posiva 2002 22 working report web
TRANSCRIPT
-
8/16/2019 POSIVA 2002 22 Working Report Web
1/107
W o r k i n g R e p o r t 2 0 0 2 2 2
Fracture
Maooing from Olkiluoto
Borehole
Image
Data
2001
Eve l i ina
T a m m i s t o
T o m a s
L eh t im ak i
J o r m a
P a l m e n
Pi r jo He l la
Eero H e i k k i n e n
i n t ac t
y
ay
2 0 0 3
Working Reports contain information
on work in
progress
or
pending
completion.
The
conclusions and viewpoints presented in the report
are
those
of
author s)
and
do not necessarily
coincide wi th those of Posiva.
-
8/16/2019 POSIVA 2002 22 Working Report Web
2/107
TEKIJAORGANISAA TIO:
TILAAJA:
Fintact y
Hopeatie 1 B
00440 Helsinki
Posiva Oy
Toolonkatu 4
00100 Helsinki
TILAUSNUMEROT:
Fin tact Oy: 9646/0 1/HH
TILAAJAN YHDYSHENKILO:
Heikki Hinkkanen
Posiva Oy
TEKIJAORGANISAATION YHDYSHENKILO:
TEKIJAT:
TYORAPORTTI 2002-22
FRACTURE MAPPING FROM OLKILUOTO BOREHOLE
IMAGE DATA 2001
Eveliina Tammisto Tomas Lehtimaki Jorma Palmen Pirjo Hella Eero
Heikkinen
TARKASTAJA:
Henry Ahokas
Fintact Oy
-
8/16/2019 POSIVA 2002 22 Working Report Web
3/107
Tammisto, E., Lehtimaki, T., Palmen, J., Hella, P. Heikkinen, E. 2002. Fracture
mapping from Olkiluoto borehole image data, 2001. Working Report 2002-22. Posiva
Oy, Helsinki. 109 p.
BSTR CT
As a part of the complementary site investigations for the underground disposal of spent
nuclear fuel at Olkiluoto site, fracture mapping from optical imaging data was done in
boreholes KR1, KR2, KR4, KR9, KR12, KR13 and KR14. The data contained BIP
imaging, carried out in 1996, from sparsely fractured sections in KR1, KR2 and KR4
that have not been included into previous interpretation (745 m), and OPTV imaging
results from KR9, KR12, KR13 and KR14 in 2001 (2306 m).
The task included fracture mapping from the image material and determination of
orientation of the fractures using the Well CAD utility, determination of properties of the
fractures, compilation
of
print-outs, and data delivery. The following fracture properties
were mapped: fracture type, aperture and filling thickness, fracture shape and colour.
The results of this independent mapping task provide supplementary information, i.e.
complete orientation coverage, apertures, etc. not found from core mapping data. The
observations were checked with comparing them to the core samples.
n total6138 fractures were mapped. These represent roughly 80 of the core mapping
fractures. Not every fracture reported from core can be observed from the images, but
on the other hand, specifically from frequently fractured and core loss sections also few
possible previously non-reported fractures have been encountered.
The open or partly open fractures, some of which might have also filling, make on
average 5
of
all fractures.
In
less fractured
KR1
and KR2 these are rare, and in KR4
and KR13 more frequent (9 ) than for the others. Fractures with filling form two-third
of all fractures, and closed ones one-third. Aperture and thickness both range from 0.5
mm to 120 mm. Thickness has been reported for most
of
the fractures.
More than a h lf of the fractures are planar and smooth in their shape (55 ). Slightly
less (one-fifth) are found both planar and rough, and undulating and smooth. The
fracture colours are determined mostly as a grey scale (60-80 . Black fillings are seen
less than others probably due to dark background, grey and white are more frequent. For
KR2 and KR13 the colours brown, green and yellow are found relatively often.
Seepage has been found from 0 - 49 fractures per borehole, most frequently in KR12.
For almost
h lf
of these seepage locations, a hydraulic conductivity indication has been
found with good depth agreement. Based on seepage, these are potential inflow
locations in open borehole conditions.
Keywords
Borehole optical imaging, fracture interpretation, nuclear waste disposal
-
8/16/2019 POSIVA 2002 22 Working Report Web
4/107
-
8/16/2019 POSIVA 2002 22 Working Report Web
5/107
ONTENTS
BSTR CT
TIIVISTELM
CONTENTS
PREF CE
INTRODUCTION 3
2 IMAGE MATERIAL 7
2 1 Image logging arrangements 7
2 2 The image properties 10
2 3 The image quality due
to
borehole conditions
14
2 4 The preconditioning of the image material
23
3 MAPPING THE FRACTURES 25
3 1
Preparation of the material
25
3 2
Picking
of
the features 25
3 3 Quality criteria of the picking
26
4 DETERMINATION OF THE PROPERTIES
31
4 1
Design of property parametres
31
4 2 The distribution of mapping results according to level of confidence
71
5 CHECKING THE OBSERVATIONS WITH THE CORE SAMPLES 73
5 1 The checking procedures 73
5 2
The results
of
the checking
73
6 RESULTS 75
6 1
Contents
of
the results
75
6 2 Fracture type distributions 75
6 3 Fracture aperture
and
thickness 80
6 4 Fracture forms
80
6 5 Fracture filling colours
81
6 6 Inflow indications 83
6 7 Presentation of results
and
data delivery
88
6 8 Comments on results 89
7 SUMMARY
91
REFERENCES 93
APPENDICES
97
-
8/16/2019 POSIVA 2002 22 Working Report Web
6/107
2
PREF CE
This report describes fracture interpretation of borehole imaging data from Olkiluoto in
2 1 (supplementary mapping
of
KRl KR2 and KR4, and mapping of KR9, KR12,
KR13 and KR14). This work belongs to Posiva site characterization programme for
spent nuclear fuel disposal. The work has been ordered from and supervised by Posiva.
The authors wish to thank Posiva s contact persons Mr. Heikki Hinkkanen and Mrs.
Liisa Wikstrom for their useful comments and guidance. We also thank the experts
who reviewed the work and results on their essential communication: Dr. Alan
Geoffrey Milnes
of
GEA Consulting, Dr. John Hudson of Rock Engineering
Consultants, Mr. Kai Front of VTT Technical Research Centre of Finland, and Mrs.
Ursula Sievanen of Saanio Riekkola Consulting Engineers.
Mr. Raimo Ruotsalainen and Mr. Esa Raivonen of
Geological Survey, and Mr. Aimo
Hiironen
of
Posiva deserve special thanks for arranging the review
of
the core samples.
-
8/16/2019 POSIVA 2002 22 Working Report Web
7/107
3
INTRODUCTION
Orientations and properties of fractures were mapped from borehole imaging data of
Olkiluoto boreholes KR9, KR12, KR13 and KR14 and partly boreholes KR1, KR2 and
KR4. The data contained 1996 BIP imaging results from those KR1, KR2 and KR4
sparsely fractured sections, that have not been included into previous interpretation
745 m, Stn1hle 1996) and OPTV imaging results from KR9, KR12, KR13 and KR14
in 2001 2306 m, Wild et al. 2002).
t was necessary to carry out the image mapping as a separate task, because the drilling
and core mapping has been performed well before some months to 2 years) this
work. On general view, as core mapping is traditionally performed immediately on
site, and for the imaging can be performed due to optical conditions not earlier than
h lf a month after drilling, the most efficient mapping procedure has been recognized a
separate work, divided into subtasks that are checked numerically between the steps.
This also saves time and preserves consistency on mapping of the image properties.
Any direct comparison to the actual core mapping data is a separate task and has been
left to the interpretation phase during later works. Background data is referred to
adequate level.
The fracture mapping used extensively the WellCAD software from Advanced Logic
Technology ALT 2001). WellCAD can handle and represent different kind of
borehole data and store the data linked to the presentations. All logs
on
a single file are
displayed on the same scale. The original image data together with borehole deviation
data were imported to WellCAD
by
Ms. Eveliina Tammisto and Mr. Tomas Lehtimaki
Chapter 2). Before mapping, the core samples and images were visually examined to
understand the appearance of
the features on the images. The fractures were mapped
and data transferred to determination
of
properties
by
Ms. Tammisto KR2, KR4, KR9,
KR13), Mr. Eero Heikkinen KR14) and Mr. Lehtimaki KR1, KR12) Chapter 3).
Determination
of
fracture properties from image was completely done by Ms.
Tammisto, a geologist. This was required by the Client, with an intention to maintain
consistency in the properties see Chapter 4). Principles on determination were agreed
with Mr. Jorma Palmen, a geologist. The data was first checked by Mrs. Pirjo Hella
mathematician) to select the observations to be confirmed or rejected. The selected
observations were checked over with the core samples see Chapter 5) at Loppi core
archive KR1, KR2, KR4, KR9, KR12) and in Olkiluoto KR13 and KR14). Ms.
Tammisto, Mr. Lehtimaki and Mr. Heikkinen participated into this work. The sole
purpose
of
checking was to remove most
of
the features encountered
on
imagery that
are not real fractures in sense of core mapping.
Planning
of
the layout for printouts Chapter 6), and data delivery were done partly by
Mr. Heikkinen, partly by Mrs. Hella and Ms Tammisto. Summary tables of different
fracture properties were compiled by Mrs. Hella. Practical arrangements for printing
and data compilation were done
by
Ms. Tammisto.
The preceding data is listed in the Table 1 below. The fracture locations and
intersection angles from core mapping were used in confirming the image observation
before review with the core sample.
Other background data has not been used directly,
but understanding of these has been required to perform the mapping.
-
8/16/2019 POSIVA 2002 22 Working Report Web
8/107
4
The mapping of core sample has listed all penetrative mechanical discontinuities with
their form and roughness on the sample, the mineralogical mapping specifically also
the coating minerals. Hydraulic conductivity is mapped with the flow logging. For
KRl
KR2 and KR4 there has been also dipmeter mapping available, that has brought
out valuable although incomplete orientation data.
Table 1 The preceding material from mapped boreholes
Method
Systematic
core
mapptng
Systematic
mineralogy
mapptng
Hydraulic
flow logging
data
Geophysical
logging
Electrical
dipmeter
BIP imaging
and mapping
Fracture
database
FDB)
OPTV
image
Properties
Length location primary
reference), type open,
filled, tight, slickensided),
intersection angle, partial
orientation, form,
roughness, tentative
mineralogy, frequency,
RQD. All observed ones.
Length, type open,
breakout, slickensided,
filled); thorough fracture
mineralogy and
appearance, thickness of
filling. Not all fractures.
Location and hydraulic
conductivity
of
the
conductive fractures
Reference to lithology,
fracture zones, hydrology
Fractures, general
orientation of banding;
interpretation
of
orientation clusters
Image from whole
borehole, mapped data
from selected sections
those not included to this
work); fracture location,
type, orientation,
aperture, form, tentative
mineralogy, alteration
Merging
of
above
mentioned fracture
properties to same
observations
Non-mapped image data,
mapped in this work
Borehole
KR1
KR2
KR4
KR9
KR12
KR13
KR14
KR1
KR2 KR4
KR9
KR12
KR13,
KR14
KR12
KR1, 2, 4,
9
KR13, 14
all
Reference
Suomen Malmi Oy 1989a
SMOY 1989b, Rautio 1995a
SMOY
1990, Rautio 1995b
Rautio 1996
Niinimaki 2000
Niiinimaki 2001a
Niinimaki 2001 b
Blomqvist et al1992 Gehor et al. 2001a
Gehor et al. 1996
Gehor et al. 1997
Gehor et al. 200 1b
Not available during mapping
Pollanen Rouhiainen 2000.
Rouhiainen 1999.
Not
available during mapping
Niva 1989,
SMOY
1989c, d, 1990b,
Julkunen et al. 1995, 1996, 2000, Lahti
et al. 2001
KR1, 2, 4 Lowit et al 1996
KR9, 12, Not available
13, 14
KR1, 2, 4 Strahle 1996; mapping supplemented by
Karanko
et
al. 2000. Systematic mapping
similar to this work performed for
70o/o
of imagery.
KR 1 2, 4 Saksa et al. 1997, Karanko et al. 2000
KR9, 12, Wild et al. 2002
13, 14
-
8/16/2019 POSIVA 2002 22 Working Report Web
9/107
5
Most important data not received from other than the image mapping are the thorough
orientation, and the aperture o the fractures, combined with the observation type seen
in image. The type o observation is different from each mapping method, and will
rather be supplementing each other than being exclusive.
It was expected that there is a proportion o fractures not seen in the imagery (Saksa et
al. 1997, Karanko et al. 2000).
n
this sense both the other mapping data and the image
mapping results are in their part inadequate to describe the fracture properties alone.
Without a direct comparison to the core data (performed in fracture database
approach), it cannot be said which (kind of) core fractures are not included into the
current observations. A priori assumption is that these may be thin, dark fractures on a
dark background, and probably often perpendicular to the borehole (horizontal lines on
image). Despite o this potential statistical bias, the coverage o core fractures is
expected to be reasonable.
The work in hand concentrated on mapping o the imagery to produce material for later
geological usage. Results were referred with the core sample for quality s sake. These
results should not be considered as the primary data source o fracturing. A relevant
data source these become only after the fracture database has linked core fractures to
the image data. For orientation distributions, the image mapping data is the only
available thorough data set until the database comes available.
-
8/16/2019 POSIVA 2002 22 Working Report Web
10/107
7
IMAGE MATERIAL
Borehole wall images
of
KR1, KR2 and KR4 BIP investigations (Stn1hle 1996) and
OPTV investigations in 2001 from KR9, KR12, KR13 and KR14 (Wild et al. 2002)
were analysed
in
this work. Previous interpretation
of
BIP data (Strahle 1996) was
supplemented from least fractured sections, omitted from the preceding work. The
interpretation included for each borehole the sections shown in Table 2.
Table
2
The extent
o
he interpretation work or this report
Borehole Borehole length range, m
Length,
m Image
type Reference
KR1
341 -500 (sections d e in
267.5 BIP
Strahle 1996
field data),
644-
740 (field data section g)
KR2 300-
390 (sections c d),
2 1
BIP
Strahle 1996
440-
539 (section e)
KR4
390-
480 (sections d and e),
276
BIP Strahle 1996
570 - 739 (sections f g and j)
KR9 40-602
559
OPTV Wild et al. 2002
KR12
40-
793 751 OPTV
Wild et al. 2002
KR13
6-499
494 OPTV
Wild et al. 2002
KR14 9-513.5 502
OPTV
Wild et al. 2002
Total 3050.5
This chapter lists the techniques used, the properties of the images, and the observed
factors in image quality, which have influenced to the mapping and
may
affect to the
results.
2 1
Image logging arrangements
The images consist of bitmaps arranged by depth and orientation. Images have been
acquired by slowly lowering or raising a wire-line camera probe in a borehole and
digitally sampling the borehole image at a dense, constant depth rate.
n
the probe the
light of a LED-string is reflected from borehole wall to a mirror and further projected
onto CCD-element (a video camera). The acquisition geometry, and the parameters of
the image data content are shown in Figure
1.
Each 360 or 720 pixels' row in the image presents a full circle around the borehole
wall captured from a circle on the image. This produces a radial resolution
of
1 or 0.5
degrees, respectively. The specifications of the tools used are presented in Table 3.
The capturing has been performed at a rate of
113
or
115
frames
per
second. The
resulting recording rate or the depth resolution of the image lines is 0.5 or 1.0 mm,
depending on available resolution and logging speed. Recorded image lines were
stored into a computer and transferred to a MO or compact disc. Images contain RGB
data at a colour resolution of 0 ...255 units for each Red, Green and Blue channels
( millions
of
colours ).
Due
to their very large size bitmap images were stored
in 3
150 m slightly overlapping sections during the field work. These data sections
( logging runs ) are indicated
by
letter indexes
a
through
k
in
each borehole.
-
8/16/2019 POSIVA 2002 22 Working Report Web
11/107
8
able 3 The tool and operation specification details for BIP and PTV images
Tool Details BIP OPTV
Probe manufacturer
RaaX Ltd Japan).
Robertson Geologging UK)/
OyO Japan)
Operator
SKB/Geosigma Strahle
Robertson Geologging
Ltd.
1996), Sweden
Wild et al.
2002), UK.
Vertical sampling used 1 mm max 0,25 mm)
0,5 mm
Horizontal sampling used
1° 360 pixels) or 0.49 0.5° 720 pixels) or 0.24 mm
mm at
a 56 mm at 56 mm and 0.33 mm at
76
diameter borehole
mm borehole diameter
Storage size
1Mb/metre
4Mb metre
Data format BIP binary
Initially LGX binary),
received as
Dill
Nominal logging rate
1 5 m/minute
0,5 m/minute
Illumination
LED at mirror LED at camera objective
Recording geometry
Conical mirror Hyperbolical mirror
Cable
Optical Coaxial steel armored
Logging direction
Upwards
Mainly upwards
An image has been oriented to the down side
of
inclined borehole BIP image, Strahle
1996), or
by
a magnetic 3-axial compass Flux gate) to the magnetic North, then
adjusted to the site North OPTV image). Because
of
the rapid changes in local
magnetic field orientation in presence of magnetized minerals in the host rock, the
initial OPTV image has been straightened up by the operator Wild et al. 2002) by
replacing the orientation with Maxibor or Fotobor orientation data Rautio 1996,
Niinimaki 2000, Niinimaki 2001 a b).
Examples
of
the images are in Figures 2 and 3, and their colour histograms in Figures 4
and 5 in Section 2.2 below.
-
8/16/2019 POSIVA 2002 22 Working Report Web
12/107
a) The down-hole tool assembly
NON M GNE11C _
CEN f iV\ ISERS
T R N
SP
A
RE
NT
WINDOW
SONDEHE O
)
XI
X
ACCELEf\O t.IETEf\
c) Screen (camera) view
9
-
Camera field
of
view
Image of
circular mirror
Sample circle
Hypothetical X Y
~ ~ ; ; . . . _ _ _ . pixel grid
b) The
OPTV
functional arrangement
CD
'0
s
r
Video Camera
c) Image
arrangement
Azimuth
N
E
s
Lighting Ring
w
Figure 1 The nomenclature used in the image presentations and alignment. a) the
PTV image tool and b) the camera functional arrangement with c) the
screen view during logging. The 3-component inclinometer and
magnetometer provide the tool orientation reference to magnetic and site
North and
to
borehole deviation. This is used to align the Sample circle in
c) to arrange the image at subsequent depth lines to show the pixels
clockwise, each row starting at reference direction for OPTV the True
North; for BIP the down side) modified from Wild et al 2002). The
sinusoid line on wrapped-out image shows a planar fracture projection.
N
-
8/16/2019 POSIVA 2002 22 Working Report Web
13/107
10
2.2 he image properties
The image properties are differing slightly with respect to the technique used in
logging. Figures 2 - 5 illustrate these differences. Generally, the difference in pixel
resolution can be seen in approximately 1
2
vertical and
1:
1 horizontal scale images in
Figures 2 and
3
This scale is typical for the on-screen mapping and image quality
assessment, but usually not for presentations or printing. The features discussed on this
Section are most clearly visible on computer screen and suffer on quality when printed.
The hair cracks on pegmatite granite, having dark coating, appear slightly jagged in 1
degree
y
1 mm BIP image Figure 2), and the overall resolution gives a bit blurred
impression on this scale. The individual image pixels can be clearly seen in this scale.
The two-fold sharper resolution of OPTV image 0.5 degrees
y
0.5 mm) on less
fractured tonalite gneiss gives a more sharp impression, the individual pixels can not
be clearly distinguished on the image on this scale, and the minor cracks and grain
boundaries do not appear as jagged
as
in BIP. Even the foliation can be seen. Due
to
better resolution the OPTV data storage size is four times larger than for the BIP.
The above-mentioned properties are a result of selecting the data acquisition
parameters and the logging speed rate rather than due to tool functional properties. The
dark coating visible on Figure 2, and the opaque band on Figure 3 are due to borehole
conditions see Section 2.3 in more detail), and not related to the tool performance.
Further to the tool and logging resolution, the tool arrangement has influenced to the
image appearance. This can be seen in Figures 2 and 3 in the differences of lightness
and color saturation. The differences are shown in Figures 4 and 5, in sense of image
analysis, in the RGB channel plots of Figures 2 and 3, respectively. For a shadow cast
on the fracture trace due to the tool arrangement see below), the difference between
BIP and OPTV can be best viewed on images shown in Chapter 4 Figures 15 and 22).
In the BIP tool the light source is located adjacent to the conical mirror, to where the
light reflects perpendicularly from the borehole wall, and further to the camera
objective. The light source is powerful and the distance short, so in places there has
occurred saturation of the colour channels Figure 4). Usually there is also due to large
variation
of
dark and light rock types, an effect
of
automated exposure or shutter speed
light intensity) adjustment. No later adjustments to the images have been applied.
In the OPTV tool the light source is located behind the camera objective, and the
oblique light beam reflects first from the borehole wall to a hyperbolical mirror image
is similar to that from a fish-eye lens), and then to the objective. Despite
of
the strong
light source, the image is rather dark Figure 5). Light intensity is higher with larger
76
mm diameter. t was required to adjustment RGB scale contrast, brightness and colour
intensity). The adjustments were performed for optimal printing on photographic paper
for reporting Wild et al. 2002), and have caused the image colours to convert a bit
false, with slightly too high relative intensity in blue and red components. The light
intensity range is a bit narrow due
to
the initial darkness
of
the image, but the contrast
is adequately sharp for on-screen mapping. No later image enhancement has been
applied for presentations.
The oblique angle of illumination allowed many fractures to cast a shadow on the
image, so these can be observed pretty clearly the difference is seen best on Figures
6a,
15
and 22).
-
8/16/2019 POSIVA 2002 22 Working Report Web
14/107
igure
2
Example ofBIP image data from depth level
340.40
360.66 m of KR2,
granite pegmatite with hair cracks. Scale is approximately 1:2 vertically
and 1:1 horizontally. The pixels on the image can be seen quite well on this
scale. The light grains are slightly overexposed see also Figure 4
for
reference). Thin lines appear jagged.
-
8/16/2019 POSIVA 2002 22 Working Report Web
15/107
2
igure 3
Example of PTV image data from depth level 40.50
40
76 m ofKR9,
tonalite gneiss. Scale is approximately 1:2 vertically and 1:1 horizontally.
The pixels on image are not distinct in this scale. Image is sharp and the
grain boundaries and hair cracks appear rather smooth. Foliation and even
the vertical tool marks can be distinguished. On the other hand, the colour
range is narrow, and the dark grains are a bit underexposed see also
Figure 5 below).
-
8/16/2019 POSIVA 2002 22 Working Report Web
16/107
3
hannel Red
Figure
4
RGB colour channels o the BIP image
in
Figure 2 The colour range
is
well covered although the red channel is partly saturated resulting
to
slightly reddish image and partial overexposure.
Figure 5 RGB colour channels
o
he OPTV image
in
Figure
3
The colour range
is
narrow and show a slight underexposure on all components specifically on
red. This has lead to a slightly bluish image quality. Differences arise from
the tool geometrical arrangements.
-
8/16/2019 POSIVA 2002 22 Working Report Web
17/107
14
2.3 he image quality due to borehole conditions
Generally the quality
of
images is good and accurate. There are several technical
factors influencing the images that also affect the mapping see Table 4).
Table 4 The factors on image quality
Factors on image quality
Reason
Figure
Vertical banding,
Tool decentralization Figure 6a
opaque bands
Flow of
mud in water Figure 6b
Tool marks
Spiral banding, reamer Figure 7a
Vertical scratch lines Figure 7b
Optical conditions
Cloudy water Figure 8a
Coated borehole wall Figure 8b
Stick-slip motion ofprobe
Uneven movement, due to Figures 9a, b
coarse
surface,
cable
tension, flow, low weight
of
tool, or other
Typically the quality deeper in some boreholes has suffered from cloudy water, dark
opaque bands on image or stick-slip motion. Vertical illumination differences see
Figure 6a) occur due to the decentralization of the tool especially for OPTV images
from larger 76 mm diameter boreholes KR13 and KR14). Other vertical banding
occurs on the bottom side of the borehole due to an opaque material flowing in the
borehole water Figure 6b
.
This line helps to confirm the image orientation.
Drilling with an oversize reamer has left spiral marks occurring as 3-5 cm wide
patches, repeated at 13-15 cm period, of different colour than surrounding image see
Figure 7a). On the other hand, tool marks can be seen also as light and narrow vertical
lines Figure
7b
. These occur both in the BIP and the OPTV images.
Dirty borehole water can be seen in many locations, especially at fracture zones. The
feature is more severe when the borehole is freshly drilled, or when other measurement
have been performed shortly before image logging Figure 8a). Boreholes drilled long
before image logging have prominent sedimentation
of
rust or other dark material onto
the wall Figure 8b).
The stick-slip motion of the imaging probe can be seen as horizontal lines of short
vertical banding. The probe had jammed instantaneously but depth record changed
continuously, and the probe has then suddenly jumped over some 5 mm OPTV,
Figure 9b) to
10
cm BIP, Figure 9a), where true image pixels are missing because
they have been replaced with a single value in each column.
The length of each slip movement is smaller in OPTV image than in BIP. This may get
an explanation from the slower 0.5 m/min probe run rate of OPTV compared to 1.5
m/min of BIP. The phenomenon is expected to be caused y friction on the probe due
to coarse wall fractures etc.), or possibly a strong flow along the borehole; or cable
tension, or the light weight
of
the probe itself causing uneven movement, among the
other possible reasons. No direct explanation for this has been available so far.
-
8/16/2019 POSIVA 2002 22 Working Report Web
18/107
5
igure 6a Vertical banding. Probe decentralization KR13, depth
36.70
36.97 m .
Light intensity is higher on the high side of borehole larger distance from probe
produces better illumination due to distance and less narrow reflection angle).
-
8/16/2019 POSIVA 2002 22 Working Report Web
19/107
6
igure 6b Vertical banding Dark material flow along the borehole KR9, depth
231.60 231.95 m). The phenomenon is worst below fracture zones
-
8/16/2019 POSIVA 2002 22 Working Report Web
20/107
-
8/16/2019 POSIVA 2002 22 Working Report Web
21/107
8
igure
7b. Tool marks on the image. Narrow vertical tool scratch lines KR13,
401.10
401.35
m). The water is also rather cloudy dirty)
in
this image, and there is an
opaque band on down side
o
the borehole
to
the east on borehole inclined to the
west).
-
8/16/2019 POSIVA 2002 22 Working Report Web
22/107
19
igure 8a Water quality. Dirty water
in
the borehole KR14, 512.50 512.80
m .
Flowing clay particles can be seen
on
the cent er line
o
the image down side o the
borehole inclined to the north).
-
8/16/2019 POSIVA 2002 22 Working Report Web
23/107
20
igure 8b Water quality. Coated surface o borehole wall KRJ, 342.80 343.05 m .
The coating will accumulate during long period, and is best preserved on the spiral
tool mark.
-
8/16/2019 POSIVA 2002 22 Working Report Web
24/107
2
igure
9a Stick-slip motion. BIP image depth
643.90- 644.15,
KRJ). The length
of
each slippage is
20 30
mm, sometimes even larger, and damages the image severely
when observed. Occurrence is rather rare on sparsely fractured bedrock.
-
8/16/2019 POSIVA 2002 22 Working Report Web
25/107
22
Figure 9b. Stick-slip motion. PTV image KR14, 505.55 - 505.80 m). The length of
each slippage is only 3-5 mm, so the mapping is not totally blocked. The phenomenon
can be thorough over long sections.
In general the BIP image had suffered less from the dirty water and does not indicate
severe stick-slip motion on sections treated in this work. In 1996 the water in the
boreholes had settled down reasonably long. Also the colour intensity is good. On the
other hand the image pixel resolution is clearly poorer than in OPTV.
or
OPTV image
the pixel resolution is good but the image is dark and a minor stick-slip motion makes
the quality at the deeper parts slightly poor. The short time after drilling and other
borehole operations and probably the upward sequence of OPTV logging made other
boreholes than long time settled KR9 to suffer from dirty water conditions. KR12 was
reasonably good but for freshly drilled KR13 and KR14 the condition was less good.
-
8/16/2019 POSIVA 2002 22 Working Report Web
26/107
3
Also the decentralization causes more uneven light distribution in 76 mm diameter
boreholes compared to 56 mm, although the image quality is otherwise better with
larger diameter.
2 4 The preconditioning of the image material
Before the mapping the images were necessary to transport into the software system
used in the mapping.
Original OPTV and BIP data was imported in 10 m sections into WellCAD (version
3.0) working logs and stored into files containing the depth and original measurement
section information (index a - k ) in the file names. During the logging there was at
each run section a 1 - 2 m overlap reproduced in the images. Data import preserved the
original data resolution and image orientation, and allowed scalability on the depth and
the radial axis.
The BIP data was contained in binary files
of
100 m in each, including recorded depth
and orientation. The depth reading was adjusted according to values obtained from the
original report (Stn\hle 1996), representative at the top of each 10 m section. The
adjustments are linear between the top and the bottom of the each 100 m run section.
Residual differences of 10 - 20 cm to core sample can occur due to local deviation
from the trend. The stretch
of
the image over 1 m section is typically 5 - 15 cm. In
places the residual difference may reach 30 cm due to deviation in core mapping depth
(reconstruction of sample has failed),
or
a slight jamming of the probe.
The OPTV image was read in as 10 m sections of Device Independent Bitmap (DIB)
files. Original OPTV records were adjusted
by
setting top
of
subsequent log to the
bottom of previous log. The DIB files do not contain depth or orientation data, but left
edge of image is at the true North, and the top and the bottom depth values for each 1
m section were taken from the field work report (Wild et al. 2002) during the import.
The difference to the core sample is typically less than 10 cm, and at largest less than
30cm
The depth differences were found during the fracture mapping, but were not
systematically corrected for in the images. A proper adjustment would require trend
analysis for each section and non-linear
or
piecewise linear adjustments on that basis.
This was not task of the work.
The imported images were checked for possible errors and proper orientation.
Supplementary data including rock types, crushed borehole intervals, drilling fractures
with orientation and intersection angle, drilling fracture frequency, and the borehole
orientation (azimuth from the North and inclination from the vertical) were presented
in the Well CAD working logs to aid the mapping.
-
8/16/2019 POSIVA 2002 22 Working Report Web
27/107
25
MAPPING THE FRACTURES
In the planning phase o the work, typical appearance
o
the fractures in the images
were compared with those from core sample mapping at Loppi core archive (KR2 and
KR4, KR12)
o
Geological Survey and in Olkiluoto (KR14). The task was to
distinguish the real fractures (penetrative mechanical discontinuities) from narrow
mica bands, veins, foliation etc. possibly appearing similar way on the images.
3 1 Preparation of the material
In Well CAD the images were set to a depth scale o
1:1
- 1:2 and stretched on the log
so that the horizontal scale was approximately the same as the vertical (image 17 - 22
cm wide on screen; aspect ratio close to
1:
1
.
With this setting the pixels on screen
(0.25 mm) were close to the true image resolution.
A new Structure Log to be used in mapping was created on the WellCAD file. The
structure log and the BIP or OPTV image log were set on top
o
each other in exactly
same horizontal and vertical scales. The borehole diameter was set to a correct value
(56 or 76 mm) in the structure log. The tadpole presentations (arrow position on depth
shows the location, on horizontal scale the dip, and the tail points to dip direction,
north to up, east to left etc.)
o
drilling observed fractures (both the 3-D orientation and
the intersection angle) were set on the side
o
these two logs.
3.2
Picking of the features
On the structure logs were drawn numerically the sinusoidal projection traces o the
mapped fracture planes. The software stored the orientation data
o
the planes into data
table. Any (near to) planar feature appears on wrapped-out image as a sinusoid trace,
where the lowest point indicates the dip direction and amplitude (difference from
highest to lowest point) indicates the dip when correlated to the borehole diameter.
When the interpreted traces were combined to the borehole deviation data, the true
orientations o the fractures were obtained and converted to the tables. The data was
presented in a tadpole log beside the image log and compared to the core logging data.
A discontinuity feature in the image was considered to be a potential fracture, when it
differed clearly from the background image; was continuous over the image width, and
was not easily confused to a vein, band o mica plates, foliation or schistosity, or other
thin, similarly orientated features. These criteria are in accordance with those applied
in core mapping. In core mapping the features that penetrate thoroughly over the
sample are reported as fractures. This cannot always be seen reliably for weak class
o
features in the image. Features
o
incomplete continuity (partial fractures - terminating
to another, faulting one; discordant cracks between two adjacent fractures) were agreed
to be left out from the image mapping in this work, although these may be o
importance. Mapping can be continued for these features later according
to
the
requirements.
Typical indications o a fracture are often light in colour over a dark rock type, or dark
in colour over a light rock. These can be few pixels to several millimetres wide, or
even o a sub-pixel width (less than
0.3
-
0.5
mm) when showing clear continuity. A
(drilling induced) breakout or washout o filling material or the borehole wall will
make the observation easier. A black line in an image would indicate open space
(water filled) between the fracture surfaces, a coloured line on the other hand some
-
8/16/2019 POSIVA 2002 22 Working Report Web
28/107
26
kind
of
filling. Examples
of
clearly visible (probable) and poorly visible (potential)
fractures are shown in Figure
10.
Fracture observations were picked from activated structure logs y clicking with
mouse pointer in minimum three points (usually more) on the sinusoidal trace. The
software then calculated the fracture plane matching to the points and displayed the
corresponding projection trace on the log. The orientation data was stored into a file for
editing and exporting. The assigned depth is the midpoint of the trace depth (average
of
high and low points). The trace can be activated and graphically edited to represent the
observations in an optimal way.
3.3
uality criteria of the picking
Depending on the curvature and roughness of the real fracture surface pretty large
deviations from the orientation can occur. The software has directly calculated the
orientation
of
the plane relative
to
the borehole coordinates. The values only need to be
corrected for borehole deviation.
Typical accuracy of the plane fit is some
1 5
degrees. The relative dip is most accurate
when the plane intersects the borehole image nearly perpendicularly. The relative dip
direction is most accurate when the trace is aligned with borehole axis. For a stepped
or undulating trace, a visually well-representative trace was fitted, and there can be
quite a large deviation locally from the plane. This also means that the orientation is
more inaccurate, error can be even several tens of degrees. The final accuracy will
depend on the orientation of the fracture. The true dip direction is very insensitive for
near-horizontal fractures, even differences of some 30 degrees need to be allowed; on
the other hand for near vertical ones the dip will greatly depend on the accuracy of the
plane fit - small curvature
of
the trace or change in the intersection angle with borehole
axis will cause comparably large difference on the true dip.
It
has to be borne in mind
that also the core mapping orientation may in cases be inadequately defined.
The core mapping data from the drilling reports were used to guide the image mapping.
The mapping was done from top to bottom in order to detect depth differences. At this
point it was not possible to combine the mapped fractures together with the fracture
data from the drilling. The features that were clear and continuous on the image were
mapped most easily. The core data were mostly used for checking the correct depth
and orientation of the image, and when poorly visible features were mapped. Extremity
points of traces were avoided to be used in plane fitting.
For each observation a level
of
certainty was determined on basis
of
visibility on image
and on correspondence to the core data depth and orientation. Clearly visible trace was
nominated as probable and poorly visible as possible . Good correspondence with
location (10 cm) and reasonable correspondence with orientation (intersection angle, or
when available the dip direction and dip within 30 degrees) was indicated with label
existing , poor correspondence to either location or orientation with new .
Finally, after each depth section of a borehole was mapped, the structure logs of
observations were copied, and the copy was transformed to the true site coordinate
system. The data was converted to tadpole presentation and compared with oriented
drilling fractures. The data were exported to an Excel sheet. All data sets of a borehole
were merged together. Duplicate observations at overlapping logging run sections (1-2
m) were discarded.
-
8/16/2019 POSIVA 2002 22 Working Report Web
29/107
27
Example o clearly and weakly visible fractures, and the mapped traces, are shown in
pair o images in Figures 1
Oa b.
The probable fracture (green line) is seen as 5 mm
wide continuous trace, with a slight irregularity and curvature on the shape. The
possible fracture (thin black line) is seen as jagged, less planar thin bluish-white line
on both sides
o
the projection line (see red arrows on Figure lOb). Similar but more
planar feature is on the bottom o Figure
10.
This kind o features needed to be
confirmed from the core.
Figure lOa. Examples o racture picking KR9, 141.50-141.75 m). A clear feature
upper, a probable fracture), and a less well visible feature lower, a possible fracture)
with the fitted sinusoid curves
o a plane projection. The poorly visible trace is
indicated on Figure
JOb
arrows).
-
8/16/2019 POSIVA 2002 22 Working Report Web
30/107
28
epth
PTV
~ ~
1:2
E s
w
Figure JOb Examples o racture picking KR9, 141.50-141.75 m). A clear fracture
upper), and a less well visible fracture lower) without sinusoid curves. The red
arrows indicate the points where the undulating and thin, bluish white fracture trace
can be seen on the image. Penetrative continuity can be seen best on screen.
The mapping was done as a separate phase of work and entirely before proceeding to
classification and property determination. To speed up the procedure, mapping was
performed by three different persons a whole borehole for each):
Ms Tammisto, a geologist: KR2, KR4, KR9, KR13, KR14
Mr. Lehtimaki, a geophysicist:
KRI
KR12
Mr. Heikkinen, a geophysicist: KR14
-
8/16/2019 POSIVA 2002 22 Working Report Web
31/107
- -
~
- - - - - - - -
-
- - - - -
- - ---
9
Due to different handwriting , experience and background of persons involved, the
mapping was assumed to lead to slightly a different result with respect to relative
amount and certainty
of
observations (specifically the less visible ones). Some persons
tend to pick more clear features (losing some true data), and some try to find as many
features as possible (with a risk
of
mapping also non-true fractures). The differences
could have been best confirmed with a blind comparison test of a same section to avoid
influence of image quality and rock type.
The procedure of separate mapping of properties, and checking of observations against
the core sample were considered essential. Differences were considered to be equalized
by limiting the determination of properties to a single person, a geologist (Ms.
Tammisto).
Also, most important, using the separate phases made each phase more efficient and
time intensive compared to a situation where all steps were carried out simultaneously.
And, the statistical checking
of
picked properties was more consistent when handling a
single phase simultaneously over a borehole before proceeding to the next phase.
-
8/16/2019 POSIVA 2002 22 Working Report Web
32/107
3
DETERMINATION OF THE PROPERTIES
The determination of fracture properties was performed
by
Ms. Tammisto, a geologist,
alone to maintain consistency of the results. The work was performed with keeping
on
display simultaneously an Excel spreadsheet file with depth and orientation data, and
the WellCAD image log from corresponding depth.
The observation was viewed from the image log and the type, aperture and filling,
level of certainty, form and colour were determined. The possible values for properties
were agreed beforehand. The data was further classified and rearranged during the
checking and analysis procedure (Chapters 5 and 6).
4 1 Design of property parametres
The parameters were designed before the mapping to preserve similarity with the
previous image mapping results (Stn\hle 1996) and core mapping results (Suomen
Malmi Oy 1989a, b, 1990, Rautio 1995a, b, 1996, Niinimaki 2000, 2001 a, b) from the
area, and
on
the other hand the work done on merging the fracture data from different
mappings (Karanko et al. 2000). The technique was adjusted further to this work to
allow thorough mapping of the information visible in the image. The mapping
concentrated to the properties that cannot be reliably or completely obtained from the
core mapping (aperture and orientation were the most important).
On
the other hand,
the other, supporting parameters that are mapped also from the core, were expected to
assist later comparison and merging of the different observations and techniques. The
observation and their illustrations
on
pairs
of
Figures 11-24 are listed
in
Table 5 below.
Table
5
The parameters used in the determination
o
properties
Nos. Properties Comments
Figures
where
illustrated
1 Level
of
Clear visibility on
image=
probable , corresponding the
certainty
core data = existing
Clear visibility on
image=
probable , not corresponding
2
the core data = new
Poor visibility on image = possible , corresponding the 3
core data = existing
Poor visibility on
image=
possible , corresponding the 14
core data = new
2-5 Type Visual properties
of
feature on image; open fractures
15a-d
Partly open fractures
16a-d
Fractures with filling (no visible aperture) 17a-b
Fractures without visual filling or aperture
18a-b
6-7 Aperture, Measurement principle
of
the properties (perpendicular to
19a-b
thickness
the fracture plane)
8-9
Form
Fracture form, seen in image width scale (planarity, steps, 20a f
undulation) and in local mm scale (local smoothness)
21a-d
11- Col
or
Color or grayscale data visible in different conditions,
22a-b
3
ranging from darkness or gray value to col or dye 23a-b
14 Seepage Indication
of
material inflow from the surface 24
-
8/16/2019 POSIVA 2002 22 Working Report Web
33/107
32
The determined properties and their possible values are summarized in Table 6
Distributions o the fractures according to their class before checking are listed in
Table 7 The details on mapping parameters are presented below.
Level
o
certainty 1)
was used as a guiding basis for internal quality analysis o the
mapping. Also the observations to be checked were selected on this basis (Chapter 5).
Checking maintains the probable/possible classifications on Table 7 based on the
image visibility, but will alter the existing/new to checked/rejected when
applicable, to Table
9
The rejected class is not maintained in the final results (Table
9). The possible ones were checked systematically, the probable ones only with
few checks. A probable feature is so clear that there is no doubt on its determination
as a fracture. Observation was possible when it was not sure from image whether
there was a fracture or a vein or whether the observation was penetrative or not.
Feature was considered existing (fracture) when there were adequately similarly
oriented observations at the same depth level in the drilling report, and new when
there were no correspondence on either location or orientation. Also depth differences
between the image and core sample result in possible class observations. The typical
observations on different categories are illustrated in Figures 11 - 14.
Fracture type
2
- 5)
consists o four independent observations. These were
openness , filling , alteration and tightness . The previously used mutually
excluding types open-with filling-closed were considered to be inadequate so these
parameters were mapped separately. This results to fractures that can be with filling
and/or open. Anyhow, a closed fracture was not classified as an open fracture or a
fracture with filling, because it cannot be judged from visual appearance on image.
The type is a property that is observed from image at the intersection line
o
the plane
(along the plane), as there is no view onto the plane surface in image like there is in the
core. Observations are limited to their scale, i.e. features clearly smaller in thickness as
the pixel size are assigned with property closed , although there can be filling
material
or
aperture thinner than 0,25 mm. Thus a closed fracture in the image can
quite well be a fracture with filling in core mapping, etc. The open and partly open
fractures may be seen
as
black pixels in BIP OPTV, and shadow in OPTV. Filling
can be present also when a fracture is open . Partial filling has not been separated fom
complete in mapping. And, i there is no observation with filling , it does not mean
there would not be filling on the surface. The Figures 15 - 18 below show examples o
different fracture types.
The thickness 6)
o the visible solid filling between the fracture surfaces and the
aperture 7)
(a distance perpendicularly between fracture surfaces being apart each
another) were measured in millimeters from central part o the fracture trace,
perpendicular to the fracture plane, or, when the fracture was partly open, from the
open part. This was thought as the most representative value. At the peak points o the
projection (upper or
lower end) the cut section is wider and usually more interfered by
drilling than at the central part. Thickness does not include aperture, nor vice versa.
Both aperture and thickness can vary considerably along the trace, so these estimates
should not be counted together to a total width estimate.
-
8/16/2019 POSIVA 2002 22 Working Report Web
34/107
33
The aperture may partly or totally originate from drilling induced physical failure
(break-out) or washout of material between the surfaces, or even between closely
spaced several fractures, or from clay-filled or brecciated larger zone. f the
observation is linked to clearly collapsed or washed wide section (a narrow zone), the
edges have been mapped as separate observations. The fractures inside the zones have
been picked and classified only
if
they appear clearly. The image is the only
opportunity to get a direct openness indication
of
a fracture surface, as usually the
reconstruction of the core sample has no means to observe it; and there are rare n
s tu
indications on open fractures in other than hydraulic conductivity data. Figure
19
shows an example ofmeasuring the aperture and thickness.
The form and roughness
8
-
9)
of the surface have been described as a deviation
from the plane (from the sinusoid trace) in two separate scales. In the scale
of
the
wrapped-out image (200 - 250 mm), form 8) was analyzed. When the fracture trace
follows accurately enough the sinusoid
of
a plane, observation is planar .
f
the trace
deviates several millimeters in any point, it is undulating (i.e. curved). In case the
surface changes suddenly several millimeters, it is denoted as stepped . In the smaller
few millimeter scale, roughness 9) was analyzed. The fracture is smooth if there is
no observable deviation from the sinusoid, and otherwise rough . Examples
of
different forms of the fractures in different scales are shown in Figures 20 - 21.
The image observation is obtained from the side of the fracture plane, not from the
surface as in the core mapping, so the observations may not be quite comparable to the
surface roughness. Because the property is clearly observable, and also indicates the
accuracy of the plane fitting, it was recorded.
The colour 11 - 13) of fracture filling was assessed on three-level scale. Depending
on the colour and darkness of the background, and quality of the image, the colour
could be observed as
brightness 11 dark or light; especially when other colours cannot be seen)
grey intensity (12, white-grey-black)
colour dye (13, brown-red-yellow-green-blue).
In certain cases there are two or more separate colours, seen partially or layered on the
trace. From OPTV data the colour was observed from initial field data records, as in
the final data the contrast adjustment has altered the colours. In Figures 22 and 23
examples
of
the colour or grey intensity observation are shown.
Seepage 14) can be observed only when some material flows into the borehole from a
fracture and the colour of flowing material differs from the background. Outflow
cannot be observed. The flow from the fracture or along the borehole can be seen as a
curved fan on the image. The fan initiates from channels on fracture surface. t can be
guided towards the high side (light, warmer water) of the borehole, or to the low side
(heavier, cold water or material) and tur narrower before it vanishes within few tens
of
centimeters. A visual observation at close probe view indicated that such trace is a
turbulent flow of material in the water. t can also be a stain of material sedimented on
the wall over a longer time. Direction (upwards or downwards) has been marked for
specific fractures. The Figure 24 shows an example
of
seepage location.
-
8/16/2019 POSIVA 2002 22 Working Report Web
35/107
34
able 6
The parameters treated during mapping with allowed values.
No.
Property
Values omments
1
Level of
Probable, Drilling fractures at same ±
10
cm depth range, orientation
certainty
existing similar to the image observation within 30 degs, clear on
image
Possible,
Drilling fractures a t same ± 10 cm depth range, orientation
existing different from the image observation, and/or not clear on
image
Probable,
Drilling fractures not observed at same ± 10 cm depth range,
new or orientation clearly different to the image observation;
however clearly visible and fracture-like
Possible,
Drilling fractures are not observed at same depth range ea.
new ±
10
cm, or orientation is different to the
TV
observation,
and are not clearly observable from image
2
Openness Open Projections apart from each other
Partly open Part of surfaces apart from each other, part are closed when
seen in the observation scale
Not open Surfaces are adjacent in the observation scale
3
Filling With filling
Filling seen in image (coloured pixels, different from
background)
No filling
No filling seen in image ( in observation scale)
4
Alteration Altered
Fracture lines are discoloured or disintegrated (rust, etc).
Fresh Fracture lines intact, no colour changes
5
Tightness
Not closed
Surfaces are either apart, separated with some material, or
weathering is observed
Closed
In the observation scale 0,25- 0 5 mm) the surfaces are
closed, there is no filling and fracture is not weathered.
Excludes the others.
Filling thickness
Measured from central part of trace (in mm)
7
Aperture
Central part of trace, for partly open from the open part (in
mm)
8
Shape Planar
On image width scale
undulating
stepped
9
Roughness Smooth
On few mm scale
Rough
10
Mineral Possible
An estimate, not stored n final data
mineral
11
Darkness Dark
Only when image dark and no color or grey scale can be
Light
estimated
12
Grey intensity
Black Other than colour dye
Grey
White
13
Colour dye Yellow
Other than grey intensity
Red
Green
Brown
14
Seepage
Upwards Material flow into borehole and its direction
Downwards
No
-
8/16/2019 POSIVA 2002 22 Working Report Web
36/107
35
PTV
e
1:2
E
N
9
Drill obs tract
7JD
Figure 11 Existing and probable observation KR14, 72 80 73.10 m green sinusoid
and tadpole). Similar core fracture black tadpole) is observed close to the same depth.
The trace is clear and continuous on image.
-
8/16/2019 POSIVA 2002 22 Working Report Web
37/107
36
epth
PlV
e
1:2
r
N
E
N
0
90
Drill s fract
90
Figure 12a. Existing and possible observation KR14, 73.60- 73.80
m,
green sinusoid
and tadpole). A core fracture is observed close to the same depth black tadpole). The
trace on image is a bit vague, and its continuity uncertain a white undulating line).
The dip is steep; the dip direction o a steep fracture can easily turn 180 degrees
in
a
vertical borehole
i
he feature is undulating; real dip difference is approx. 3 0 degrees
over the vertical.
-
8/16/2019 POSIVA 2002 22 Working Report Web
38/107
37
OPl\1
:2
N
N
N s
Jtl
N
Figure 12b Existing and possible observation KR14, 73.60 73.80 m without the
sinusoid curve. The red arrows clearly indicate the undulating white line, a possible
fracture with filling. The real reported fracture can be at slightly different position
i
re-opened.
-
8/16/2019 POSIVA 2002 22 Working Report Web
39/107
38
Pmjection 11 9
igure 13a A new and probable observation KR9, 70.00 70.20 m . Similar core
fractures are not observed near to the same depth, but the observation is clear on
image. The fracture clearly
is
there, and typically when checking from the core sample
the observation was confirmed. It is possible that a welded fracture has not been
reported in drilling report although it could have been observed i broken apart. The
form deviates significantly from planar see arrows
on
Figure 13b).
-
8/16/2019 POSIVA 2002 22 Working Report Web
40/107
39
Depth
OPTV
:2
E
s
w
Projection
E s w
Figure 13b. New and probable observation KR9, 70.00 70.20 m without the
sinusoid curve. The arrows indicate the position where the continuous, undulating line
is best observed on image.
-
8/16/2019 POSIVA 2002 22 Working Report Web
41/107
4
Pmj
ectjon 1 9
Figure 14a New and possible observation KR9, 71.55-71.75 m, black line and
tadpole, on sparsely fractured rock . Similar core fractures are not observed close to
the same depth, and the observation is not very clear on image. It is possible that there
is a mica plate originated continuity on core, or a hair crack i seen on image is not
penetrative; or the fracture has not been observed
on
the core mapping. The checking
o these features on the core either led to rejection
o
observation, but
in
few cases a
new real fracture has been added to the database.
-
8/16/2019 POSIVA 2002 22 Working Report Web
42/107
4
epth
PTV
:2
E
s
w
Projection
E
s
w
71 6
Figure 14b. New nd possible observation KR9, 71.55-71.75 m) without the sinusoid
curve. The arrows indicate where the faint trace
of
possible hair crack has been seen
on image black, continuous undulating line between feldspar grains).
-
8/16/2019 POSIVA 2002 22 Working Report Web
43/107
42
Figure 15a An open fracture with filling
KR9, 13 7
55
13
7
7
5
m.).
The arrow
shows the location where some filling material has been observed. The filling is not
penetrative in this case and may have partly washed out during drilling.
-
8/16/2019 POSIVA 2002 22 Working Report Web
44/107
Depth
:2
137 6
43
E
PTV
s
w
Figure 15b. An open fracture, with fi lling KR9, 137.55 137.75 m). The sinusoid and
arrow removed so the trace is more clearly seen.
-
8/16/2019 POSIVA 2002 22 Working Report Web
45/107
Figure 15c An open fracture with sinusoid curve, no visible filling KR12, 713.35
713.55). There is some indication
o
the drilling debris lain on bottom
o
the surface,
but no compact filling between the surfaces. Either filling did not exist on this location,
or has been completely washed away.
-
8/16/2019 POSIVA 2002 22 Working Report Web
46/107
Depth
:2
713 4
45
OPTV
s
w
N
Figure 15d
n
open fracture without sinusoid curve, no visible fill ing KR12, 713.35
7
.55). The same image as in Figure 15a.
-
8/16/2019 POSIVA 2002 22 Working Report Web
47/107
6
Figure 16a A partly open fracture, with filling KR12, 738.35- 738.50 m . There
is
clearly compact filling calcite?) between the fracture surfaces, and
p rt of
he
fracture trace is clearly open on North left) side.
-
8/16/2019 POSIVA 2002 22 Working Report Web
48/107
7
Depth
PTV
~ ~
:2
s
w
738 4
Figure 16b A partly open fracture, with filling KR12, 738.35- 738.50
m .
The same
image as on Figure 16b.
-
8/16/2019 POSIVA 2002 22 Working Report Web
49/107
8
Figure 16c A partly open fracture with sinusoid curve, no visible filling KR12,
713.15- 713.35 . The aperture is clearly seen but no indication
o
any filling material
is present.
-
8/16/2019 POSIVA 2002 22 Working Report Web
50/107
49
epth
PTV
:2
~ ~
N
s
w
N
713 .2
Figure 16d A partly open fracture without sinusoid curve, no filling KR12, 713.15
713.35). The same image as
in
Figure
16c
-
8/16/2019 POSIVA 2002 22 Working Report Web
51/107
50
Figure 17a
A fracture with filling, neither open nor partly open KR9, 142.65
142.80
m).
The filling, light in colour, can be seen on west right)
p rt
ofthe trace.
In
the observation scale, there cannot be seen any aperture or breakout fracture
is
healed).
-
8/16/2019 POSIVA 2002 22 Working Report Web
52/107
epth
:2
N
5
E
OPTV
w
N
Figure 17b. A fracture with filling, neither open nor partly open KR9,
142 65
142.80
m .
The same image as in Figure17
a.
-
8/16/2019 POSIVA 2002 22 Working Report Web
53/107
52
epth
OPTV
1:2
r
N E S W N
PROJE TION
N
E
s w N
Figure 18a
A closed fracture KR9, 41.70-41.90
m)
with sinusoid curve. There is a
narrow curved crack trace cutting the mineral grains that does not allow any
aperture or filling material to be observed.
-
8/16/2019 POSIVA 2002 22 Working Report Web
54/107
5
epth
OPTV
2
s
w
4 B
Figure 18b A closed fracture KR9,
41
.70-41.90 m) without sinusoid curve. The red
arrows show the trace. There is no aperture or filling visible on the trace length. This
does not exclude the possibility
o
illing observed on the surface, or a minor less than
0.25 mm) aperture being present.
-
8/16/2019 POSIVA 2002 22 Working Report Web
55/107
54
Figure 19a The measurement principle o aperture KRJ2, 94.95 95.20 m .
The
reading
is
taken from the mid part o the trace, between the surfaces apart in the
image.
-
8/16/2019 POSIVA 2002 22 Working Report Web
56/107
Figure 19b The measurement principle of thickness KR12,
74.80
75.00 m . The
reading is taken from the mid par t
of
he trace, over the filling material.
-
8/16/2019 POSIVA 2002 22 Working Report Web
57/107
56
Figure 20a Fracture form in image width scale 200 mm), planar KR9, 147.85
148.05 m with sinusoid curve. The form follows nicely the sinusoid curve over the
image width.
-
8/16/2019 POSIVA 2002 22 Working Report Web
58/107
Depth
:2
148.0
E
57
OPTV
s
w
igure
20b.
Fracture form in image width scale 200 mm), planar
KR9,
147.85
148. 05 m) without sinusoid curve. The same image as in Figure 20a.
-
8/16/2019 POSIVA 2002 22 Working Report Web
59/107
~
8
Figure 20c
Fracture form
in
image width scale 200 mm), undulating KR12, 65.55-
65.80 m with sinusoid curve. The trace form is clearly deviating from the sinusoid
curve o plane projection.
-
8/16/2019 POSIVA 2002 22 Working Report Web
60/107
59
Depth
OPTV
1:2
1 N E S W N
6: 6
Figure 20d Fracture form in image width scale 200 mm), undulating KR12, 65 55
65.80
m
without sinusoid curve. The image is same as
in
Figure 20c.
-
8/16/2019 POSIVA 2002 22 Working Report Web
61/107
6
Figure 20e
Fracture form in image width scale 200 mm), stepped fracture KR12
61.35 61.66 m with sinusoid curve. There is clearly a step probable brittle minor
fault) at the middle
o
the trace. A differently oriented minor crack seems
to
cut the
fracture mapped.
-
8/16/2019 POSIVA 2002 22 Working Report Web
62/107
61
Dep h
OPl\1
1 2
61 6
Figure 20f. Fracture form in image width scale 200 mm), stepped fracture KR12
61.35- 61.66 m without sinusoid curve.
-
8/16/2019 POSIVA 2002 22 Working Report Web
63/107
6
Figure 2
a
Fracture form
in
local, mm scale smooth KR12, 66.00 66.10 m with
sinusoid curve. The surface
is
even, no deviation from planar form is seen.
OPTV
1:2
E s
w
Figure
2lb
Fracture form
in
local, mm scale smooth KR12,
66 00
66.10
m
without
sinusoid curve. The same image as
in
Figure 21
a.
-
8/16/2019 POSIVA 2002 22 Working Report Web
64/107
6
igure 21
c.
Fracture form in local, mm scale rough fracture KR12, 62.15 62.35 m
with sinusoid curve. The local f w mm variation on the surface from the planar
projection is clearly seen.
-
8/16/2019 POSIVA 2002 22 Working Report Web
65/107
64
Depth
PTV
N
E
s
w
N
igure
2 d
Fracture form
in
local, mm scale rough fracture KR12, 62.15 62.35 m)
without sinusoid curve. The same image as in Figure
21 c
-
8/16/2019 POSIVA 2002 22 Working Report Web
66/107
6
Figure 22a A white fracture KRJ , 370.00- 370.20
m
with sinusoid curve. The filling
material seen between the surfaces is white calcite, kaolinite?)
in
eo/or.
-
8/16/2019 POSIVA 2002 22 Working Report Web
67/107
Depth
BIPS
N s
w
Figure 22b A white fracture KRJ, 370.00- 370.20
m
without sinusoid curve. The
same image as in Figure 22a.
N
-
8/16/2019 POSIVA 2002 22 Working Report Web
68/107
7
Figure 23a
A grey fracture
KR2, 313.9 314.15 m)
with sinusoid curve. The dark
grey eo/or
of
illing between the surfaces is clearly seen quartz, chlorite?).
-
8/16/2019 POSIVA 2002 22 Working Report Web
69/107
epth
1:2
314.0
N
E
68
IP
s
w
Figure 3
b A grey fracture
KR2,
313 9 314 15
m)
without sinusoid curve The
same image as in Figure 23a
N
-
8/16/2019 POSIVA 2002 22 Working Report Web
70/107
9
Figure 24a
A location where material flows into the borehole (KR9,
280.54
280.82
m) with sinusoid curve. There is a fan ofmaterial flowing upwards, tending to reach
the high side
of
he borehole (north), and a thicker line reaching to the down side
(south)
of
he borehole, flowing downwards. The first is probably soluble material and
water flowing, the latter probably solid material rending to depth, or heavier water
fraction.
-
8/16/2019 POSIVA 2002 22 Working Report Web
71/107
Depth
m:2m R)
N
200 8
7
E
PTV
s
w
Figure 24b A location where materia/flows into the borehole K.R9, 280.54 280.82
m without sinusoid curve. The same image as
in
Figure 24a.
N
-
8/16/2019 POSIVA 2002 22 Working Report Web
72/107
71
There was no attempt to observe existence
of
an alteration rim around the fracture trace
or to measure its thickness. Neither were assessed the filling properties (grain size,
compactness, clay, carbonate, quartz) as these were considered to be best mapped from
the core. Both can be estimated from the image to some extent, but the latter not with a
certainty.
4 2 The distribution of mapping results according to level of confidence
The original mapping resulted in 7933 fractures for 3050 m, see Table 7 for
observations in each borehole before checking.
Table
7
The distribution and amount o ractures before checking
K.Rl, KR2,
KR4 KR9
KR12,
KR13,N
KR14,
N( ) N( ) N( ) N( )
N( )
(%) N( )
Existing/ 226 (60)
98 (27) 99 (41) 887 (71) 1797 (71) 1073 (67) 615 (40)
probable
Existing/ 86 (23)
90 (25) 81 (33) 134 (11) 321 (13)
205 (13)
110 (7)
possible
New/
14
(4)
101 (28) 38 (16) 104 (8) 201 (8) 155 (10) 171(11)
probable
New/ 52 (14) 77 (21) 26 (11) 124 (10)
227 (9) 161 (10)
660 (42)
possible
Probable 240 (63) 199 (54) 137 (56) 991 (79) 1998 (78) 1228 (77) 786(51)
Possible 138 (37) 167 (46) 107 (44) 258 (21) 548 (22) 366 (23)
770 (49)
Total 378 366 244 1249 2546
1594 1556
Obs. length 267.5 201 276 559 751
494 502
m
Observations 1.41 1.82 0.88 2.23 3.39
3.23 3.10
/m
Fractures/m 1.42
1.68 0.85
2.24 3.62 3.77
1.54
(drilling)
Initial fracture frequencies are similar to those observed in the core mapping. The host
rock sections (outside defined fracture zones) in KRl, KR2 and KR4 indicate less
fractures than the completely mapped other boreholes. Less fractured KR14 is an
exception in terms
of
comparison with the core mapping data.
The proportions
of
probable and possible features distribute interestingly. The BIP
mapped boreholes KRl, KR2 and KR4 show fewer probable observations
(54-
63%)
than the OPTV mapped KR9, KR12, KR13 (77-79%).
An
exception
of
this trend is
KR14 (51%), which is least fractured and was mapped by a different person. Also the
image is poor due to stick-slip interference and dirty water. Class existing/ possible
is more frequent
(23-
33%) in BIP image mapping than in OPTV mapping (7-13%).
For new fractures there is more variation in BIP image results (4-28%) than in
OPTV (8-11 %, except new possible 42% in KR14). These may arise from the
correctness
of
the depth adjustment in BIP images or core sample.
-
8/16/2019 POSIVA 2002 22 Working Report Web
73/107
72
The certainty class was used to decide which borehole sections would be checked over
with the core sample.
t
appeared that the better resolution
o
OPTV image allows to
observe the features with greater certainty, although the relative amount
o
the
observations does not depend so much on the image source.
n
analysis
o
the different
certainty classes it was observed that the possible observations are more often
closed or with filling than the others. So the checking against the core sample was
focused into existing/possible , new/possible and new/probable , leaving the
existing/probable that was already linked to the core sample mapping for lesser
interest as it had external confirmation from the drilling data.
-
8/16/2019 POSIVA 2002 22 Working Report Web
74/107
73
CHECKING THE OBSERVATIONS WITH THE CORE SAMPLES
5 1
The checking procedures
The observations were checked towards the core samples at the core sample archive
of
Geological Survey of Finland in Loppi (boreholes KRl, KR2, KR4, KR9 and KR12),
and at Olkiluoto (KR13 and KR14). All the observations of classes 'New, Possible
and New, Probable were checked systematically as well as most
of
the observations
Existing, Possible .
The images and results were compared with the samples. The results
of
the first
checked borehole (KR2) were analyzed to allow guidance of the remaining work.
Checking required typically a day for 300- 400 observations. The rate depended on
fracture frequency, proportion
of
observations to be checked, rock type, quality
of
image and the accuracy
of
the depth adjustment. The checked fractures received status
probable , and are indicated also with a label confirmed in the final database. The
others have a label unchecked . Rejected not a fracture -observations have been
removed from the final fracture lists. Influence
of
checking is presented in Table 8.
5.2
The results of the checking
After the checking 6138 fractures remained in the data (78% of the initial amount).
Generally some 78-88%
of
observations remained, except for KR4 (62%) and KR14
(5lo/o).
Table
8
Influence
o
checking
Inspection
KRl,
KR2, KR4, KR9, KR12, KR13,
KR14,
N( )
N o/o) N( )
N( )
N( ) N( ) N( )
Initially
378 366
244 1249 2546 1594 1556
Final
295 (78)
321 (88) 148 (61) 1026 (82) 2228 1342 (84)
778 (51)
(88)
Checked 153 (40) 213 (58) 151 (62) 386 (31) 804 (32) 535 (34) 969 (63)
Rejected 83 (22) 58 (16)
96 (39) 223 (18) 317(12)
252 (16) 770 (50)
Rejected
of
54% 27% 64% 58% 39% 47% 79%
checked
Exist/Cert 2 (1%, 1 (0%,
3 (3%, 13 1 %,
15 (1%, 10
1
%, 27 (4%,
rejected N=226) N=98) N=99) N= 887) N=1797) N=1073) N=604)
Exist/ uncert
36 (42%,
14 (16%, 48 (59%, 74 (55%, 99 (31%, 78 (38%, 63 (57%,
rejected N=86) N=90) N=81) N=134) N=321)
N= 205) N=llO)
New/cert 5 (36%,
11 11 %,
21
(55%, 44 (42%, 51 (25%, 59 (38 %, 95 (34%,
rejected N=14) N=lOl) N=38)
N=104) N=201) N=155) N=278)
New/uncert 40 (77%, 32 (42%,
24 (92%, 92 (74%,
152 105 (65%,
585 91 %,
rejected
N=52) N=77)
N=26) N=124) (67%, N=161) N=644)
N=227)
New,
0
13
(4%)
0 0
1 (0%)
0
12 (1.5%)
confirmed
Frequency
1.10
1.60
0.54 1.84 pes/m 2.97 2.72 1.55
pes/m pes/m
pes/m pes/m pes/m pes/m
Drilling
1.42
1.68
0.85 2.24 pes/m 3.62 3.77 pes/m 1.54
frequency pes/m pes/m pes/m pes/m pes/m
-
8/16/2019 POSIVA 2002 22 Working Report Web
75/107
74
Varying by borehole some 40-62% of the observations were checked from BIP, and
from the checked ones 27-64% were rejected, the others confirmed. For KR9-KR13
OPTV 31 - 34% were checked, and 39-58% of the checked ones were rejected, others
were confirmed. In KR14 63%
of
observations was checked and 79% of the checked
ones were rejected, the remaining 21% confirmed. Typically the rejected fractures
represented rather types closed or fractures with filling . Any of the rejected
fractures were
of
types open or partly open .
The fractures classified as Existing, Probable were checked only occasionally (2-3%)
especially when a depth error or disorientation of the core sample were suspected. A
proportion of 0-4%
of
all were rejected (some one-third of the checked ones in this
class). Table 9 shows the proportion of fractures in the certainty classes after checking.
The properties probable and possible practically lost their meaning in checking.
The few possible observations are related to locations where the sample has been
missing. The greatest remaining uncertainty is found for observations initially
belonging to the class possible , as these have not been checked as extensively as the
others. Generally these are linked to similarly oriented core mapping fractures at the
same depth level and usually are very clear in the image. The information has not been
merged in this work. According to tentative observation some 1 o of all the features in
this class would change when checked, mostly at locations with depth or orientation
errors.
n
any case the core mapping and image mapping would produce slightly
different results due to e.g. accuracy reasons.
The proportion 6 - 14% of new fractures suggests, that there are some fractures
unobserved in the core sample mapping. Some
of
these may barely indicate
an
inadequate depth value in core reconstruction (deviation from the image depth
adjustment), or an uncorrected drift on image depth value.
Table 9 Certainty classes after checking Those rejected are not counted or in the
proportions The possible ones confirmed have been transferred to probable class
Borehole/ KRl
KR
KR4
KR9 KR12 KR13
KR14
Certainty (N=295) (N=321) (N=148) (N=1026) (N=2228)
(N=1342)
(N=778)
Existing/ 272 148 134
91
%) 943 (92%) 2029 1197 662 (85%)
Probable
(92 ) (46%) (91 ) (89 )
Existing/ 5 (2%)
30 (9%) 2 (1%) 3 (0%) 3 (0.1%)
7 (1%) 7 (1%)
Possible
New/ 14 (5%)
130
11
(7%) 74 (7%) 190 (8.5%) 133 (10%)
105 (13%)
Probable (40%)
New/ 4 (1%)
13
(4%) 1 (1%)
5 (0%)
6 (0.3%)
3 (0%) 4 (1%)
Possible
-
8/16/2019 POSIVA 2002 22 Working Report Web
76/107
75
RESULTS
6 1
Contents of the results
n
total 613 8 fractures were included into the final results after checking. The
frequencies and amount represent 81%
of
the core sample fractures (63% - 100% for
different boreholes). Lowest proportion is found in KR4 (63%). Reason might emerge
from image quality or fracture type distribution, or accuracy in the image adjustment.
Highest proportions (95% and 100%) are in KR2 (BIP) and KR14 (OPTV). The former
was checked first and in more detail than the others. From the latter smaller scale and
more detailed possible fractures were mapped resulting to a greater amount of rejected
observations at the checking phase. The proportion for other boreholes is 77 - 82%.
There are probably some 0-5% new observations in different boreholes. The new
fractures may be drilling induced, from core loss areas (not from triple-tube drilled
KR13 and KR14), or features that have not been reported from sample because
of
being closed, but can be mapped from image.
The coverage of previous BIP interpretation (Strahle 1996) was checked for
comparison. Mapping has covered in average 43% of the core mapping reported
fractures, varying between 22 - 60% depending on borehole and depth interval.
Proportions of observed fractures were less near to surface where the fracture
frequency is highest. Mapping in 1996 did not utilize the core mapping data but was
based on image data alone, and recorded only the most clear indications.
6.2
Fracture type distributions
The fracture type distribution was analyzed. The open , partly open and with
filling types can exist simultaneously forming five major classes whereas the sixth
major class closed is excluding the others by definition. The class altered is met
only in boreholes KR2 and KR13, probably reflecting local variation in bedrock
conditions. Distribution of types in results are in Table 10 and in Figures 25 - 32.
Table 10 Fracture type distributions
Borehole/
KRl KR2
KR4 KR9
KR 2
KR 3
KR 4 All
Types
N=295 N=321
N=148 N=1026 N=2228 N=1338 N=778 N=6134
Open
0 (0%) 0 (0%) 1 (0.6%) 6 (0.6%)
15
(0.7%) 29 (2.2%) 5 (0.6%) 56
(0.9%)
Partly 0 (0%) 0 (0%) 0 (0%) 16 56 (2.5%) 45 (3.4%)
18
135
open
(1.6%)
(2.3%) (2.2%)
Open,
2 (1%)
1 (0.3%)
2 (1.2%)
1 (0.1 %) 2 (0.1 %) 3 (0.2%) 3 (0.4%)
14
with
(0.2%)
fillin2
Partly 0 (0%) 3 (1%) 10
13
25 (1.1%) 45 3 .3%)
19
115
open, with
(6.8%)
(1.3%) (2.4%) (1.9%)
fillin2
With
181
256
114 646 1400 915
536
4048
fillin2
(61%)
(80%)
(77%) (63%) (62