The existence of shallow gas
reservoirs in the Miocene and Oligocene sands of southwest Mississippi and
the Florida Parishes of Louisiana was first revealed on modern seismic
data in the mid-1980's, when large grids of new 2D seismic data acquired
for the Lower Tuscaloosa Mid-Dip Stratigraphic Play - in southwest
Mississippi and the Florida Parishes of Louisiana - illuminated dozens of
probable "bright spots" and velocity anomalies in the shallow Tertiary
section. At first, the exploitation of these shallow gas sands was limited
to those areas located within a mile or two of existing gas pipelines, for
economic reasons. As pipeline infrastructure slowly expanded throughout
the region in the next 20 years, more and more of the shallow seismic
anomalies were targeted - especially in Amite and Wilkinson Counties in
Mississippi and West Feliciana Parish in Louisiana. These shallow gas
sands were predominantly Frio in age, but some Miocene reservoirs were
also discovered and developed. Results were mixed, with many gas
accumulations being rather small in volume and deliverability. Because
only two
significantly large (>5 BCF) fields were discovered in the first 15 years
of exploration - with the largest field establishing only 15 BCF of
recoverable reserves - interest was lost in the Wilkinson / Amite / West
Feliciana Parish Trend, and that play has been fairly dormant in the last
five years.

However, in 2000 an
intriguing discovery occurred far from the established trend as described
above. A Mississippi geologist, intrigued with the potential for shallow
gas production in localized patch reef build-ups of the Heterostegina
("Het") Limestone, utilized existing 2D seismic data to identify what
appeared to be a patch reef in the Het Lime on the west flank of Waveland
Field, a Lower Cretaceous (predominantly Mooringsport) gas field in
Hancock County, Mississippi. A subtle velocity "sag" that developed
beneath the anomaly was suggestive of shallow gas, because of the presumed
time delay attributed to the displacement of water in the reservoir by gas
- through which acoustic waves travel at much slower velocities. A Het
Lime test was drilled to investigate the anomaly, but the Het was
apparently devoid of hydrocarbons; however, a 28 foot-thick Miocene
sand located not far above the Het Lime was found to be gas-bearing and (as one
would expect, at 4,000 feet) very porous and permeable.
Casing was run and the well
was subsequently perforated across the Miocene Sand, later named the
"Amphistegina Sand" in recognition of the foraminifera associated with
that stratigraphic interval. Unlike the Tertiary gas completions further
to the west, this reservoir flowed at sustained rates in excess of
2,500,000 cubic feet of gas per day (> 2.5 MMCFGPD) with over 1,500 psi
flowing tubing pressure. In fact, aside from some downtime associated with
mechanical issues, this initial discovery - the #1
International Paper 7-5 - continued to produce 2
MMCFGPD with only a minor loss of reservoir pressure until February of
2004. The operator
successfully offset this well with a second gas producer (the
#1 International Paper 7-10) that also
encountered 29 net feet of gas pay and also potentialled at an approximate rate of
2.6
MMCFGPD.
Logs for the #1
International Paper 7-5 &
7-10 wells are shown immediately below.
Unfortunately, as of March
2004, two developmental offsets for the field area (subsequently named
"Mariner Field") have been plugged, and the #1
International Paper 7-10 watered out in December 2002;
and now (March 2004) the discovery well, the 7-5, is watering out. It appears that Mariner Field represents a
4 BCF combination structural/stratigraphic trap,
formed by the drape of the Amphistegina reservoir sand over a thick
underlying channel; and that the gas production has been
laterally swept by active water encroachment. Several other wildcats drilled in the immediate area have
been plugged. At this point in time (spring 2004), it would seem that
this young Trend is destined to "die on the vine" unless another
significant discovery is made in the near future. Check back with us in
the near future for further updates.


