Table 2.

Summary of the four coupling scenarios in a two-layer elastic medium (Table 1). α2 and β2 are the P- and S-wave velocities of the half-space, respectively. β1 is the first-layer S-wave velocity. Further details and corresponding references can be found in Section 3.

Velocity relationshipSeismic-wave types in the half-spacePressure field examplesObservation sites or environments
c > α2Homogeneous P and Sv wavesOblique (nearly vertical) acoustic wave incidence generated by meteors or airgunsOnshore seismic stations, marine seismic surveys
β2 < c < α2Inhomogeneous P wavesAcoustic waves generated by airgunsShallow water seismic surveys
Homogeneous Sv waves
(c = VL)(leaky-mode surface waves)
c < β2Inhomogeneous P and Sv wavesInfrasound generated by meteors, lighting,Sedimentary structures
(c = VR)(air-coupled Rayleigh waves)airborne human activities
cβ1Inhomogeneous P and Sv waves in the both layershorizontal-propagating infrasound and winds, dust devils, ocean wavesEarth’s seafloor, Martian and Earth’s surfaces
Velocity relationshipSeismic-wave types in the half-spacePressure field examplesObservation sites or environments
c > α2Homogeneous P and Sv wavesOblique (nearly vertical) acoustic wave incidence generated by meteors or airgunsOnshore seismic stations, marine seismic surveys
β2 < c < α2Inhomogeneous P wavesAcoustic waves generated by airgunsShallow water seismic surveys
Homogeneous Sv waves
(c = VL)(leaky-mode surface waves)
c < β2Inhomogeneous P and Sv wavesInfrasound generated by meteors, lighting,Sedimentary structures
(c = VR)(air-coupled Rayleigh waves)airborne human activities
cβ1Inhomogeneous P and Sv waves in the both layershorizontal-propagating infrasound and winds, dust devils, ocean wavesEarth’s seafloor, Martian and Earth’s surfaces
Table 2.

Summary of the four coupling scenarios in a two-layer elastic medium (Table 1). α2 and β2 are the P- and S-wave velocities of the half-space, respectively. β1 is the first-layer S-wave velocity. Further details and corresponding references can be found in Section 3.

Velocity relationshipSeismic-wave types in the half-spacePressure field examplesObservation sites or environments
c > α2Homogeneous P and Sv wavesOblique (nearly vertical) acoustic wave incidence generated by meteors or airgunsOnshore seismic stations, marine seismic surveys
β2 < c < α2Inhomogeneous P wavesAcoustic waves generated by airgunsShallow water seismic surveys
Homogeneous Sv waves
(c = VL)(leaky-mode surface waves)
c < β2Inhomogeneous P and Sv wavesInfrasound generated by meteors, lighting,Sedimentary structures
(c = VR)(air-coupled Rayleigh waves)airborne human activities
cβ1Inhomogeneous P and Sv waves in the both layershorizontal-propagating infrasound and winds, dust devils, ocean wavesEarth’s seafloor, Martian and Earth’s surfaces
Velocity relationshipSeismic-wave types in the half-spacePressure field examplesObservation sites or environments
c > α2Homogeneous P and Sv wavesOblique (nearly vertical) acoustic wave incidence generated by meteors or airgunsOnshore seismic stations, marine seismic surveys
β2 < c < α2Inhomogeneous P wavesAcoustic waves generated by airgunsShallow water seismic surveys
Homogeneous Sv waves
(c = VL)(leaky-mode surface waves)
c < β2Inhomogeneous P and Sv wavesInfrasound generated by meteors, lighting,Sedimentary structures
(c = VR)(air-coupled Rayleigh waves)airborne human activities
cβ1Inhomogeneous P and Sv waves in the both layershorizontal-propagating infrasound and winds, dust devils, ocean wavesEarth’s seafloor, Martian and Earth’s surfaces
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close