Two solenoid guide system for horizontal boreholes

BACKGROUND OF THE INVENTION

The present invention relates to a method and apparatus for tracking and guiding the drilling of a borehole, and more particularly to tracking a borehole being drilled generally horizontally under an obstacle such as a river, a highway, a railroad, or an airport runway, where access to the ground above the borehole is difficult or perhaps not possible.

Various well-known drilling techniques have been used in the placement of underground transmission lines, communication lines, pipelines, or the like through or beneath obstacles of various types. In order to traverse the obstacle, the borehole must be tunneled underneath the obstacle from an entry point on the Earth's surface to a desired exit point, the borehole then receiving a casing, for example, for use as a pipeline or for receiving cables for use as power transmission lines, communication lines, or the like. In the drilling of such boreholes, it is important to maintain them on a carefully controlled track following a prescribed drilling proposal, for often the borehole must remain within a right of way as it passes under the obstacle and its entry and exit points on opposite sides of the obstacle, must often be within precisely defined areas.

Prior systems, such as those illustrated in U.S. Pat. No. 4,875,014 issued to Roberts and Walters and U.S. Pat. No. 3,712,391 issued to Coyne, have provided guidance in the drilling of boreholes, but in some circumstances have presented problems to the user since they require access to the land above the path to be followed by the borehole to permit placement of surface grids or other guidance systems. Often, however, access to this land is not available; furthermore, the placement of guidance systems of this kind can be extremely time consuming, and thus expensive. The Earth's magnetic field is usually utilized for determining azimuthal direction, in such prior systems, but this creates additional problems because of the disturbances caused by nearby steel objects such as bridges, vehicular traffic and trains.

Other systems, typified by the system described in U.S. Pat. No. 4,710,708 to Rorden and Moore, provide to methods for guiding a drill in which the relative location of magnetic dipole transmitters with respect to magnetic field receivers is determined by measuring the magnetic field signals generated by the dipoles. In the system of this patent, for example, data is processed using unsynchronized clocks to derive amplitude and phase information from sinusoidally varying magnetic signals. These amplitude and relative phase signals are used to determine location and direction parameters of interest in a computational fitting procedure of successive approximation, using a gradient projection method. The application of this method to several configurations of practical interest is described in the '708 patent.

In addition, U.S. Pat. Nos. 5,485,089, 5,589,775 and 5,923,170 to Kuckes disclose methods for determining the lateral distance and orientation between substantially parallel boreholes using a solenoid powered by direct current together with an industry standard measurement while drilling (MWD) tool. U.S. Pat. No. 5,513,710 discloses a drilling guidance method for drilling boreholes under rivers and other obstacles using a direct current powered solenoid and an industry standard MWD system.

Although such prior systems are useful in various drilling guidance applications, it has been found that in many situations, increased precision and accuracy is needed.

SUMMARY OF THE INVENTION

The present invention is directed to an improved method and apparatus for providing guidance in drilling boreholes. The invention disclosed herein uses a localized electromagnetic source, which is oriented with respect to gravity, to generate magnetic fields. Vector components of this generated field are measured at a remote location with a system of sensors whose orientation with respect to the direction of gravity is known. The magnetic field measurements are analyzed mathematically to determine the azimuthal orientation of the sensors with respect to the azimuthal orientation of the source, and to determine the distance and inclination angle from the sensors to the magnetic field source.

The apparatus of the invention employs a magnetic field source that is oriented with respect to gravity and generates two mutually perpendicular, horizontal dipole magnetic fields whose polarity is periodically reversed by precise clock signals. Measuring instruments, also controlled by precise clock signals, at a remote location include three vector component alternating magnetic field sensors to measure the magnetic fields produced by the field source and three vector component gravity sensors to measure the direction of gravity relative to the measured vector components of the magnetic fields. Analysis of the magnetic field measurements gives a three dimensional sensor location with respect to the source location, and provides the azimuthal direction of the measuring instrument axes relative to the azimuthal direction of the magnetic dipole axes.

When the method of the invention is applied to drilling a borehole along a planned path, the measuring instrument package is deployed downhole, in the borehole and near the drill bit, as part of a measurement while drilling (MWD) assembly and the solenoid source is positioned at a known uphole location with respect to the planned borehole path, preferably on the Earth's surface above the path. After approximately every 10 meters of drilling, the drilling process conventionally is stopped to add a new segment of drill pipe. During this down period the required measurements and analysis required by the present invention can be carried out. This usually requires only a few minutes, during which time the solenoid source is powered in two perpendicular azimuthal orientations, the measurement data are gathered,and the measurements are analyzed. The distance and direction to the downhole instrument package and the orientation of the downhole coordinate system relative to the uphole coordinate system of the solenoid source are determined from the downhole magnetic field and gravity measurements. By comparing the measured location and orientation with the planned borehole trajectory specifications, up/down and left/right drilling direction adjustment recommendations for the next segment of drilling are provided to the driller at each measuring station. Tests at an industrial site with a system based upon the preferred embodiment disclosed herein gave useful results for drilling guidance out to a 150 meter spherical radius from the source location.

Although the invention will be described herein with respect to the drilling guidance of certain boreholes, various other applications of the disclosed method and apparatus will become apparent. For example, the system of the invention may be used in the precise determination of the paths of existing boreholes, the determination of locations in mines with reference to a surface location, or the relative location determinations which arise in tunnel construction. In certain applications, where only a few location and direction evaluations are required, enhanced range for the present system is readily provided by overnight or even longer signal averaging.

BRIEF DESCRIPTION OF THE DRAWINGS

The foregoing and additional objects, features and advantages of the present invention will be apparent to those of skill in the art from a consideration of the following detailed description of a preferred embodiment thereof, taken in conjunction with the accompanying drawings, in which:

FIG. 1

is a diagrammatic illustration of a drill guidance system utilizing the invention for guiding the drilling of a horizontal borehole following a proposed path to a proposed punch out point;

FIG. 2

is a diagrammatic illustration of a solenoid and turntable beacon showing provisions for setting the azimuthal orientation and for leveling the solenoid source;

FIG. 3

is a diagrammatic illustration showing the electronic circuitry configuration powering the solenoid source;

FIGS. 4A and 4B

are diagrammatic illustrations showing the waveforms of the clock control signal and the solenoid current flow vs. time, respectively;

FIG. 5

is a diagrammatic illustration showing components of the alternating magnetic field and gravity measuring system;

FIGS. 6A-6C

are a flow diagram of the process of the present invention for computing the distance and direction from a field source to the measuring instruments;

FIG. 7

is a diagrammatic illustration showing the relationship of vector quantities which enter into the mathematical analysis of the fields;

FIG. 8

is a diagrammatic illustration of the vector relationships between the instrument package xyz coordinate system, the downhole hsrsg coordinate system, the drilling direction which is the z axis of the instrument package, and the location vectors RSrcSens and r;

FIG. 9

is a diagrammatic illustration of the vector relationships from the source to an arbitrary point on the proposal path; and

FIG. 10

is a diagrammatic illustration showing an alternative two solenoid source which allows simultaneous generation of the two dipole magnetic fields.

DESCRIPTION OF PREFERRED EMBODIMENTS

One embodiment of the apparatus utilized in the method of the present invention in a borehole drilling application for the laying of pipeline under a river is illustrated at

10

in

FIG. 1. A

borehole

12

is illustrated as being drilled using an industry standard drilling motor

14

and drill rig

16

. The crossing of river

18

may entail drilling along a planned path

20

at a depth of 20 meters, for example, to a planned exit location

22

, which may be 1000 to 1500 meters away from a borehole entry point

24

. A solenoid beacon

30

is shown at a river bank

32

, which in this case is the exit side of the river, the beacon being energized to produce magnetic fields that will provide the information needed to guide the drilling at each measurement station under the river and subsequently under the earth's surface

34

as drilling progresses toward the proposed exit location

22

. The drilling motor

14

is mounted on a drill stem

36

to drive drill bit

38

, in conventional manner, with an instrument package

40

, which includes a three component accelerometer to measure the direction of gravity and a three component magnetometer to measure alternating magnetic fields, mounted on the drill stem just above the drilling motor. These instruments may or may not be part of a conventional measurement while drilling (MWD) package.

The beacon source

30

is illustrated in greater detail in FIG.

2

. In the preferred form of the invention, the beacon is positioned and oriented by land surveying techniques at a selected, known location with respect to the planned path

20

and exit location

22

. The beacon may consist of a turntable

50

upon which a solenoid

52

is mounted. The turntable is mounted on a base

54

to rotate about an axis

56

made vertical by adjusting the lengths of base support legs

58

,

60

,

62

to thereby make the solenoid

52

horizontal at all azimuthal orientations as the turntable rotates. Any convenient method, such as the use of a spirit level, may be utilized for this purpose. The turntable can be set in two orientations perpendicular to each other by a pair of pins

64

and

66

at diametrically opposite locations on the turntable that fit into two pairs of holes

68

and

70

in an orientation ring

72

mounted on base

54

. This ring can be rotated about the turntable axis

56

and clamped at any orientation by clamps

74

and

76

. After the base

54

is leveled, the orientation of ring

72

is set by loosening clamping screws

78

and

80

on clamps

74

and

76

, rotating the solenoid

52

while sighting along its axis

82

to make it point toward a surveyed reference location such as location

84

in

FIG. 1

, and tightening the clamp screws. The axes and the location of the beacon can thus be fixed by a simple, field-friendly procedure.

The solenoid

52

is illustrated in

FIG. 3

as having a 23 kilogram laminated core

90

that, in a preferred embodiment, is 1.25 meters long. To provide the desired magnetic field, this solenoid may require 40 watts of power, for example, and this is supplied by a portable power supply such as a small, 12 volt lead acid battery

92

connected to a polarity reversing FET (field effect transistor) switch circuit

94

connected across the solenoid winding

96

. The direction of electric current flow in the solenoid winding is periodically reversed by a reference square wave with a precise cycle period of 0.5 seconds derived from clock signals

96

(

FIG. 4A

) generated by a crystal oscillator

98

having a frequency that is precise to a few parts per million. The solenoid current vs. time waveform illustrated at

100

in

FIG. 4B

produces a magnetic dipole field of alternating polarity Although the principles of physics governing the behavior of the magnetic fields used in the analysis to be described are those appropriate to time independent magnetic fields, it is desirable to repeatedly reverse the direction of current flow in the solenoid to allow precise separation of the solenoid field from the Earth's magnetic field and from instrumental and magnetic field noise. It is also possible to simply turn the solenoid current on and off and to record the field differences. In this case the amplitude of the alternating polarity component of the magnetic dipole and field produced will be one half that produced if the current is reversed.

A schematic diagram of the downhole measuring apparatus

40

is shown in

FIG. 5

as being connected via a borehole telemetry link

110

to an uphole drilling control room

112

at the drilling rig

16

on the Earth's surface. The control room has a computer

114

for processing the data received from the downhole electronics and a controller

116

for operating the drill. A power supply

118

is connected via link

110

to power the down hole measuring instruments and telemetry circuits and to permit them to receive data from the instruments and convert the data to computer input signals. The power supply link may be a wire inside the drill stem

36

leading to the downhole instruments

40

.

The downhole instrument package

40

includes a three vector component magnetometer

120

and a three vector component accelerometer

122

, each of which generates output signals with respect to an xyz set of axes. The z axis of the instrument package

40

is aligned with the borehole

12

being drilled, and the perpendicular x and y axes have a known orientation alignment to the drill face; i.e., to the direction of a bent housing in the drilling motor which controls the direction of drilling. Direct current is received from the power supply

118

on the surface to power the instruments. The magnetometer AC outputs are passed through band pass amplifiers

124

, and are multiplexed with the magnetometer DC outputs and the accelerometer outputs at multiplexer

126

, where the signals are converted from analog to digital form and finally put into a form suitable for telemetry to the surface. The timing for digitization and telemetry is generated by a downhole clock

128

controlled by a quartz crystal whose frequency is precise to a few parts per million.

Data Acquisition and Processing

After drilling has been stopped at a measurement station along the proposed borehole path, the solenoid

52

is set to a first orientation, and energized as described with respect to FIG.

3

. The resulting reversing field with an alternating polarity component is detected by magnetometers

120

, the resulting output signals are transmitted uphole, a few minutes of data are recorded, and a data file is generated. The solenoid

52

is then set to a perpendicular orientation by rotating the turntable 90°, is energized to create a reversing field which is detected, a second set of data are recorded, and a second data file is generated. During each set of measurements the downhole multiplexer circuitry sequentially samples the output voltages of the magnetometers and the accelerometers at fixed time intervals and telemeters the results to the surface computer

114

, which separates the gravity measurements at

130

from the Earth's field measurements at

132

and the AC field measurements at

134

. The relative time at which each measurement is made is precisely preserved by the position it has in the serial data stream being telemetered, and the gravity data and AC field data are stored at data files

136

and

138

, respectively. The computer

114

generates from the gravity data a single row, three column matrix gxyz with elements gx, gy and gz, which are the representation of the measured gravity g in the xyz coordinate system. From the magnetometer measurement data, two 3-column matrices h

1

and h

2

are generated. The first matrix hi has three columns h

1

x, h

1

y, and h

1

z which are tabulations of the time sequence of the digitized magnetometer measurement data from the first orientation of the solenoid. The second matrix h

2

has three columns h

2

x, h

2

y, and h

2

z which are tabulations of the time sequence of magnetic field measurements from the second orientation of the solenoid.

The first step for processing the recorded magnetic field data is the generation of a reference wave form which is time synchronized with the solenoid switching circuitry

94

, as illustrated in

FIGS. 6A-6C

. For the apparatus disclosed herein, this time synchronization should be updated approximately once per hour; in practice it is convenient to do this at each measurement station. Signal averaging the magnetic field data matrices h

1

and h

2

with respect to this reference wave form produces two single row, three column matrices, H

1

xyz and H

2

xyz, of the time averaged solenoid vector magnetic field components. The first matrix has the elements H

1

x, H

1

y, and H

1

z, and the second has elements H

2

x, H

2

y, and H

2

z, which are the xy and z vector components of the two generated solenoid fields. H

1

xyz and H

2

xyz are xyz coordinate system representations of the field vectors measured. In general, the digital signal averaging computation method applied to the measured magnetic field components has a one-to-one correspondence to a method using an analog lockin amplifier (for example an Ithaco model 3962). A lockin amplifier passes the input voltage signal through a band pass filter (functionally similar to the downhole band pass amplifiers

124

), multiplies the filtered signal with a time synchronized reference voltage waveform and averages the resulting voltage. The time average of randomly varying noise thus processed goes to zero after a long enough time, whereas the true signal component, which is synchronized with the reference waveform, produces a DC output proportional to the desired signal component. The reference waveform which is multiplied with the signal must have good time and polarity correlation with that of the signal. The lockin amplifier incorporates circuitry to generate this reference wave form from a user-supplied input reference voltage which has periodic rising or falling edges which have precisely the same period as the signal source excitation, i.e. the same period as the square wave controlling the solenoid current. To obtain optimum time overlap correlation between the signal and reference waveform, a manual adjustment is provided to adjust the time delay between the reference voltage edges supplied and the symmetric reference waveform generated by the instrument. A good procedure for making this adjustment is to process a strong, representative signal while adjusting the time shift to maximize the averaged output. This time shift adjustment and reference input are then left fixed and the signals of interest processed.

Generation of Reference Signal and Signal Averaging

More particularly, and as illustrated in the flow diagram of

FIGS. 6A-6C

, the first part of the digital procedure includes generating in computer

114

a symmetric reference waveform which is time-synchronized with the uphole solenoid source

52

. As illustrated in

FIG. 6A

, the signals (block

140

) detected by magnetometers

120

and accelerometers

122

and supplied to computer

114

are processed at block

142

to extract the clock signals of downhole clock

128

from the data sequence being transmitted. To determine an optimal time shift from the signals

140

at a given measuring station, the strongest signal of the six magnetic field vector components is selected and processed (block

144

) to find an optimal time shift. For this purpose, a reference waveform is defined, against which all six magnetic field components can be signal averaged. To choose the magnetic field components with the strongest signal, the average square of the six data columns, h

1

x, h

1

y . . . h

2

z, is computed, using the MATLAB function “mean” to perform the operations mean(h

1

. *h

1

) and mean(h

2

. *h

2

). From the six numbers thus found, the largest defines a column matrix of data, called hmax. The serial telemetry data stream locations assign a time to each of the measurements of hmax, and those times are put into a single column matrix called Timehmax. The functional form of the reference wave form to be used is cos(w*t), where w is the fundamental radian frequency of the source, i.e., w=2*pi/SrcPer, where SrcPer is the source period; i.e., 0.5 seconds.

Two single column reference test matrices are defined as Reftest

1

and Reftest

2

, as illustrated in

FIG. 6A

at block

146

:

RefTest

1

=cos(

w

*Timehmax) (Eq. 1)

Reftest

2

=cos(

w

*(Timehmax-SrcPer/4)) (Eq. 2)

RefTest

1

is a single column matrix evaluating cos(w*t) at the times Timehmax; i.e., the times at which the measurements of hmax were made according to the downhole clock. RefTest

2

is a second cosine reference wave form evaluated at times shifted by a quarter of the time period of the solenoid clock from RefTest

1

. Passing hmax through a “digital lockin”, first with reference function RefTest

1

and then with RefTest

2

, means doing the two following evaluations

HMaxRef

1

=2*mean(RefTest

1

.*hmax) (Eq. 3)

HMaxRef

2

=2*mean(RefTest

2

.*hmax) (Eq. 4)

A multiplication by 2 has been included in these definitions because the average value of (cos(w*t)){circumflex over ( )}2=½. The optimum time shift (TimeShft) indicated by these two choices of the reference functions RefTest

1

and RefTest

2

is computed (block

148

of FIG.

6

A):

TimeShft=(SrcPer/(2

*pi

))*

a tan

2(HMaxRefTest

1

,HMaxRefTest

2

) (Eq. 5)

where a tan

2

is the MATLAB 4 quadrant inverse tangent function.

As illustrated at block

150

, all six columns of the data are now signal averaged with respect to a cos(w*t) reference function with this time shift. The 3-column measurement matrix h

1

of field measurements at solenoid orientation

1

, has an associated 3-column time matrix Timeh

1

, giving the times at which each of the measurement values of the three column matrix h

1

was performed according to the downhole clock. The time shifted reference function is given and signal averaged field vector components (block

152

) are given by:

Refh1=cos(

w

*(Timeh

1

-TimeShft) (Eq. 6)

H

1

xyz

=2*mean(Refh

1

.*

h

1

) (Eq. 7)

Likewise, the measurements at solenoid orientation

2

are signal averaged with the same reference function with the same time shift i.e.:

Refh

2

=cos(

w

*Timeh

2

-TimeShft) (Eq. 8)

H

2

xyz

=2*mean(Refh

2

.*

h

2

) (Eq. 9)

H

1

xyz and H

2

xyz, the AC magnetic field data from the two positions of the solenoid, are each one row, 3-column matrices giving signal averaged values of h

1

x, h

1

y h

1

z and h

2

x, h

2

y and h

2

z with respect to the time shifted cosine reference function. H

1

xyz and H

2

xyz are the amplitudes of the fundamental Fourier frequency component of the respective xyz vector components of h

1

and h

2

. H

1

xyz and H

2

xyz are the representations of the magnetic field vectors H

1

and H

2

with respect to the xyz coordinate system defined by the instrument axes.

Use of a reference function of the form cos(w*t) in this manner gives the time projection of all the magnetic field vector component data onto a single reference function to give the signed cos(w*t) Fourier series amplitude of each vector component. This method of signal averaging does not give any relative phase information between the components which may be contained in the magnetic field measurement data.

Instead of generating time synchronization from the data, establishing direct time synchronization between the uphole and downhole clocks is sometimes the most appropriate method. This can be done by a wire or other telemetry link between the two sites. Alternatively, time signals can be derived from global positioning units or from WWV radio signals.

Magnetic Field Analysis

The notation and uphole configuration definitions for this analysis are shown in FIG.

7

. At the Earth's surface

34

, the two orientations for the solenoid

52

excitation, as illustrated by unit vectors m

1

and m

2

and these, together with the direction of the gravity unit vector g, define the surface coordinate system. RSrcSens is the vector from the origin

160

of the source coordinate system to the borehole sensors

40

near the drill bit and below the Earth's surface. The analysis begins by writing RSrcSens as a product of the magnitude of the vector R and a unit vector RUv, as follows:

RSrcSens=R*RUv (Eq.10)

The lower case vector r is the projection of RSrcSens onto the horizontal plane of the Earth's surface, i.e., the plane of the vectors m

1

and m

2

as shown in FIG.

7

.

Rm

1

m

2

g is the representation of RSrcSens in the m

1

, m

2

and g coordinate system, as illustrated in

FIG. 7

, and gives:

Rm

1

m

2

g=R

*(sin(

AgR

)*cos(

Am

1

r

)*

m

1

+sin(

AgR

)*sin(

Am

1

r

)*

m

2

+cos(

AgR

)*

g

) (Eq. 11)

The magnetic field vectors H

1

and H

2

at the sensors

40

, generated by the solenoids m

1

and m

2

, have strength m Ampere m{circumflex over ( )}

2

. Maxwell's equations give the generated fields as:

H

1

=(

m

/(4

*pi*R{circumflex over ( )}

3))*(3*dot(

m

1

,

RUv

)*

RUv−m

1

) (Eq. 12)

H

2

=(

m

/(4

*pi*R

{circumflex over ( )}3))*(3*dot(

m

2

,

RUv

)*

RUv−m

2

) (Eq. 13)

The “dot” functions appearing in equations (12) and (13) return the vector dot product of its two vector arguments. There are two “azimuthal” angles Am

1

r, i.e., the angle between m

1

and r (the horizontal projection of RSrcSens onto the horizontal plane) which give the same vectors H

1

and H

2

. They are:

A

m

1

r

=0.5

*a

tan 2(2*dot(

H

1

,

H

2

),(dot(

H

1

,

H

1

)−dot(

H

2

,

H

2

)) (Eq.

14

)

or

A

m

1

r

=0.5

*a

tan 2(2*dot(

H

1

,

H

2

),(dot(

H

1

,

H

1

)−dot(

H

2

,

H

2

))+

pi

(Eq. 15)

Since the vector dot product of two vectors does not depend upon the coordinate system in which their representations are defined, the Am

1

r can be found from the field measurement results, i.e.,

A

m

1

r

=0.5

*a

tan 2(2*dot(

H

1

xyz,H

2

xyz

),(dot(

H

1

xyz,H

1

xyz

)−dot(

H

2

xyz,H

2

xyz

)) (Eq. 16)

or

A

m

1

r

=0.5

*a

tan 2(2*dot(

H

1

xyz,H

2

xyz

),(dot(

H

1

xyz,H

1

xyz

)−dot(

H

2

xyz,H

2

xyz

))+

pi

(Eq. 17)

The quantities shown in Eq.16 and Eq.17 are computed from the data as indicated in block

170

. The correct value of Am

1

r is chosen from a knowledge of the approximate azimuthal location of the sensor package with respect to the source location.

The horizontal unit vector in the direction of r, rUv, can be written as

rUv

=cos(

Am

1

r

)*

m

1

+sin(

Am

1

r

)*

m

2

(Eq. 18)

The inclination angle AgR, is computed, as illustrated at block

172

, by forming the vector cross product of H

1

and H

2

(cross(H

1

,H

2

)) and dividing it by the total field quantity, dot(H

1

,H

1

)+dot(H

2

,H

2

) to give:

xH

=cross(

H

1

,

H

2

)/(dot(

H

1

,

H

1

)+dot(

H

2

,

H

2

)) (Eq. 19)

The vector xH lies in the plane of g and RSrcSens. To show this, compute cross (H

1

,H

2

) noting that m

1

, m

2

and g form a right handed coordinate system. When dot(cross(RrcSens,xH) is computed using Eq.(11) for RrcSens, a null result is obtained. Thus, xH must lie in the plane defined by RsrcSens, and g.

It is useful to write xH in terms of two components. The first is the projection of xH onto g and the part of xH which is perpendicular to g. Since xH is in the plane of g and R, xH can be written as sum of two vectors, one in the rUv direction and a second in the g direction:

xH=xHr+xHg*g=magxHr*rUv+xHg*g

(Eq. 20)

where:

xHg

=dot(

xH,g

)

xHr=xH−xHg*g

magxHr=mag

(

xHr

) (Eq. 21)

The MATLAB function “mag(A)” computes the magnitude of the vector A, which is sqrt(dot(A,A)). After some algebraic manipulation, the angle AgR can be written

AgR

=(½)*

a

tan 2(6

*magxHr

, 7

*xHg

+1) (Eq. 22)

Both xHg and magxHr are directly computable from the data, since the vector cross product and the vector dot product are both invariant to the coordinate systems of representation; that is:

xHxyz

=cross(

H

1

xyz,H

2

xyz

)/(dot(

H

1

xyz,H

1

xyz

)+dot(

H

2

xyz,H

2

xyz

)) (Eq .23)

xHg

=dot(

xHxyz,gxyz

) (Eq. 24)

xHrXyz=xHxyz−xHg*gxyz

magxHr=mag

(

xHxyz−xHg*gxyz

) (Eq. 25)

Thus, the angle AgR is computable from the measurements as noted in block

172

.

Finally, as indicated in block

174

, the distance R between the source and the sensor locations (RsreSens) can be related to the total field strength, as follows:

R

=((

m

/(4

*pi

)){circumflex over ( )}2*({fraction (7/2)}−({fraction (3/2)})*cos(2

*AgR

))/(dot(

H

1

,

H

1

)+dot(

H

2

,

H

2

)){circumflex over ( )}(⅙) (Eq. 26)

Again in terms of measurement representations of H

1

and H

2

, R can be written as

R

=((

m

/(4

*pi

)){circumflex over ( )}2*({fraction (7/2)}−({fraction (3/2)})*cos(2

*AgR

))/(dot(

H

1

xyz,H

1

xyz

)+dot(

H

2

xyz,H

2

xyz

)){circumflex over ( )}(⅙) (Eq. 27)

Thus, a systematic procedure has been disclosed to find from the measurement data the coordinate parameters of the vector RsrcSens; i.e., the distance R, the azimuth angle Am

1

r, and the inclination angle AgR.

Alternatively, the downhole coordinate system representation of RSrcSens may be called Rhsrsg, as illustrated in

FIG. 8

, wherein:

Rhsrsg=R

*(sin(

AgR

)*cos(

Ahsr

)*

hs

+sin(

AgR

)*sin(

Arsr

)*

rs

+cos(

AgR

)*

g

) (Eq. 28)

To determine Rhsrsg, the downhole representation parameters of RSrcSens in terms of the downhole coordinate system, it is necessary to find only the angle Ahsr, as illustrated in block

176

, since the angle AgR and R are the same in both representations. To find Ahsr (FIG.

8

), it is useful to evaluate projections of xHr onto the hs and rs axes. To do this, the unit vector representations of hs and rs in the instrument xyz coordinate system must first be found. Since the borehole drilling direction is in the z direction, in the xyz system z=[

0

0

1

], it is possible to define rs and hs unit vectors as:

rs

=cross(

gxyz

, [0 0 1])/mag(cross(

gxyz

, [0 0 1]) (Eq. 29)

hs

=cross(

rs,gxyz

) (Eq. 30)

The rs unit vector is horizontal and perpendicular to the direction of drilling and points to the right side looking down the borehole. The hs unit vector is horizontal and perpendicular to both g and rs. If the borehole inclination, that is its angle with respect to gravity is less than 90 degrees then hs is on the high side of the borehole and in the plane of g and the borehole. The unit vector hs is the horizontal projection of the borehole direction.

The angle Ahsr can be found from the expression:

Ahsr=a

tan 2(dot(

rs,xHrxyz

),dot(

hs,xHrxyz

)) (Eq. 31)

Thus, the parameters of Rhsrsg have also been found from the measurements.

Distance and Direction to Proposed Location

The planned drilling path, or proposal, is defined with respect to surface coordinates so that the vector RsrcProp (

FIG. 9

) from the source location

160

to an arbitrary location

180

on the proposal path

20

is readily written in terms of the m

1

m

2

g surface coordinate system (FIG.

7

), from the solenoid source location site

160

. The space vector from the sensor location

40

to a point

180

on the proposal RSensProp given by:

RSensProp=RSrcProp−RSrcSens

(Eq. 32)

All the coordinate quantities of RSensProp in the m

1

m

2

g coordinate system representation are thus known; that is, all the quantities in the equation:

RSensPropm

1

m

2

g=RSrcPropm

1

m

2

g−Rm

1

m

2

g

(Eq. 33)

are known. To guide further drilling, the vector from the sensors at the drill to a proposal point the coordinate quantities entering the down hole coordinate system representation, at sensor

40

, illustrated in

FIG. 9

as the hsrsg coordinate system of RsensProp, must be known. Since both the m

1

m

2

g system of FIG.

7

and the hsrsg systems of

FIG. 9

share the same g axis, the transformation from one system to the other is simply a rotation Rotm

1

m

2

gtohsrsg) about the g axis. The rotation angle is Am

1

hs=(Am

1

r-Ahsr). Thus noting that RSensPropm

1

m

2

g is a single row 3-column vector, and in MATLAB the transform of a matrix is denoted by “′”, the vector may be computed, as indicated at block

182

in

FIG. 6C

, as follows:

RSensProphsrsg

=(

Rotm

1

m

2

gtohsrsg*RSensPropm

1

m

2

g

′)′ (Eq. 34)

Rotm

1

m

2

gtohsrsg

=[cos(

Am

1

hs

) sin(

Am

1

hs

) 0;−sin(

Am

1

hs

) cos(

Am

1

hs

) 0; 0 0 1] (Eq. 35)

The parameters RSensTghsrsg in the downhole coordinate system have been all related to the measured quantities. Thus the driller can be presented with the proposal location and the direction of this proposal location with respect to the present drilling location and the direction of drilling, from which the drill bit tool face can be set to make the necessary adjustment to drilling direction.

Both the location of the downhole sensors and their relationship to the source can be determined without making use of gravity measurements. This is implied by the observation that, from the six measurements discussed above; i.e., the three vector components of H

1

and the three vector components of H

2

, it should be possible to determine the three vector components of the source location and the three quantities specifying the relative orientation of the downhole measurement system with respect to the source. Indeed, this computation is readily carried out. However, for a given precision of the magnetic field measurements the difference in precision of the computed quantities of interest is vastly different. The greatest improvement in accuracy is obtained by determining the vertical elevation of the borehole

12

relative to the source solenoids

52

, which is of dominant interest, for the guidance of pipeline boreholes. For example, if the apparatus disclosed herein is used with the borehole sensor

40

located 10 meters below the Earth's surface at a radial distance of 100 meters from the source

52

, with the measurements of H

1

and H

2

having +/−1% precision, the disclosed method yields an elevation of 10+/−0.7 meters. In contrast, using a purely electromagnetic method the useless value of 10+/−30 meters is found.

Determination of the right or left direction for this case, using the method disclosed, gives an expectation error of approximately ½ degree. This precision is better than can be expected operationally using conventional Earth magnetic field measurements. Allowing +/−2 degree errors in the location determination with a signal averaging time acceptable for drilling operations, the disclosed apparatus is useful at a range of about 150 meters.

An alternative source, which generates two independent dipole fields simultaneously, is illustrated at

190

in

FIG. 9

, wherein similar components carry the same identifying numerals as the apparatus of FIG.

2

. Source

190

consists of two horizontal solenoids

192

and

194

mounted perpendicular to one another and supported on the turntable

50

rotatably supported by base

54

to allow the solenoid pair to be oriented with respect to a surveyed landmark. Once this apparatus is leveled and oriented at a selected source location it remains stationary until deployment at a new source location becomes necessary. The solenoids can be powered simultaneously, each by a power source similar to that shown in

FIG. 3

but with different source time periods; for example, SrcPer

1

=0.4 seconds and SrcPer

2

=0.6 seconds. The data processing to evaluate the fields H

1

and H

2

generated in this way is similar to that disclosed above, except that only a single data file is obtained. It is first processed, as disclosed, looking for a signal with a period equal to SrcPer

1

and then a second time looking for a signal with source period equal to SrcPer

2

. Such a source beacon has important advantages; it is amenable to remote, unmanned operation and for a given measurement precision less than ½ the drill rig down time is usually required to capture the required data.

Although the invention has been described in terms of preferred embodiments, variations and modifications may be made without departing from the true spirit and scope thereof, as set out in the following claims.

Number	Name	Date	Kind
3712391	Coyne	Jan 1973	A
4710708	Rorden et al.	Dec 1987	A
4875014	Roberts et al.	Oct 1989	A
5258755	Kuckes	Nov 1993	A
5485089	Kuckes	Jan 1996	A
5513710	Kuckes	May 1996	A
5589775	Kuckes	Dec 1996	A
5923170	Kuckes	Jul 1999	A

Two solenoid guide system for horizontal boreholes

Information

Patent Number

Date Filed

Date Issued

Inventors

Original Assignees

Examiners

Agents

CPC

US Classifications

Field of Search

US

International Classifications

Term Extension

Abstract

Description

Claims

US Referenced Citations (8)