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					 RESISTIVITY IMAGE LOGS 
 
					This page describes resistivity image 
					logs profiles, in the order of their appearance over the 
					years. This presentation style provides insights into tool 
					evolution, and a specific tool’s capabilities and 
					limitations. You will find most these tool types in your 
					well files – here’s your chance to learn more about them.
					 
					  
					In
                1986, the "ultimate" dipmeter was developed by
				Schlumberger, called
                the formation microscanner (FMS). Later versions were called
				formation micro-imager (FMI). There are now similar services
				available from other suppliers. The tool is generically known as
				a resistivity image log. Using an additional 27 electrodes
                on each of two dipmeter pads of the dipmeter; each pad records 27 microresistivity
                curves spaced 1/10 inch apart on the borehole surface. Each pad
                covers a 2.8 inch wide portion of the circumference of the well
                bore. Several passes over the interval will often provide virtually
                complete coverage of the rock face. The
                resistivity traces are translated into images based on their relative
                resistivity values, in either black and white or colour. The
                resistivity data provided by this tool are of very high resolution,
                in the order of a few millimeters. Thus, a substantially large
				data array must be handled, and it is an obvious challenge to
				process and display this information in a way which facilitates
				its interpretation. This is resolved through a point to point
				mapping of the resistivity traces into a spatial image, each
				pixel in the image display having a gray scale or colour value
				associated with a particular resistivity level. Subsequent
				interpretation benefits from the close relationship between this
				image and core photography. 
 The gray
                scale or colour spectrum can be stretched or squeezed in the computer
                to enhance certain features, such as porosity, fractures, or shale
                laminations. Images can be plotted at the same scale as the core
                photographs for comparison.
 
 It is traditional to show low resistivity (shales and open
				fractures) as black, shading to white for high resistivity
				(tight streaks and healed fractures). Porous sands and shaly
				sands will be grey or a mix of yellow-brown with darker colour
				suggesting higher resistivity and possibly lower porosity. In
				rare cases, such as tar sands and oil shale, the colours may be
				reversed to make hydrocarbon layers black and shales lighter
				colours.
 
				 Resistivity image log showing calculates dips, raw curves, and
                image log from a two pad FMS device.
 A
                resistivity image logging tool with fewer (sixteen) electrodes per pad, but
                with four or eight imaging pads, is now available, and provides
                better coverage of the wellbore wall than the two pad version.
                The electrodes are smaller, allowing for higher vertical resolution, but
                are spaced to provide the same wall face coverage, about 2.5 inches
                per pad. In an 8 inch diameter hole, electrode coverage is about
                80% and in a 6 inch hole is greater than 100%. This overcomes
                one of the major complaints about the FMS, namely the number of
                passes needed to obtain a complete image of the well bore. An
				example is shown below. 
			
			 Evolution of the Schlumberger resistivity image
			log pad design, starting with the original two pad FMS (located on 2
			of the 4 pads of the SHDT dipmeter), the four pad FMI (which could
			be twinned with another tool at 45 degree offset for better borehole
			coverage), and the eight pad FMI-HD tool (which gives about 98%
			coverage in an 8" boreho;e).
 
			 Four pad FMI log in fractured granite reservoir showing
                computed dip angle and direction. North is at centerline of
			image.
 
 
  An 8-pad FMI-HD log in a gas shale. Left track is static (fixed
			colour scale) image. Right track is dynamic image, in which a
			running average type of colour scaling is used to amplify
			resistivity contrasts, making easier to see stratigraphic features,
			faults, and fractures.
 The
                primary use of the tool is definition of bedding plane dips, for identification of irregular features,
                such as vugs and fractures, for accurate sand counts in thin bedded
                zones, and for identifying stratigraphic features. If sufficient
                rock face is imaged, dips can be found by digitizing the bedding
                planes visible on the microscanner image, or by automatic computation
                using all valid image traces.  The dips found by FMI dip processing
                are superior to CSB or LOC dips because a larger number of resistivity
                traces can be used in the calculation. They can be computed automatically
                and displayed on the FMS image. In addition, calculated dips can
                be edited or removed, and new bed boundary correlations picked
                with a mouse on an interactive CRT image. Thus dips that pass
                or fail preconceived processing criteria can be deleted or added
                as the analyst desires. Dip tadpoles can be coded by colour to
				indicate bedding, cross bedding, fractures, or faults. 
				
				 RESISTIVITY IMAGE LOG EXAMPLES Images
			courtesy of Schlumberger
 
				 Left track is caliper, right track is formation dips. Dip in
				the cross beds indicate paleocurrents to the WNW direction. This
				is confirmed by the imbricated shale clasts.
 Channel orientation is ESE to WNW
 
 
  Resistivity images are best dislayed horizontally for
				horizontal wells-- toe of the well is on the right. Top track is
				formation or fracture dips, bottom track is borehole deviation.
				Images illustrate fenestral porosity within a carbonate unit
				intersected by a horizontal well. Actual well productivity with
				this type of reservoir is higher than convention open hole logs
				would indicate.
 
 
  The slimhole FMS* provides imaging capabilities in boreholes
				as small a 114mm (4.5 in). This Image reveals a normal fault and
				fractures in a horizontal well. Fault block downthrown to the
				N45E direction with 63' dip.
 
 
 
 
 
 
 
 
			 Expanded colour scale image of tight streak (light
                brown) on resistivity image shows detail of porosity laminations
			- light colour is tight, darker colours are more porous, black is
			shale.
 
 
  Formation microscanner images in various environments
 
				 Formation microscanner images in various environments
 
 
				 RESISTIVITY IMAGE LOGS IN OIL-BASE MUD (OBM) SYSTEMS Material in this section is based on "Imaging - Getting the Picture
			Downhole" edited by Tony Smithson, Schlumberger Oilfield Review,
			Sept 2015.
 
 Conventional resistivity image logs require a conductive mud system
			to operate. In oil based (nonconductive) mud, a knife blade
			electrode, or "scratcher pad", version of the resistivity image log
			was available from several suppliers in the later 1980's. The
			scratcher systems worked reasonably well for bedding dips and sand
			counts, but could not see fractures very well, because they filled
			with nonconductive mud.
 
 Schlumberger
                introduced a new typw of oil-based mud imaging log (OBMI) for use in nonconductive
			mud systems in 1988. It uses micro induction resistivity
			measurements instead of the usual electrical resistivity pads. It
			had 4 pads with 2 rows of 4 electrodes on each pad, operating in the
			10 to 20 kiloHertz range. A second tool could be added at 45 degree
			offset to increase borehole coverage. Resolution vertically and
			horizontally was about 1 cm, much coarser than the conventional
			tools (FMS, FMI). It was not very effective in fractures and there
			were other artifacts that caused shadow events, making the image
			difficult to interpret in some cases.
 
 The micro-induction technique of
			older OBM imagers and scratchers of even older dipmeters have been
			replace by Schlumberger's  Quanta Geo tool. It makes a
			capacitive measurement at two frequencies in the megaHertz range
			(instead of the kiloHertz range used in conventional tools) and then
			derives the best image from the optimal frequency. The tool has 8
			pads so the coverage is good compared to other OBM tools. The
			electrodes are surrounded by guard electrodes that focus current
			through the mud and mudcale into the formation.
 
			
			 Core image (left), static and dynamic images from Quanta Geo
			image log
 The capacitive measurement allows
			the processing to determine the amplitude of the current / voltage
			ratio and the phase shift between the two measurements. The ratio
			gives the electrical impedance of the rocks. At the frequencies
			used, the impedance is not directly proportional to resistivity, but
			the images produced have the same general appearance as conventional
			image logs. Vertical resolution is 6 mm and horizontal resolution is
			3 mm, comparable to the FNI-HD in water based mud. Both open and
			healed fractures are quite evident on the Quanta Geo output as high
			resistivity (white) sinusoids. An acoustic image log uld be used to
			distinguish open from healed. 
			 Fractures (white sinusoids) in oil base mud using Quanta Geo image
			log. Open fractures cannot be distinguished from healed as both are
			resistive in OBM.
 
				
				
				 LOGGING
			WHILE DRILLING IMAGE LOGS Measuring
			resistivity at the drill bit is part of a normal logging while
			drilling operation. Three resistivity curves sampling different
			depths of investigation are sent uuole in real-time, along with any
			other logs in the tool string. Since the tools are rotating while
			drilling, the deep resistivity scans the entire wellbore as the tool
			moves slowly down hole. The scanned data is too much to send uphole
			in real-time and is recorded, then  recovered at the surface
			when the drill string is tripped for a bit change. Some newer RAB
			tools can transmit sufficient dats to create an image uphole for
			near real-time display. Once all the image data is assembled, it can
			be processed to obtain dip indoemation i a manor similar to wirekine
			image logs.
 Since the density log
			is also a directionally focused tool that rotates, it too can give
			an image, although with less contrast than resistivity. 
			 Deep resistivity image from a logging while drilling tool called
			Resistivity at Bit (RAB). As for all image logs, black represents
			low resistivity, white is high resistivity. North is at centerline
			of each image. Since this is a deep resistivity, light colours could
			mean hydrocarbons or low porosity. Comparison to an open hole FMI or
			an LWD density image log could resolve the ambiguity.
 
			
			
			 LWD density image log,  black is low density (shale or porous),
			white is high density (tight). Comparison to RAB
 can identify
			hydrocarbons: light colour on RAB + dark colour on density image =
			hydrocarbon. This image is from a
 horizontal well; bottom side of
			hole is at the centerline of the image.
 
 
  Typical Resistivity-At-Bit (RAB) image log shows gamma ray at
				left, resistivity image, dip tadpoles, and 3 resistivity curves
				on the right. This image illustrate open fractures (with blue
				traces) cross-cutting bedding (in green).
 
			  
			 IMAGE LOGS FROM DIPMETERS Dipmeters and image logs are an essential for assessing structure
			and stratigraphy of reservoir rocks and for Identification of
			fracture intensity and fracture porosity. Tool design has improved
			considerably since its introduction in 1986.
 A
                resistivity image log has about 10 times the spatial resolution of an
				acoustic image log
                and 500 times the amplitude resolution, due to the difference
                in contrast between the resistivity and acoustic impedance ranges
                measured by the respective tools.  The
			standard tool works only in conductive mud in open hole, and a
			specialized tool is available for non-conductive mud. It does not
			work in cased holes. An extension of the
				stratigraphic high resolution dipmeter (SHDT) processing provides a core-like image
                of the borehole, using the LOC dip correlations and the measured
                resistivity curves. The program is called STRATIM (Schlumberger
                trademark). This image predates the resistivity image log by a
				few years. 
				 An
                example is given on the left. The program produces a 360 degree
                image of the borehole wall by interpolating between the eight
                resistivity measurements from the eight electrodes on the SHDT
                pads. Images can be coded in gray scale or colour. Dark gray or
                dark colour usually represents conductive, often tight shale,
                beds and light colour resistive, often porous sand, beds. If shales
                are more resistive than sands (or carbonates), the colour scheme
                can be reversed to keep shales looking dark. The dipmeter curves are rotated to their true azimuth but are
                not adjusted to true dip. The dips seen on the image are as they
                would appear on the surface of a conventional core. The trace
                of a plane dipping bed forms a sinusoidal curve when the image
                of the borehole wall is unwrapped and laid flat, as they are in
                these images. Bed boundaries, dipping beds, slump features, and
                fractures are easily seen, if present. Images can be enhanced
                as in Formation Microscanner processing, but processing is cheaper
                because much less data is manipulated.
   A
                similar program, called DIPVUE is available from Western Atlas,
                illustrated below. Here the 3-D image can be rotated in real
				time to view the artificial "core" from any direction. In addition, most core service companies
                can provide core photographs and dip logs from core data for comparison
                with log derived borehole images.  The
			colour convention is to show low resistivity in black and high
			resistivity in white (or yellow). This makes shale beds black and
			clean sands white, with shades of grey or brown representing shaly
			sands. In carbonates, the same rules are used, but white may now
			mean tight streaks with grey representing porosity. The colour scale
			can be stretched and squeezed to enhance the image for a particular
			situation. Note
			that a planar, dipping, bedding plane will trace a sine wave on a
			circumferential image, such as those shown above 
				 DIPVUE image created from dipmeter data
   
				  
			
				 RESISTIVITY IMAGES FROM
			MODERN LATEROLOGS Azimuthal resistivity image logs
			(a form of laterolog) and high resolution laterologs can be
			displayed as images as well as resistivity curves. 
			Below is a sample of an array induction (AIT) log and an azimuthal
			resistivity (AIR) log, the latter showing the azimuthal image log
			presentation.
 
			   Comparison of array induction log (left) and azimuthal resistivity laterolog (right). Curve complement and
			presentations vary considerable with age and contractor. The image
			log on the azimuthal resistivity presentation is "poor man's"
			resistivity microscanner log, giving a reasonable sand count 
			regional dip, and some fracture information. A real microscanner
			image is shown for comparison (left image).
 
			 High resolution laterolog showing deep invasion and high
			resolution image.
			All curves are focused to
 about 8 inches. This tool is not azimuthal so image shows flat-lying
			beds even when dip is present.fs
 
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