Hydrocarbon Correction for Neutrondensity log. Respond of neutron and formation density log in HC bearing. How to correct them? Hydrocarbon Correction for Neutrondensity log. Respond of neutron and formation density log in HC bearing. How to correct them? Hydrocarbon Correction for Neutrondensity log. Respond of neutron and formation density log in HC bearing. How to correct them?
Trang 1R E S P O N S E O F N E U T R O N
HYDROCARBON B E A R I N G FORMATIONS
by
R GAYMARD and A POUPON SPE Schlumberger - P a r i s
EDITOR’S NOTE: In this interesting paper the authors
consider the effect of residual hydrocarbons on the re-
s p o n s e of the Neutron a n d Formation Density logs I t
should be o f interest to those working with t h e s e poros-
ity tools P o s s i b l e applications a r e included for both
shaly formations o r complex lithologies
ABSTRACT
I t is usually assumed that, in oil bearing formations,
the Neutron and Formation Density logs are not signifi-
cantly affected by the residual oil in the invaded zone
and that they respond a s if t h e volume investigated was
entirely filled with mud filtrate However when porosities
a r e fairly high, t h e effect of t h i s residual oil is not
always negligible, particularly if the oil is light
Computations have been made t o evaluate t h i s effect
Formulae have been developed for clean oil or g a s
bearing formations T h e s e formulae permit a more accu-
rate evaluation of the porosity Some of the formulae may
a l s o have application in the cases of shaly formations
and of complex lithologies
EFFECT OF HYDROCARBONS
ON THE NEUTRON LOG
In Neutron logging, a source emits fast neutrons into
the formation T h e s e neutrons a r e slowed down through
collisions, mostly with hydrogen nuclei of t h e surround-
ing medium, and after reaching the so-called thermal
level of energy, a r e absorbed by nuclei of the formation,
usually hydrogen or chlorine nuclei; e a c h capture of a
thermal neutron is followed by t h e emission of gamma-
rays of capture A detector, a t some distance from the
neutron source, measures either t h e gamma-rays of
capture (Neutron-Gamma type of tool) or the thermal
neutrons (Neutron-Thermal Neutron tool) or the neu-
trons before they have reached t h e thermal l e v e l (Neutron-Epithermal Neutron tool) For all tools, the slowing down of t h e fast neutrons by hydrogen nuclei is
t h e predominant phenomenon, and t h e reading, for given hole conditions, depends mostly on t h e hydrogen index
of the formation, proportional t o the quantity of hydrogen per unit volume of formation near the bore hole
In clean water bearing formations, the hydrogen is found in the water only, and with a concentration which
is practically independent from the combined effects of temperature and pressure; in t h e s e conditions t h e Neutron reading is directly related to porosity Hydrocarbons, like water, contain hydrogen, but a t variable concentra- tions which depend mostly on the density of the hydro- carbons in situ For some oils, the hydrogen concentra- tion will be practically the same a s in water; but g a s and light oil have substantially lower hydrogen concen- trations As a result the presence of gas, or light oil, in
t h e volume of formation near the bore hole, is likely to have a substantial effect on the Neutron reading
L e t Srh : residual hydrocarbon saturation in invaded
zone
= : hydrogen index of the hydrocarbons : hydrogen index of t h e mud filtrate
If the Neutron log is calibrated in fresh water bearing formations, we can write:
Neutron log porosity = + [ a s , h + p (1 - S,, ) ] (1)
T h e hydrogen index of fresh water is 1, by definition; the hydrogen index of a sodium chloride solution i s somewhat smaller than 1
It will be assumed in t h e following that the Neutron log is calibrated through cross-plots Neutron-Formation Density or Neutron-Resistivity in water bearing inter- vals; then one can write:
a
Trang 2E F F E C T O F HYDROCARBONS
ON THE FORMATION DENSITY LOG
D o l o m i t e CaCO,!MgCO, 2.870
Gamma r a y s of fairly high energy l e v e l a r e emitted
by a r a d i o a c t i v e s o u r c e T h e i r i n t e n s i t y i s gradually
a t t e n u a t e d through c o l l i s i o n s with t h e e l e c t r o n s in t h e
formation (Compton effect) T h e Schlumberger Formation
D e n s i t y l o g i s b a s e d on t h e measurement of t h e gamma
ray d e c a y e d i n t e n s i t y a t a given d i s t a n c e from t h e
s o u r c e
C 0.9985 0.9991 0.9977 0.9990 1.1101 1.0797 1.1407
As t h e Compton e f f e c t i s proportional t o t h e number of
e l e c t r o n s per unit volume and as, i n f i r s t approximation,
t h e number of e l e c t r o n s per unit volume i s proportional t o
t h e d e n s i t y of t h e formation, i t i s c l e a r t h a t t h e log
r e s p o n d s t o t h e d e n s i t y of t h e formation
Actually t h e number of e l e c t r o n s per unit volume i s
not e x a c t l y proportional t o t h e d e n s i t y In t h e case of a n
e l e m e n t , if w e c a l l p b t h e true d e n s i t y and p e t h e ((elec-
tronic density)) t o which t h e s o n d e r e s p o n d s , i t c a n b e
shown that:
Z Z = atomic number
A A = a t o m i c weight
with C = 2- w h e r e
Similar r e l a t i o n s h i p s e x i s t for compounds p e d i f f e r s
from pb only t o t h e e x t e n t t h a t C i s not e x a c t l y e q u a l
t o 1
For most of t h e e l e m e n t s and compounds found in
sedimentary formations C i s very c l o s e t o o n e , a s shown
in t a b l e s herebelow:
Element
H
C
0
N O
S I
C I
Ca
A
1.008 12.011 16.000 22.99 28.09 35.46 40.08
1
6
R
1 1
1 4
1.9841 ,9991
1 oooo ,9569 ,9968 ,9588 ,9980
T h e r a t h e r l a r g e d e p a r t u r e from 1 which a p p e a r s for
o i l and w a t e r i s d u e t o t h e p r e s e n c e of hydrogen, t h e C
of which is almost e q u a l to 2
To c o p e with t h i s problem t h e tool r e s p o n s e is
c a l i b r a t e d i n c l e a n f r e s h w a t e r bearing l i m e s t o n e s with
p o r o s i t i e s ranging from z e r o t o 40%; in fresh w a t e r bearing dolomites or s a n d s t o n e s , t h e error r e s u l t i n g from
t h i s c a l i b r a t i o n is very s m a l l , and e n t i r e l y negligidle
F o r fresh w a t e r bearing l i m e s t o n e t h e s t a n d a r d formula
r e l a t i n g d e n s i t y t o porosity c a n b e written both for true
d e n s i t y and for e l e c t r o n i c d e n s i t y :
(5)
By virtue of formula (3), equation (5) writes:
By eliminating 4 between (4) and (6), then r e p l a c i n g
p L s , p w , C I S and C w by their numerical v a l u e s , we g e t :
pb = 1.07 p , - 0.188
S i n c e t h e l o g i s c a l i b r a t e d in s u c h a way t h a t p
p b in fresh water bearing l i m e s t o n e s , it r e s u l t s that:
=
l o g
P l o g = 1.07 p , - 0.188 (7)
T h i s , t h e n , i s t h e r e l a t i o n s h i p , between t h e e l e c t r o n i c
d e n s i t y and t h e reading of t h e Formation D e n s i t y log
L e t u s now revert to our problem and c o n s i d e r a c l e a n hydrocarbon bearing formation T h e fluid in t h e i n v e s -
t i g a t e d z o n e i s made up of Srh % of hydrocarbon and (1 - S r h ) % of mud filtrate E q u a t i o n s (7) and (6) write:
where C m a p,,, C m , p m f and C h p h a r e r e s p e c t i v e l y t h e
e l e c t r o n i c d e n s i t i e s of t h e matrix, of t h e mud f i l t r a t e and
of t h e hydrocarbons
By eliminating p , between (7) and (8), and noticing
t h a t :
= 1.07 Cma p,, - 0.188
pmo
Trang 3w e get the relationship between pb (log reading) and 4
(true porosity):
T h e apparent porosity $,, derived from the Density
log, by definition:
p m a - p b
4 D = , is given by:
p m a - P m f
INFLUENCE O F MUD SALINITY
T h e following parameters, used in formulae (2) and
(lo), depend on mud filtrate salinity:
P mud filtrate hydrogen index,
p m f mud filtrate density,
C, pd mud filtrate electronic density
We s h a l l l i m i t our study t o the case where the mud
filtrate c a n be considered as a pure N a C l solution
In the formulae the filtrate salinity will b e given a s
a function of the parameter:
N a C l Concentration (ppm)
P =
1,000,000
T h e following approximate formulae have been es-
blished:
(11)
p = 1 - 4 P
INFLUENCE O F HYDROCARBON DENSITY
a On Neutron log
In formula (2) above (Neutron equation) D( is the
hydrogen index of the hydrocarbons or, more precisely,
t h e ratio of the hydrogen content per unit volume of
hydrocarbons over that of water It c a n b e shown that D(
is given by the following formula:
where nH is the proportion of hydrogen by weight in the
hydrocarbons
By plotting nH v s ph for a number of saturated hydro-
carbons (C,H,, + ,) under average reservoir conditions,
and assuming the heaviest components to have a density
of 0.9, we have obtained the following empirical formula:
For methane which h a s a density of 0.2 f 25% under most of reservoir conditions, t h e formula gives nH =
0.25, the correct figure, i f one t a k e s ph = 0.2
For heavy oil, i.e p h = 0.9, the formula gives nH =
0.15, which is a good approximation s i n c e the lower
l i m i t for heavy saturated hydrocarbons is:
1
7
- 0,143
By eliminating nH between (14) and (15), we obtain
= as a function of p,only:
(16)
2
a = 9 p, f0.15 + 0.2 (0.9- p,) 1 Graphical study of t h i s third degree function shows that i t can reasonably b e assimilated to two different linear functions, depending on t h e range of P, values ( s e e fig 1):
- if 0.25 p h < 0.9, i.e practically for oil, we can write:
- if p,< 0.25, i.e practically for gas, we can write:
b On Formation Density log
In formula (lo), C, p h is the electronic density of the hydrocarbons C, is related t o nH through the fol- lowing simple formula:
Taking (14) into account, we get:
c, p, - (1 + rlH) p, = x +
9 p h
i f 0.25 4 p h < 0.9 using the expression of O( given by (17), we find:
c h p h = 1.11 ph + 0.03
- if ph < 0.25 with 0: = 2 2 p h , we find:
C, ph = 1.24 p ,
Trang 4d RELATIONSHIP BETWEEN DENSITY OF HYDROCARBONS A N D THEIR HYDROGEN INDEX
( H index)
G E N E R A L F O R M U L A E EXPRESSING T H E E F F E C T
OF R E S I D U A L H Y D R O C A R B O N S A T U R A T I O N O N
N E U T R O N A N D F O R M A T I O N D E N S I T Y LOGS
a Neutron log
I t is a s s u m e d i n t h e following t h a t t h e Neutron l o g
i s c a l i b r a t e d t o g i v e t h e t r u e porosity in c l e a n i n t e r v a l s
w h e r e t h e r e is mud f i l t r a t e only, with n o r e s i d u a l hydro-
c a r b o n s If a n i n t e r v a l c o n t a i n s r e s i d u a l hydrocarbons,
t h e a p p a r e n t Neutron porosity + N will n o longer b e e q u a l
t o t h e t r u e porosity 4 :
T h e v a l u e of A& i s readily found by combining
r e l a t i o n s h i p s (2), i l l ) , (17) or (18), and (23):
for oil:
for g a s :
b Formation Density l o g
T h e p r e s e n c e of r e s i d u a l h y d r o c a r b o n s i n s t e a d of mud f i l t r a t e c a u s e s a variation Ap, of t h e log reading,
a n d a s a r e s u l t t h e apparent porosity q5D differs from
t h e true porosity 4
T h e e x p r e s s i o n s of Apb and ApD are found by com- bining e q u a t i o n s (9) or (19), (12), (13), (21) or (22), and (26)
for o i l :
(28)
+ 1.07 4 Srh [1.11 (1 - ph) + 65 P - .031
A + D =
p , - 1 - .7 P for g a s :
A p b = - 1.07 4 S r h [1.11 + 65 P - 1.24 p h l (29)
(30)
+ 1.07 4 S , h [ l l l + 65 P - 1.24 p h I
A 4 D =
p , - 1 - .7 P
F i g u r e s 2 and 3 are a graphical representation of t h e and Ap, r e l a t i o n s h i p s
Trang 5EFFECT OF HYDROCARBON ON NEUTRON LOG
A@,,, CHART
I
TRUE POROSITY 4 = 28%
EXAMPLE RESIDUAL HYDROCARBON
HYDROCARBON DENSITY Qh = 0-2
SATURATION srh = 60 % "N -s*5%
FILTRATE S A L I N I T Y 200.000 P P M THE NEUTRON LOG READS = 28 - 8.5 = 19.5 %
I
0 0 0
FIGURE 2
PRACTICAL APPLICATIONS
The final Neutron and Formation Density formulae
(24), (25), (27), (28), (29) and (30) look somewhat com-
plicated, but charts based on these formulae are easy
to use, a s will be illustrated on a few typical cases
a Clean sands ( p g = 2.65) containing hydrocarbons with
known p h
Let u s assume, for example, that the density of the
mud filtrate pf = 1, and that ph = .114 (this is the c a s e
of gas with a hydrogen index of 25)
From (25) w e derive:
From (29):
p b = 2.65- 1.65 4-1.04 4 S,, (32)
On a cross-plot of r,bN versus pb, the lines for con- stant values of + and for constant values of Srh are straight line The chart (fig 4) is practically the same
a s chart 40-1 in the Schlumberger Paris Chart Book of
1966
Similar charts can be made for other values of ph ( s e e fig 5 for ph = S )
Similar charts can also be made for clean limestones
(pma = 2.71) or dolomites (pma = 2.87)
Trang 6EFBECU OF HYDROCARBON OM FORMATOOM DENSITY LOG
AQb CHART
RESIDUAL HYDROCARBON SATURATION S,h= 75%
TRUE POROSITY 6 = 21%
I
EXAMPLE HYDROCARBON DENSITY ph ~ 0 6
I FILTRATE SALINITY 150.000 P P M
b Clean Sands containing hydrocarbons of unknown ph
FIGURE 3
I t c a n b e shown that, t o a good approximation, regard-
l e s s of t h e v a l u e of ph:
Therefore, t o e v a l u a t e 4, we n e e d t o make an assump-
about Srh F o r t u n a t e l y t h i s assumption i s not c r i t i c a l
We c a n then c a l c u l a t e a v a l u e of ph which is e x p r e s s e d
a s a function of Srh and 0 = C , S ~ / + , in t h e following
e q u a t i o n s :
for oil:
for g a s :
T h e whole p r o c e s s i s s o l v e d graphically by figure 6
T h e more a c c u r a t e v a l u e of S r h which is n e e d e d t o
d e r i v e p h from t h e s e c o n d part of t h e c h a r t is c a l c u l a t e d from:
.62 Rm,
6 2 1 5 ( 1 - SrJ2
R x o =
c Hydrocarbon bearing shaly sands
Formulae (24), (25), (27) and (29) remain valid in
s h a l y formations T h e s e formulae s h o w t h a t t h e often
u s e d method of deriving a v a l u e of s h a l e c o n t e n t V s h
Trang 730%
20%
10%
a
I
60;
40%,
\
'
2
FIGURE 4
EFFECT O F GAS O N N-FDC C O M B I N A T I O N
1.65
1.25 1.114
I o
30%
20%
10%
A
I
z
7
FIGURE 5
EFFECT O F LIGHT OIL ON N - F D C COMBINATION
t
9
SANDSTOb
HYDROCAfi FRESH M U
\
2 6 5
m (X - a e -
P f = 1 0
D N D E N S I l Y f h = 0 5
I
Trang 8L
f
0
a
Trang 9SYMBOLS USED ABOUT T H E AUTHORS
T h i s paper h a s been written using a new set of
symbols which follows as closely as possible the
standard API list We apologize for t h e inconvenience
t h i s will certainly c a u s e those who are accustomed to
t h e old system, but we felt that the change had to b e
made:
Physical Parameters:
R resistivity
p density
q5 porosity
S fluid saturation
V proportion by volume
a hydrogen index of hydrocarbons
hydrogen index of t h e mud filtrate
ppm N a C l
P =
1,000,000
Subscripts:
s h s h a l e
Under t h i s system we have t h e following equivalence
t o the old list:
ROS Sro Residual oil saturation
RGS Srg Residual g a s saturation
Srh Residual hydrocarbon sat
Matrix (Grain) density
p, p m a
Mr R Gaymard graduated in 1947 from Ecole Polytechnique, Paris, and in 1948 from Ecole Nationale Supgrieure du P&- role, near Paris, with a Petroleum Engineering degree During
1948-1951 he was drilling and Production Engineer for SN REPAL, Algeria He joined Schlumberger in 1951 and was assigned successively to SWSC (U.S.), Surenco (South Ameri- ca), SPES (Europe and Africa) and Schlumberger Overseas (Libya)
He is presently working a t the Sales Interpretation Department
of Schlumberger, Paris, headquarters where he is i n charge of Computer Processed Interpretation
i
Andre Poupon graduated in 1933 from Ecole Polytechnique in Paris After one year of military service and three years with P
the French Railroad, he joined Schlumberger at the end of
1937 He worked in the field in Trinidad, France, and Vene- <
zuela and was transferred to Schlumberger’s research center I
I
Mr Poupon moved to Paris in September, 1955, to work in the
J Tittman and J S Wahl: “The physical Foundations of Interpretation Department of S.P.E Schlumberger He is at
P
of formation
1
REFERENCES
I
I
Trang 10through a cross-plot of q5N versus pb gives Vsh values
that are too low in formations containing light oil In
gas beaiing formation the error on Vsh could be quite
large On the other hand, i f a reliable value of shale
content can be estimated independently of the Neutron
and Density logs (Gamma Ray, or SP, or Resistivity),
q5N and C$D can be corrected Then:
- if ph is known the clean sand charts (such a s those of
fig 4 and 5) can be used t o derive q5 and Srh;
- i f ph is not known the chart of fig 6 can be used to
estimate q5 and p h
chart indicates a porosity of 25% and the probable lithology is 50% h e s t o n e + 50% dolomite, with a grain density of 2.79
If that same formation contains hydrocarbons, both the Neutron and Density readings will be affected Let
us assume p = .55 and Srh = 40%
h
From (24) we find, for P = 0 (fresh mud):
d Complex lithologies: determination of q5 and p,,
In wate'r bearing mixtures of sand, limestone and
dolomite, with no shale, the porosity and approximate
grain density can be derived from a cross-plot of pb
versus q5N, such a s that of fig 7 which corresponds to
pf = 1 (chart 42 of the Schlumberger Paris Chart Book of
1966) For example, for C$N = 26% and pb = 2.34, the
the apparent Neutron porosity then is 26 - .015 = .245
or 24.5%
From (27)
A p b = - 1.07 X .25 X .40 (.S- .033) =-.05
2.1
2.2
2.3
2.4
2.5
2.6
2.7
2.8
2.9
3 0
COMPLEX LITHOLOGY FIGURE 7
f
porosity )
the bulk density reading is 05 gr/cc too low, and is equal to:
2.34 - .05 = 2.29
The point for q5N = 24.5% and pb = 2.29 on the chart
of fig 7 falls exactly on the line corresponding to pure limestone, and indicates an apparent porosity of 24.5%
Due to the effect of the residual hydrocarbons, then, the estimated porosity is very slightly in error, and the estimated grain density is appreciably off, 2.71 instead
of 2.79 At low porosities the hydrocarbon effect would
be negligible
From this example, it can be concluded that in for- mations containing light oil, when the porosities range from medium to high, the residual hydrocarbons are not likely to have much effect on the porosity determination, but lithology cross-plots cannot be satisfactorily in- terpreted without taking into account the effect of the residual hydrocarbons The correction for residual hydrocarbons, needed for a correct determination of the
lithology can be made only if ph is known and i f an R x o
log is available to give an approximate value of Sr,