Mr. Anthony Zelen reports
LONGHORN EXPLORATION CORP. ANNOUNCES COMPLETION OF AMT SURVEY
AT THE FAME GOLD PROPERTY
Longhorn Exploration Corp.
has completed a
geophysical survey on the Fame property (located approximately 82 kilometres southwest of
Williams Lake, B.C.) in July, 2024.
The geophysical team conducted a Volterra-AMT survey that complemented the data generated from
the 2022 magnetometer and VLF (very low frequency) airborne survey. The team created a 3-D
model of both the AMT and IP resistivity showing anomalously high and low numbers. Based on the
results of the airborne and ground geophysical surveys targets may be delineated for future
exploration.
The Fame property consists of 11 contiguous mining titles and covers an area of 3,200 hectares. It
hosts several mineral showings consisting of mineralization that have been classified as epithermal
gold. The main target type on the Fame property is an epithermal gold deposit. The 2012 IP survey
that was conducted over most of the known showings was successful in delineating zones of higher
chargeability, which may relate to zones of disseminated pyrite or other sulphides; higher resistivity,
which may relate to either intrusions or zones of silicification; in addition to providing depth profiles
of targets.
The development of this work program is based on the information generated by the analysis of
previous work completed on the Fame property, combined with the 2022 completed airborne
geophysical survey.
A low resistivity, subvertical structure appears in the AMT data which correlates well with the low
resistivity area in the IP interpretation. It also trends north-northwest at the same location low
resistivity; subvertical structure appears in the AMT data which correlates well with the low
resistivity area in the IP interpretation. It also trends north-northwest at the same location.
A low resistivity feature is seen between these interpreted high resistivity features in the IP and AMT
data. The AMT data also show another high resistivity area directly below the IP resistivity high
below a depth of approximately 900 almost directly underneath the Kelsch and Double Diamond
showings and may be associated with the Kelsch lineament.
The AMT model appears to be consistent with an historical IP resistivity model in a broad sense
where areas of anomalously high and low data in each data set are compared. The interpretation is
made of a subvertical, low-resistivity feature trending in the north-northwest direction coincident
with the location of the Discovery lineament. Several previously identified showings appear to be
located above areas of interpreted low resistivity. The AMT model does not show anomalously high
resistivities near the surface as does the IP model, but could be explained by the limitation of the
AMT method where extremely high frequencies are required to image the near surface in highly
resistive areas; the inversion did not have enough information in this area. The AMT data also show
another high resistivity area directly below the IP resistivity high below a depth of approximately
900 m. A low resistivity feature is seen between these interpreted high resistivity features in the IP
and AMT data. It lies almost directly underneath the Kelsch and Double Diamond showings and may
be associated with the Kelsch lineament.
Qualified person
The scientific and technical information contained in this news release has been reviewed and
approved by Chris Dyakowski, PGeo, a consultant of the company, the optionor of the Fame property
and a qualified person as defined in National Instrument 43-101 -- Standards of Disclosure for
Mineral Projects. Mr. Dyakowski verified the data disclosed which includes a review of the
sampling, analytical and test data underlying the information and opinions contained therein.
SJ Geophysics Ltd. completed the Volterra-AMT. The Fame property grid consisted of nine survey
lines, spaced 200 metres apart and oriented with an azimuth of 53 degrees. The length of the lines are
600 m. Along each line, 100 by 100 m orthogonal crosses were planned at a spacing of 200 m. The
Volterra distributed acquisition system was employed for acquiring audio-magnetotelluric (AMT)
data. AMT data were collected overnight to gather high-quality data, resulting in approximately 10
hours of measurements at each station. The SJ Geophysics field crew consisted of one crew lead, one
field geophysicist and one technician to perform the day-to-day operations of the survey. A second
geophysicist joined the crew on July 15, 2024. This team oversaw all operational aspects including
field logistics, data acquisition and initial field data quality control.
About Longhorn Exploration Corp.
Longhorn Exploration has the exclusive right and option to acquire PureWave Hydrogen's
rights and obligations under four lease agreements, located in Kansas, United States, known as the Lily Rock
hydrogen project, which allow for the prospecting, exploration, drilling and production of any
substance including hydrogen gas. The company also has an option to acquire a 100-per-cent interest and
title to the Fame property located in the Clinton mining division, British Columbia.
We seek Safe Harbor.
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