potential in the Barents Sea region: play distribution and potential. In: T.O. Vorren et al. (Editors), Arctic Geology and Petroleum Potential. Norwegian Petroleum Society (NPF), Special Publication, pp. 273-320.- Ritzmann, O., Maercklin, N., Faleide, J.I., Bungum, H., Mooney, W.D. and Detweiler, S.T., 2007. A three-dimensional geophysical model of the crust in the Barents Sea region: Model construction and basement characteriza-tion. Geophysical Journal International, 170(1): 417-435.- Skilbrei, J.R., 1991. Interpretation of Depth to the Magnetic Basement in the Northern Barents Sea (South of Svalbard). Tectonophysics, 200 (1-3): 127-141

    4 transects FORWARD MODELLING

    To validate the inversion results, to test the susceptibility distribu-tion and to refine the top basement geometry we apply forward modelling.The seismic models reflect the main structures and constrain the geometry.Density modelling provides extra constraints for the deep struc-tures (e.g. Moho). The results of the susceptibility inversion have been used to set the average susceptibility on the initial magnetic domains.After large number of tests the initial magnetics, densities and crustal geometries were jointly refined.The results along the WE lines are integrated and combined using the SNBS.

    Error= 2.2927

    = Calculated= Observed,

    Grav

    ity (m

    Gal)

    -10

    0

    10

    20

    Mag

    netic

    s (nT

    )

    -100

    0

    100

    200

    300

    Dept

    h (k

    m)

    40

    30

    20

    10

    0

    0 400 800 1200Distance (km)

    0.0032700

    0.0032500

    Cenozoic/Mesozoic sediments

    Paleozoic sedimentsPaleozoic/Riphean complex

    Finmark Platform

    Central Barents

    Monocine Tiddlybanken

    BasinFedynskiy

    High

    North East Barents

    Sea BasinKola-KaninMonocline

    MaliginskiyGraben

    Paleozoic/Riphean complex

    0.0082760

    0.0182760

    0.0132730 0.04

    2910

    0.0352810 0.079

    27900.0522880

    0.0212850

    0.0272800

    0.0292720

    0.0232710

    0.00013290

    Error=35.34

    = Calculated= Observed,

    Mantle

    0.0053020

    0.0053020

    0.0053000

    SBS

    line

    CBS

    line

    NBS

    line

    D1 D2 D3

    BasmABasmB

    Susceptibility SIDensity kg/m3

    SNBS line

    0.0022810

    0.012840 0.035

    2950

    0.0272830

    0.01628500.027

    2750

    0.003 ?2810|

    0.0032700

    0.0013060

    0.0013110

    0.0013000

    0.019 ?2770

    0.0012500

    Cenozoic/Mesozoic sediments

    Paleozoic sediments

    Grav

    ity (m

    Gal)

    0

    50

    100

    Mag

    netic

    s (nT

    )

    -100

    0

    100

    200

    Dept

    h (k

    m)

    40

    30

    20

    10

    0

    500 1000 1500Distance (km)

    Error= 50.149

    = Calculated= Observed,

    Error= 15.142

    = Calculated= Observed,

    0.0032760

    0.0092890

    02700

    02800

    0.0042830

    02500

    0.00063290 Mantle

    NO DATANO DATA

    BasmABasmB

    Bille�ordenFault Zone

    Norwegian Greenland Sea

    Svalbard Margin

    Franz Victoria Basin

    Kong KarlsPlatform

    North East Barents Sea Basin

    Skalistoe Uplift

    C1 C2 C3 C4 C5

    NSBS

    line

    Susceptibility SIDensity kg/m3

    NBS line

    D=2700, S=0.006

    0.0053040

    0.0053010

    0.0182820

    0.0312850 0.014

    28400.0112930

    0.0192820

    0.0272820

    0.0013290

    Mantle

    027500.022

    2880

    0.0152780

    0.0272730

    0.0012500

    Central Barents Sea Monocline

    Kong KarlsPlatform

    OlgaBasin

    SørdkappBasin

    EdgeøyaPlatrdorm

    Norwegian Greenland Sea

    Cenozoic/Mesozoic sediments

    Paleozoic sediments 0.003, 2700

    Error= 10.606

    = Calculated= Observed,

    NavayaZamlya

    0 500 1000 1500

    SNBS

    line

    Distance (km)

    0

    -30

    30

    60

    0

    10

    20

    30

    40

    Error= 35.631

    = Calculated= Observed,

    Dep

    th (K

    m)

    Gra

    vity

    (mG

    al)

    Mag

    netic

    s (n

    T)

    50

    -80

    80

    0

    0.0052000

    AdmiralityHigh Kara Sea

    BasmABasmB

    Noth-East Barents Sea Basin

    B1 B2 B3 B4

    Susceptibility SIDensity kg/m3

    CBS line

    Dep

    th (K

    m)

    Gra

    vity

    (mG

    al)

    Mag

    neti

    cs (n

    T)

    0.0452710 0.046

    2720

    0.062940

    0.042780

    0.0012450

    0.0262750

    0.0482980

    0.0142770

    0.0013290

    Mantle

    0.0052930

    0.0342810 0.027

    2850

    02740

    0.0242730

    0.0012500

    Central Barents Sea High

    S-East Barents Sea Basin

    NavayaZemlya

    NordkappBasin

    OttarBasin

    NorselHigh

    SvalisDome

    BjørnyaBasin

    StappenHigh

    VastbakkenVolcanicProvince

    SNBS

    line0 400 800 1200

    0

    10

    20

    30

    40

    0

    -30

    30

    60

    -100

    0

    100

    200

    Distance (km)

    Error= 6.662

    Error= 39.625

    = Calculated= Observed,

    = Calculated= Observed,

    Cenozoic/Mesozoic sediments

    Paleozoic sediments 0.002, 2700

    A1 A2 A3 A4

    BasmABasmB

    Susceptibility SIDensity kg/m3

    SBS line

    2) MAGNETIC BASEMENT STUDY FROM INVERSION

    Layers Susceptibility (SI*10-3) Boundaries layer0 km constant grid

    1-Water 0Bathymetry1

    2-Upper sediments 0.314 8 km constant grid

    3-Lower sediments 2.51 Top basement2

    4-Upper crust 12.57-37.7 25 km constant grid

    5-Lower crust 5.03Moho 3

    6-Mantle 0.6283

    3) BASEMENT STUDY FROM COMBINED FORWARD MODELLING

    NGU-VESEGEI compilation 2009

    H ig h p a s s m a g n e tic fie ld L o w p a s s m a g n e tic fie ld

    T ilt d e riva tive m a g n e tic fie ld P s e u d ogra vity

    High pass 70 km trendsHigh pass 120 km trendsTilt derivative trends

    On the map the picks of the filtering and tilt derivatives are displayed. The pseu-dogravity in the background helps to define the magnetic anomaly regions.

    MAGNETIC FIELD ANALYSIS

    Anomalies enhancement

    3D INVERSION TECHNIQUE

    3D Euler solutions

    Shallower solutions :1-Kola kanin Monocline extending northward up to the Nordkapp Basin2- Eastern part of Svalbard

    Medium solutions1- Central North Barents Sea

    Deep solutions:1- Noethwest of Admirallity Highand Myszheniya Highs2- southern part of the South East Barents Sea3- two central Barents Sea anomalies

    SI= 0.5 Thick step

    4 . 18 8 .38 12.6 17 .8 23 28 .3 33 .5 3 8 . 7 SI x 10-3

    HM

    HM

    LM

    HM

    MM

    MM

    LM

    HMMM

    HM LM

    LM

    MM HM

    LM HM

    HM HM

    MM

    LM

    HM

    LM HM MMHM

    LM MM HMHM

    NBS line

    CBS line

    SBS lineSNBS line

    a)

    b)

    c)

    d)

    e)

    NBS

    CBS

    SBS

    SNBS

    Sensitivity test Influence onsusceptibility results

    Top basement uncertainty depths max8kmshallower

    -3,8 SI*10-3

    Top basement uncertainty depths max6 km deeper

    6 SI*10-3

    Low pass filtered magnetic field -2,5 – 2,5 SI*10-3

    Upper continued magnetic field -5,6 – 5 SI*10-3

    All basement magnetic -7,5 – 5 SI*10-3

    Uncertainty ≈ 30%

    3D INVERSION TECHNIQUE

    inversion tests

    SUSCEPTIBILITY INVERSIONMAGNETIC RESIDUAL

    1=IBCAO model (Jakobsson et al., 2008); 2=W-Barents Sea (Skjlbrei et al. 1991); E-Barents Sea (Johansen at al., 1992: Gramberg et al., 2001); 3=combination of Barents 50 (Ritzmann et al., 2007) and Moho depth of the European Plate (Grad et al., 2009)

    SENSITIVITY TEST

    First regional indication of the mag-netization distribution in the Barents

    Sea basement.

    Low Magneticbasement

    Medium Magneticbasement

    High Magneticbasement

    Magnetic Map Anomaly

    Magnetic anomaly regions defined from field analysis.

    Parameters used for the susceptibility inversion:

    - Total magnetic field-inverted layer (upper crust) simpliffied as the sum of vertical prisms of

    infinite depth extension.-Inversion routine for basement: combination of filters and inverse Earth

    filter (Blakley, 1995)-Starting susceptibility: 0.031 SI

    -Maximum standard deviation= 10 nT-Maximum number of iterations= 9

    -No changes in geometries

    Forward modelling results:

    - give reasonable explanation of magnetic and gravity anomalies- are consistent with the inversion results- refine the magnetic basement

    ++++ Observed magnetic anomaly++++ Calculated magnetic anomaly

    W E

    W E

    W ES N

    T33A-1867

    Dimakis at al. 1998

    Density-depth relation

    1) Linear function 2) Exponential function

    Petrophysical database(density and susceptibility)

    Velocity / density relation

    Structural maps

    1) EXISTING DATA Seismic informations

    Moho depths from BARENTS50 modelhttp://www.norsar.no/c-90-Barents-Sea-3D-Model.aspx

    Top Basement models

    The uplift and the con-sequent emersion and erosion of the West Bar-ents Sea have implica-tion in the physical property distribution.

    BasmA: form Skilbrei et al., 1991 (West Barents Sea) and Johansen et al., 1992 (East Barents Sea).BasmB: from Skilbrei et al., 1991 (West Barents Sea) and Gramberg et al., 2001 (East Barents Sea).

    Contour lines every 2.5 km.

    The Barents Sea tectonic setting is the result of multiple tectonic processes including three orogenic phases (Timanian, Caledonian and Uralian) and several episodes of rifting leading to a complex tectonic setting. Most prominently this can be observed in the differences between the rift basins configuration of the West Barents Sea and the mega-sag basins of the Eastern Barents Sea. The mechanisms leading to the present day basin and crustal architecture are still not completely understood.

    In the present study we investigate the top basement geometry and the basement properties of the Barents Sea by testing the validity of previ-ous studies and trying to overcome the discrepancies between them. To reach our interest beside the conventional magnetic field analysis, we run inversion magnetic modelling and sensitivity tests. The inversion re-sults are then integrated along four profiles with seismic and gravity data and using 2D combined forward modelling we refine the magnetic properties along the profiles. The four lines are linked together and illus-trate the main crustal units of the all Barents Sea associated as different magnetic basement domains. Finally we discuss the meaning of the magnetic anomalies and of our results in terms of tectonic and geologi-cal implications.

    Neog

    ene

    Pale

    ogen

    eCr

    etac

    eous

    Jura

    ssic

    Tria

    ssic

    Perm

    ian

    Carb

    onife

    rous

    Devo

    nian

    Silu

    rian

    Ord

    ovici

    anCa

    mb-

    rian

    MES

    OZO

    ICPA

    LEO

    ZOIC

    rifting (N. Atlantic, Arctic, W. Siberia)

    episodic rifting episodes

    Verkhoyansk orogenyEast Siberia

    uplift-erosion in Arctic areas

    Initiation of EurekanOrogeny

    N. Atlantic riftingleading to breakup

    BREAKUP EURAMERICAN BASIN

    BREAKUP N. ATLANTIC

    carbonate platformorganic buildups

    evaporites

    progressive closure ofthe Iapetus

    CollisionBaltica-Greenland(Scandian Orogen)

    Post-orogenic collapse

    GEODYNAMIC EVENTS

    TERT

    IARY

    Q u a te rn a ry

    widespreadintracratonic

    rifting

    Uralideorogeny

    Ellesmerian/Caledonian

    orogeny

    Iapetus formation

    major plate reorganisation

    Siberiantrapps

    renewed uplift and erosionof Ural orogen

    transtensionnal and transpressive regimes along the Western Barents shelf

    humid climate affects sedimentation

    Boreal and Thetys oceans disconnected

    Pale

    o-pr

    oter

    ozoi

    c

    PRO

    TERO

    ZOIC

    Mes

    o-pr

    oter

    ozoi

    cNe

    o-pr

    oter

    ozoi

    c

    Timanianorogeny

    INTRODUCTION


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