CHAPTER 4, VERTICAL MAGNETIC GRADIENT ANALYSIS 46
CHAPTER 4. CHAPTER 4. VERIIICAL MAGNETIC GRADIENT ANAIYS/S 49
Computed gradient anomaly
Part of a
total
field profile andits
computed gradient is reproducedin
Figure 4.7. The magnetic anomalyZ
car-be
correlatedwith a pyrite
bearingquartzite (strike
Ó= 5")
which has beenfolded
into the Monarto
Syncline (Mancktelow,1979).
Using stacked profllesof the
vertical gradient,this
magneticunit
can be followedfor
over30km,
and easily traced around the fold ofthe
syncline.A drill
hole, located 3.5km north of
Z, intersected bedded layersof
sulphides (containingboth
magnetite andpyrrhotite) within
the quartzite,at
a depth of 30 metres.The
anomalyZ
was interpretedto be
dueto a thin
sheetat a
depthof
116m below the sensor,with
an index parameter d=
319o andI :
15360. Taking the average sensor heightto
be80m
givesthe
depth below ground surfaceto
be36m.
Assuming rlo remanent component,the dip
was estimatedto be 44"W and 0.16m to be the product of the
susceptibility and thickness. The depth estimateis
reasonably accurate, considering the undetermined extent of weathering and the shallow depth involved, and while the dip estimate couldnot
be verified,it
was consistent
with
the general dips in the area. Measured susceptibilities vary from 100 x 10-5 SIto
1000x
10-5 SI. The corresponding thicknesses would then varyfrom
160to
16 metres.4.2.2 Error analysis
Vertical gradient profiles computed from the measured one-dimensional
total
magnetic field over two-dimensional structures are reasonably accurate when the depth to the top of the source lies betweenA
and 10z\,A
beingthe
productof the
differencinginterval
andthe
sample spacing (Paine, 1986). When computed gradient anomalies are interpreted, errorsin
the gradient values resultin
inaccurate parameter estimates.To study the
effectof filtering
errorson
parameter estimates,a FORTRAN
program waswritten to carry out the error
analysisfor a
wide tangeof
parameter(depth
andd)
va,lues.The theoretical
total
field anomaly over athin
sheet was computedfor
different values of d and depth, using a sample spacing of 25 metres andwith
the origin of the model as a sample point.The profiles were taken perpendicular
to strike.
The vertical gradient was computed from thetotal
field as describedin
Section 4.1.1.The errors
in
the estimates were defined as follows:eIIOIh eIrOId
100
x (true
depth-
estimated depth)/ true
depthtrue0-estimatedd.
Depths were varied from 60m
to
1500m while á was varied from 0oto
180o. For each depth valuethe
vertical gradient anomaly was interpreted, parameter estimates recorded, and errors computed. The errors varied bothwith
depth as well as d andfor
a given depth, varied widelywith 0.
For each depth value,the
minimum and maximum errorsin the
parameter estimates were usedin
drawing Figures 4.8 and 4.9.Where depth
to the top of the
sheetis ( A,
thereis
alot of "ringing" in the
computed gradient andthe
accuracyin the
estimated depth varieswith
d andthe error
can be as much as80%.
For depth: A, the
errorin
depth estimates can go ashigh
as 30%,but
is generallywithin
10%error.
For depths between1.64
and84,
depth estimates are wellwithin
10% error and estimates of dwithin
6oerror.
For depths> 94,
the peaks tend to flattenout
and accuracy decreases. Wherethe origin is not a
samplingpoint, the
nearest samplingpoint
canbe
atllrrr
16
l2
WIDTH/DEPTH RATIO
-.2000 0 300 600 900
1 200
.3
a p
ì
o Þ5 p
ÌtÈ dl (ú
.FÉ
tho Þ.E
of
Þ
8
É.ll
oçÍ
É.
LrJ 6
-9 -9
-12 -12
-15
Figure 4.10: Error
in
usingA,
as awidth
estimator of a dy.l,-etoo-.ly.
't50.0
100.0
50.0
0.0
.4000
.æ00
.0000
f-E
'tÕ
õ
iT
€'
l- co
o-o
o
Figure 4.11: Total magnetic fieid intensity and
its
vertical gradient over athick
dyke: (Dyke1)CHAPTER 4. VERTICAL MAGNETIC
GRADIENTANAIYSIS
50the
most 12.5 metres away. Thereis
no significant changein
the parameter estimates and for1.64 <
depth( 84,
accuracy isstill within
acceptable limits.The
accuracyin
parameter estimationin
usingthe
nomogramon the
computed gradientis
dependent onthe
accuracy of the gradient values. These values are reasonably accurate for two-dimensional structures whenthe
depthto the top
lies betweenÀ and 104, A
being theproduct of the
differencinginterval
andthe
sample spacing. Depth estimates arewell within
10% error providedthat
thetrue
depth lies between1.64
and84.
Estimates of 0 are accurateto
a few degrees over a wider range oftrue
depth values.4.3 Interpretation of thick dyke anomalies
The equations
for
thetotal
magneticfield
andits
vertical gradient over athick
dyke are givenin
equations 4.6 and 4.7. As thewidth to
depthratio
of a dyke incteases, the number of peakson its vertical
gradient anomaly increasesfrom two to flve. The original
aimin
solving for characteristic points on the gradient anomaly was tofind
relationships between the peak values and locations which would yield all the parameters of the model. Since peak values could not be described by analytical expressions, they were calculated by forward modelling. The theoretical gradient was computedfor
model dykes: thewidth to
depthratio
was variedfrom
.5to
10 in steps of .5, and d was varied from 0oto
360oin
steps of 5o.A
computer program waswritten
to search the gradient anomaliesfor
the peak values and positions. As before, the main minimum is Vrrri. and the main maximum Vrrr.*. The distance between the peak positions of Vr,¡. andV-r*
along the profile is defined
to
beAr.
The
initial
ratios which were investigated were vertical ratios (ratios of different combinations of the peak values) and horizontal ratios (ratios of the profile distance between different peaksto Ar.
No satisfactorywidth to
depth estimator wasfound.
However, the analysis showedthat for
the dykes investigated:1. A,
is a goodwidth
estimatorfor all
values of d providedthat
thewidth to
depth ratio is greaterthan or
equalto 2.
The error barsin
Figure 4.10 indicate the maximum possible elrors,2. Lalh
and V..¿;o=
lVrninlVror*l are complicated functionsof the
dyke parameters.If
thewidth to
depthratio
can be determinedby
some other method,then
I/.'¿¡ois
unique for a given valueof d.
Once dis
known,the
depthto
thetop
can be determined using the appropriate valueof Lolh.The
two main sources of errorin
estimating depth and d arise from the inaccuraciesin the
approximation of the vertical gradient andin
the estimation of thewidth to
depthratio.
Notethat if
the anomaly is symmetric, then V,,,¡,, is taken to be the most westerly (or southerly) minimum and Vrrr"* is the most easterly (or northerly) maximum.This method was tested on two dykes. Figures 4.11 and 4.12 show the
total
field and vertical gradient anomaly causedby
two different dykes. The intensity of the Earth's magnetic field istaken
to
be60000nT
andits inclination to
be -65o.The
width to
depth ratiosfor
each dyke were determined using Barongo's (1985) "straight slope" method. Tablesfor
the V¡¿¿¡6 andA,
as functions of thewidth to
depthratio
(these are includedin
Appendix G) were used to compute thewidth,
depth and á and the results are givenin
Table4.2.
The correct determination of thewidth to
depthratio
iscritical to
the success oftr
co
õ iI
Ê
Èg
(5
o_o
o
100.0
50.0
0.0
.4000
,2000
.0000
0 300 600 900
Figure 4,12: Total rnagnetic field intensity and
its
vertical gradient over athick
dyke: (Dyke2).Parameter
Dykel
Dyke2True ue timated Value
00
200m 700 m
400 500 B
225m
675 m 45"
450 E
True value Estimated Value Strike
Depth
width
0
Dip
00
200m 300 m
300 600
w
178m 266 m
300
600w
Table 4.2: Results of interpreting the models shown