AGS SPIA
SPIA, a versatile processing and inversion software, is designed for ground-based Time-domain Electromagnetic (TEM) and Direct Current/Induced Polarisation (VES) data. Integrating the robust and fast AarhusInv inversion code, SPIA features a user-friendly graphical interface, facilitating the editing of data and models directly within the software. This innovative platform supports a range of inversion methods, including Resistivity, Cole-Cole, and Maximum Phase Angle (MPA), catering to TEM data affected by IP effects.
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AGS SPIA Introduction
What is AGS SPIA?
SPIA, a versatile processing and inversion software, is designed for ground-based Time-domain Electromagnetic (TEM) and Direct Current/Induced Polarisation (VES) data. Integrating the robust and fast AarhusInv inversion code, SPIA features a user-friendly graphical interface, facilitating the editing of data and models directly within the software. This innovative platform supports a range of inversion methods, including Resistivity, Cole-Cole, and Maximum Phase Angle (MPA), catering to TEM data affected by IP effects.
How to use AGS SPIA?
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Why Choose AGS SPIA?
You should choose this if you’re dealing with complex geophysical data and need a reliable, user-friendly software for processing and inversion of TEM and IP data. It’s tailored for professionals needing precise and fast analysis.
AGS SPIA Features
Features
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Pricing
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AGS SPIA Tags
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