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Seismological Perspectives on Broadband Tilt, Strain, and Rotation Measurement

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Seismological Perspectives on Broadband Tilt, Strain, and Rotation Measurement

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    1. Seismological Perspectives on Broadband Tilt, Strain, and Rotation Measurement Charles Langston Center for Earthquake Research and Information University of Memphis

    2. Ground Motions have 6 Degrees of Freedom

    3. Rotation (tilt) as Noise Seismological practice using 3 component seismometers usually assumes that recorded ground motions represent ground displacement. It is very well known, however, that horizontal seismometers are particularly susceptible to tilt, which is a rotation about a horizontal axis. Tilt is a common noise signal for shallow-depth, temporary installations, as in many PASSCAL experiments, where diurnal thermal or water-saturated ground expansion and contraction produces high levels of noise on the horizontal channels.

    4. Typical horizontal/vertical noise levels CMG-40T Installation

    5. Rotation as "Pseudo" Signal Tilt may also be a direct signal of tectonic interest. Broadband installations on active volcanoes often record large "long-period" pulses that have been interpreted as long-period pressure waves but may also be simple tilts induced in the near-field of intrusive or extrusive loads within the volcano. Thus, a major improvement in broadband seismometry is needed to separate the effects of simple ground displacements from the effects of tilt.

    6. Hidayat, D., B. Voight, C. Langston, A. Ratdomopurbo, C. Ebeling, Broadband seismic experiment at Merapi volcano, Java, Indonesia: very-long-period pulses embedded in multiphase earthquakes, J. Volcan.Geotherm. Res., 100, 215-231 (2000).

    8. Geometry

    9. Hypothesis is that these long-period pulses are due to near-field tilts from the growing lava dome

    11. Rotation and Strain as Future Real Signal Tilt or rotation, in itself, is also a very interesting observable in wave propagation and should be part of seismic interpretation. Rotation is closely related to strain and both quantities can be used to gain a deeper understand seismic wave propagation. For example, combined use of displacement polarization, rotation, and/or strain at a single observation point yield estimates of wave horizontal phase velocities.

    12. Example: Strong Motion Array Recording During the October 28-29, 2002, Embayment Seismic Excitation Experiment (ESEE)

    13. Array Geometry

    15. Compute partial strain(or rotation)from array channels

    16. Plane Wave Model

    17. Velocity Estimate

    18. Rotation and Strain as Future Real Signal (2) Measurement of local strains and tilts could be made by differencing the signals of closely spaced seismometers. Ironically, closely matched instrument responses and tilt insensitivity of individual sensors would be a requirement for accurately estimating rotations and strains with such micro arrays.

    19. Broadband Micro-Array or Finite Difference Star

    20. To compute rotation (or strains):

    21. Thus, instrument responses must be known to better than 1 part in a million. It is probably better to design a broadband rotation meter.

    22. Conclusions Future broadband velocity sensors should be insensitive to rotation. Future broadband rotation sensors should be insensitive to linear motion. Combined Linear and Rotational measurements will yield interesting new information on seismic wave propagation.

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