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Extensions of the Galperin Transformation Matrices for Triaxial Seismometers
Talso C P Chui1, Andrew Erwin1, Inseob Hahn1
1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
This study details the physics of Galperin symmetric triaxial seismometers, extending original work to include practical, non-idealized conditions for improved seismic detection on Earth and Mars.
Area of Science:
- Seismology
- Geophysics
- Planetary Science
Background:
- The Galperin symmetric triaxial seismometer, invented in 1955, is a key instrument for seismic detection.
- Its application has expanded to include seismic exploration on Mars.
- Detailed physics of this seismometer are not widely available in open literature.
Purpose of the Study:
- To present detailed, unpublished physics of the Galperin symmetric triaxial seismometer.
- To extend the original theoretical work to encompass more practical operational scenarios.
- To enhance the understanding and application of this seismometer in diverse environments.
Main Methods:
- Theoretical extension of Galperin's original work.
- Inclusion of non-idealized geometric and operational parameters.
- Analysis of seismometer performance under varied conditions.
Main Results:
- Developed a more comprehensive physical model for the Galperin seismometer.
- Accounted for non-ideal tilt angles and component orientations (deviations from 120°).
- Incorporated the effects of distributed mass and low-frequency operations.
Conclusions:
- The extended model provides a more realistic representation of seismometer behavior.
- This work enhances the utility of Galperin seismometers for challenging seismic detection tasks.
- Improved understanding facilitates more accurate seismic data interpretation on Earth and other planets.
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