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

Chapter

3 – P ressure Transient Analysis (PTA)

- p64/743

After transformation, we get the equation of the Horner plot straight line in terms of pressure:







 

t

t

t

kh

qB

p p

p

i

BU

log

6. 162

Permeability-thickness product and the skin are then calculated.

Permeability-thickness product:

mh

qB

k

6. 162

Skin factor if t

p

is large enough:



 

23.3

log

1

log

151 .1

2

1

wt

p

p

wf

hr

rc

k

t

t

m

p p

S

Note that the time function is such that the data plots ‘backwards’, as when ∆t is small, at the

start of the build-up, the Horner function (log (tp+∆t)/∆t) will be large, and when ∆t tends to

infinite shut-in time the Horner time tends to 1, the log of which is 0.

Fig. 3.B.3 – Horner plot

If the reservoir were truly infinite, the pressure would continue to build-up in infinite-acting

radial flow and eventually intercept the y-axis at pi, the initial pressure. However, as no

reservoir is infinite, the extrapolation of the radial flow line at infinite shut-in time is called p*,

which is simply an extrapolated pressure.

If the reservoir is infinite:

*

p p

i

It is important to notice that the calculation of the permeability is valid even in the case of a

short production before the shut-in, while the validity of the calculation of skin is conditioned

to a producing time long enough, so IARF was reached before t

p

.