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Dynamic Data Analysis – v5.12.01 - © KAPPA 1988-2017

Chapter

3 – P ressure Transient Analysis (PTA)

- p63/743

3.B.3

Build-up response and Horner plot

The MDH plot, with the simple log(∆t) time function, results directly from the log

approximation to the drawdown solution for infinite-acting radial flow. In order to use semilog

analysis for any flow period other than the first drawdown, it is necessary to take into account

superposition effects.

How to get the Horner plot:

Build-up superposition:

 

 

t

t p t

p t p t

p

p DD

DD

p DD

BU

  

 

) (

IARF approximation:

 

 



S

rc

k

X

kh

qB

X p

wt

DD

8686 .0 228 .3

log

log

6. 162

) (

2

If

t is large enough to reach IARF, so will t

p

+

t. A lot of terms cancel out and we get:

Build-up superposition:

 

p DD

p

BU

t p

t

t

t

kh

qB

t

p





 

log

6. 162

) (

Rearranging:

 

 





 

p

p DD

p

p

BU

t

kh

q

t p

t

t

t t

kh

qB

t

p

log

6. 162

log

6. 162

) (

If the production time was too short, IARF was not reached during the flow period and ∆p

DD

(t

p

)

cannot be turned into a log approximation. The constant term on the right of the equation

becomes unknown. In this case, the analysis described below will give the permeability, but

not the skin factor. If the production time was long enough, then the term t

p

can also be

turned into a logarithmic approximation and we get:

IARF at t

p

:

 

 

 



S

rc

k

kh

qB

t

kh

qB

t p

wt

p

p DD

8686 .0 228 .3

log

6. 162

log

6. 162

2

So:

 





 

S

rc

k

t

t

t t

kh

qB

t

p

wt

p

p

BU

8686 .0 228 .3

log

log

6. 162

) (

2

We introduce the Horner Time as:

t

t

t t

p

p



Infinite-acting radial flow for a build-up is characterized by linearity between the pressure

response and the logarithm of Horner time. Drawing a straight line through this point gives a

slope and an intercept:

IARF straight line:

b

t

t

t t

mb

t

t

t t

kh

qB

Y

p

p

p

p







log

log

6. 162

If the producing time t

p

was long enough to reach IARF, the IARF approximation for a build-up

will be similar to the drawdown relation, replacing time by Horner time, and will be given by:

IARF for a build-up:

 





 

S

rc

k

t

t

t t

kh

qB

t

p

wt

p

p

BU

8686 .0 228 .3

log

log

6. 162

) (

2