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European Journal of Applied Sciences – Vol. 12, No. 3

Publication Date: June 25, 2024

DOI:10.14738/aivp.123.17110.

Hansen, J. (2024). Sill Propagation and Climbing in Layered Crystalline Host-Rocks: Examples from Saucer-Shaped Sills of The

Faroe Islands. European Journal of Applied Sciences, Vol - 12(3). 570-579.

Services for Science and Education – United Kingdom

Sill Propagation and Climbing in Layered Crystalline Host-Rocks:

Examples from Saucer-Shaped Sills of The Faroe Islands

Jógvan Hansen

HansenReSearch, Undir Heygnum 8, FO 100 Tórshavn, Faroe Islands

ABSTRACT

Mafic sills, which commonly occur in layered sedimentary and crystalline settings

worldwide, may occur as sub-lateral sheets or as saucer-shaped bodies. Values

and distributions of Young’s Modulus within their ambient host-rocks determine

their mode of emplacement. Current models on development of saucer-shaped

sills depict either melt propagation from single sources along sub-lateral

relatively weak layers, from which they abruptly climb/transgress through

stronger layers at intervals, or they may evolve by radial melt

propagation/intrusion from one or more sources, while gradually/continuously

ascending/climbing through strong and weak layers alike. The first model invokes

involvement of sill overburdens and overlying free surfaces, while the latter

envisages closed igneous systems, where host-rocks both above and below the

advancing magmas are affected without involvement of overlying free surfaces.

Margins of saucer-shaped sills at various stages of developments, cropping out in

the FaroeIslands, offer some new insights into sill evolvement in layered

crystalline host-rocks. This study suggests that the slightly upward-curving

geometries of Faroese sills stem from initial radial propagations/intrusions of thin

magma fronts, where systematic depth-dependent variations of Young’s Modulus

in the Earth’s crust governed gradual and continuous climbing of these. Some of

their melts likely propagated initially as lobes or thin magma-fingers in a mole- like fashion before coalescing, without noticeably affecting the overlying free

surfaces prior to the main inflation phases.

Keywords: Faroe Islands, flood basalts, sill intrusion, sill propagation, sill climbing

INTRODUCTION

Basaltic sills, displaying a variety of geometries and sizes, have been reported in numerous

extension/rifting related settings worldwide, the most common of which being sedimentary

basins and basaltic lava piles (1,2). Sills may occur individually, but do not un-commonly

occur in droves, where individual intrusions can be interconnected and are thus often

thought to have acted as reservoirs and conduits during magma transport to the Earth’s

surface (1,2,3,4,5,6). As sill intrusions reside in both offshore and onshore environments,

investigations of these are in general based on seismic images/profiles for the former and on

direct visual observations and measurements for the latter versions. Although widespread sill

networks can be highly visible in seismic images from offshore sedimentary basins (7,8),

direct investigation of sill networks and/or individual sills, cropping out onshore, may better

disclose details in their developing history.

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Hansen, J. (2024). Sill Propagation and Climbing in Layered Crystalline Host-Rocks: Examples from Saucer-Shaped Sills of The Faroe Islands.

European Journal of Applied Sciences, Vol - 12(3). 570-579.

URL: http://dx.doi.org/10.14738/aivp.123.17110

A mechanism with sub-lateral melt propagation along weak layers with intermittent

transgressions/climbing through stronger stratum, i.e. melt advancement through layers with

varying values of Young’s Modulus, has frequently been invoked for development of saucer

shaped sills in stratified sedimentary media (9). Interaction between advancing melts and

overlying free surfaces during sill formation is commonly envisaged for sill emplacement in

relatively shallow crustal environments, where certain sill lengths/diameters versus their

depths of intrusion are thought to determine their angles of transgression/climbing and

hence their ultimate sizes (6,9). An alternative theory, applicable for sill intrusion into

layered crystalline media, such as basaltic lava successions of various thicknesses, which are

occasionally separated by thinner sedimentary/volcaniclastic sequences, proposes

propagation of thin magma fronts, where uneven displacement of strata above and below

advancing sill tips determine their angles of gradual and continuous transgression/climbing

(1,4,10). These authors did not envisage any noticeable interaction between the advancing

melts and overlying free surfaces prior to any main inflation phases. This latter model relies

on the fact that systematic depth dependent variations in values of Young’s Modulus have

been reported for the Earth’s crust previously (11).

In this study, we focus on well-exposed margins of a few Faroese sills of various thicknesses.

Field evidences suggest that at least some of their initial magmas progressed in a radial

fashion in part as lobes or as broad fingers prior to ultimately coalescing.

GEOLOGY OF THE FAROE ISLANDS

The basaltic lava pile, making up the archipelago of the Faroe Islands, which are situated at

the NW European margin hosts a number of saucer-shaped sills of various sizes, which are

‘frozen in time’ in various stages of developments (1,4,10). In general, most of the eight

formations making up these basaltic successions are intruded by a host of sub-vertical dykes

and numerous irregular intrusions, while the sills of this study crop out in the three

uppermost formations (Fig. 1).

The sills of the Faroe Islands were emplaced in an extensional/rifting related geological

environment during a relatively wide time span from ~55.5 Ma to ~50.5 Ma (12). These sills

are typified in that they decreased in sizes and volumes with time, i.e. the largest sills are

~55.5 Ma old with younger ones decreasing in size until intrusion of the least voluminous at

~50.5 Ma (12). The oldest Faroese sills and sill segments decrease in thicknesses from the SE

towards the NW, which is also consistent with intrusion at increasingly greater

stratigraphically depths from the SE towards the NW (1,4,10,12).

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Figure 1. Brief description of the general area and locations utilised in this study (Modified

from: Hansen and Ganerød, 2023). a, Geographical location of the Faroe Islands, based on

Google Earth. b, Geological map of the Faroe Islands, based on topographic data from Munin fo,

displays local geological formations and geo-locations of the local saucer-shaped sills of this

study. c, Close-up view of the three sills included in this contribution, based on topographic

data from Munin fo, where small black circles indicate exact localities.

FIELD EVIDENCES AND MEASUREMENTS

The sill margins being focused on in this study display thicknesses of 0.35 to 0.60 metres for

the Kvívík Sill,  1.5 metres for the Vestmanna Sill and  15 metres for the Streymoy Sill. If it

is assumed that the uppermost Faroese Enni Formation (Fig. 1) had an original average

thickness of ~1 to ~1 1⁄2 km (13), then the melts that gave rise to the fringes of the sills, which

are utilised in this contribution, originally crystallised at stratigraphical depths of ~1 to ~1 1⁄2

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Hansen, J. (2024). Sill Propagation and Climbing in Layered Crystalline Host-Rocks: Examples from Saucer-Shaped Sills of The Faroe Islands.

European Journal of Applied Sciences, Vol - 12(3). 570-579.

URL: http://dx.doi.org/10.14738/aivp.123.17110

Figure 2. Images of a very thin margin of the Kvívík Sill in the valley of Gassádal. a, slightly

inclined thin sill lobes ( 3-4 dip towards ESE), being  0.5 m thick, arranged in en-echelon

fashion, which are more or less connected by a moderately inclined ‘dykelets’. Yellow dashed

lines indicate sill outlines. b, ‘Dykelets’ become thinner with decreasing depths. c, Closer view

of b, with inset showing close-up view of dykelets.

km as regards the ~55.5 Ma old Streymoy Sill and ~1.4 to ~1.9 km as regard the ~55.5 Ma

Kvívík Sill and the ~50.5 Ma Vestmanna Sill. Hence, the studied thin margins of the Kvívík and

Vestmanna sills crystallised at 400 to 500 metres greater stratigraphical depths when

compared to the much thicker studied margin of the Streymoy Sill. The characteristics

displayed by these three sill margins/fringes are described below.

The actual locality of the Kvívík Sill is characterised by discontinuous slightly inclined thin sill

lobes, which are more or less arranged in en-echelon fashions (Fig. 2a). Here, the front of one

exemplified section to the right (SE) is connected to the tail of the next one at slightly lower

elevation to the left (NW) by a number of very thin dykes/ ‘dykelets’ (Fig. 2b). It is

noteworthy that thicknesses and density of ‘dykelets’ decrease slightly downwards from the

SE towards the NW (Fig. 2c).

The studied margin of the Vestmanna Sill represents a cross section of two relatively thin

sub-horizontal magmatic lobes exposed at slightly different elevations, with the higher to the

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left (NW) and the lower to the right (SE) (Fig. 3a). These two lobes are connected ‘end to end’

by a much thinner sub-vertical ‘connection’ (Fig. 3b).

Figure 3: Images of a thin margin of the Vestmanna Sill on the mountain of Hægstafjall. a, Cross- section of thin ( 1.5 m thick) roughly sub-horizontal sill lobes arranged at slightly different

altitudes. Yellow dashed lines indicate lobe outlines. b, the sill lobes are connected by an even

thinner ( 0.35 m thick) short sub-vertical section.

The studied margin of the Streymoy Sill is characterised by a thick and continuous margin to

the left (SE), with a somewhat thinner and lower-lying lens-shaped margin/section to the

right (NW). These are separated by a belt of host-rocks measuring around 15 to 20 metres

(Fig. 4a). These two margin sections are more or less connected by a multi-dike, emanating

sub-vertically upwards from the SE tip of the lens-shaped lower margin and sub-vertically

downwards from the bottom of the upper margin. The uppermost parts of this multi-dyke,

consisting of 4 to 5 thin individual dykes/’dykelets’, extend downwards for ~1/4 of the total

distance from the upper margin, while ~12 closely spaced individual thin dykes/’dykelets’,

with individual thicknesses from a few centimetres to a maximum of ~12 cm with a

combined maximum width of between 1.6 to 1.8 metres for the entire multi-dyke, extend

upwards for ~3/4 of the total distance from the lower margin (Fig. 4b, c).

Strike and dip measurements suggest that initial magma flows progressed more or less from

right to left for the Kvívík Sill (Fig. 2), while initial melts broadly progressed towards the

reader at slight upwards angles in the other two sill margins (Fig. 3; Fig. 4).

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Hansen, J. (2024). Sill Propagation and Climbing in Layered Crystalline Host-Rocks: Examples from Saucer-Shaped Sills of The Faroe Islands.

European Journal of Applied Sciences, Vol - 12(3). 570-579.

URL: http://dx.doi.org/10.14738/aivp.123.17110

Figure 4: Images of the thick margin of the Streymoy Sill in the valley of Hundsarabotn. a,

Cross-section of a more than ~20 m thick sill margin, moderately inclined ( ~5° dip.) towards

the SW arranged as a lens-shaped body to the right and a continuous section to the left at

slightly higher altitude being separated by a belt of hostrocks. The margin/sections are more

or less connected by a sub-vertical multi-dyke. Yellow dashed lines indicate outlines of sill

margin/sections. b. A few ‘dykelets’ of the upper1/4 of the multi-dyke. c, Numerous ‘dykelets’

of the lower 3/4 of the multi-dyke.

MODES OF SILL INTRUSION

Based on some of the noticeable characteristics displayed by the investigated sill

margins/rims of this contribution, a few inferences can be put forward.

The actual margin of the Streymoy Sill is thick and this intrusion was probably fully

developed, while the studied margins of the basal sections of the Vestmanna and Kvívík sills

are thin and were quite likely only in their infancy once they crystallised at deeper

stratigraphical levels. It is noticeable that the upper rims of e.g. the Kvívík Sill a few

kilometres towards the ENE (Fig. 1, not shown) are much thicker (£ 15 m), thus giving this sill

an overall wedge-shaped appearance, a feature also displayed by the Faroese Morskranes and

Sundini sills (1,10) (Fig. 1b).

The multi-dykes/’dykelets’, associated with the margins of the Kvívík and Streymoy sills of

this study reveal details on initial principal stress axes in host-rocks around their advancing

tips and on either side of the evolving intrusions. During sill intrusion prior to any breach of

overlaying free surfaces two sets of principal stress axes are in existence within their

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Hansen, J. (2024). Sill Propagation and Climbing in Layered Crystalline Host-Rocks: Examples from Saucer-Shaped Sills of The Faroe Islands.

European Journal of Applied Sciences, Vol - 12(3). 570-579.

URL: http://dx.doi.org/10.14738/aivp.123.17110

provide an ample proof of the compression of host-rocks below thin advancing sub- horizontal magma tips/fronts, and not only above them. The restricted thicknesses of the

actual lobes of the Kvívík Sill in particular and their relatively great stratigraphical depths

strongly suggest that their initial melts advanced and climbed as slightly inclined lobes or

fingers in a molelike fashion (prior to ultimately joining together) without interacting with

the Earth’s free surface. Here, general depth-dependent variations in Young’s Modulus in the

Earth’s crust (11), where host-rocks atop thin advancing magma fronts are displaced slightly

more than those below these due to uneven values of Young’s Modulus, most probably caused

the magma lobes/fingers to advance and climb at slight angles, as envisaged in previous

studies (1,4,10) (Fig. 5a, b).

When it comes to the actual margin of the Vestmanna Sill, it could represent a slight evolution

from its thinner counterpart in the Kvívík Sill, where the thin connecting section either

represents a single ‘dykelet’ that has inflated to ~0.35 metres or it may represent several

‘dykelets’ that ultimately coalesced into one following displacement of initial slivers of host- rocks in between (Fig. 3; Fig. 5c).

Figure 6: Simplified drawings depicting sill evolution in basaltic lava successions (Modified

from: Hansen, 2011, Hansen et al., 2011). a, Fully developed sill geometry from propagation of

thin magma fronts in a closed system. b, Sill overburden is breached atop its highest point and

inflation has commenced. The Faroese Kvívík, Sundini and Morskranes sills display similar

wedge-shaped geometries. Small open circle denoted KS points to studied margin of the Kvivik

Sill while that being denoted VS points to studied margin of the Vestmanna Sill. c, Sill

overburden is breached atop either ends and intrusion is fully inflated. The Faroese Streymoy,

Eysturoy and Svínoy-Fugloy sills largely display similar geometries. Small open circle denoted

SS points to the studied margin of the Streymoy Sill.

It is overwhelmingly likely that the actual margin of the Streymoy Sill, situated at a relatively

high stratigraphic level, displaced and breached its overburden and the Earth’s free surface

during inflation. This scenario, where tensile strengths in host-rocks on top of the inflating sill

no longer played a vital role, most likely caused a reorganisation of local principal stress axes,

which is reflected by the orientation and overall asymmetrical nature of the actual subvertical

multi-dyke (Fig. 4; Fig. 5d). Here, the greater density and lengths of ‘dykelets’ emanating

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upwards from the lower-laying lens-shaped sill margin, as compared to those stretching

downwards from the higher sill margin, point to interaction with the overlaying free surface

during sill inflation. Accordingly, the probable breaching of the overlaying free surface likely

interfered with the local largest principal stress axis 1 between the two inflating sill sections,

so as to reduce compression below both of these during the final phases of their

evolvement/inflation. Therefore, host-rocks above these margins were relatively more

compressed by propagation/inflation compared to those below them (Fig. 4; Fig. 5d).

CONCLUDING REMARKS

In conclusion, the following statements may be put forward: Sill margins of this study

crystallised at various stratigraphical levels and at various stages of development. The

characteristics displayed by these and associated multi-dykes may disclose general facts on

evolution patterns of basaltic sills intruded into volcanic lava successions. Here, the

characteristics of the thinner sill margins point to development by slight climbing of thin

magma fronts across strong and weaker layers alike in response to general depthdependent

variations in values of Young’s Modulus in the Earth’s upper crust. Accordingly, the greater

parts of sill geometries in such settings may form prior to any involvement or breaching of

overburdens and overlaying free surfaces. Once sill overburdens and overlaying free surfaces

are indeed breached, general sill inflation will take place (Fig. 6a-c).

References

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European Journal of Applied Sciences, Vol - 12(3). 570-579.

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