1984
DOI: 10.1029/gl011i004p00287
|View full text |Cite
|
Sign up to set email alerts
|

Mapping convection in the mantle

Abstract: Abstract. Long-period (100-250 sec.) Love and Rayleigh waves are used to map heterogeneity and azimuthal anisotropy in the upper mantle. Spherical harmonic descriptions of anisotropy up to £ = m = 3 and 28 are derived. Azimuthal anisotropy obtains values as high as 1 Yz OJo. There is good correlation of fast Rayleigh wave directions with upper mantle return flow directions derived from kinematic considerations. This is consistent with the a-axis of olivine being aligned in the flow direction. The main differen… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
4
1

Citation Types

1
74
0

Year Published

1984
1984
2021
2021

Publication Types

Select...
8
2

Relationship

0
10

Authors

Journals

citations
Cited by 185 publications
(75 citation statements)
references
References 16 publications
(22 reference statements)
1
74
0
Order By: Relevance
“…It may be related to passive motion of the lithosphere over the stationary asthenosphere, in which case, the most likely location for anisotropy would be in the transition zone between the two shells and the fast direction of anisotropy would be close to that of plate motion (Leven et al, 1981). Alternatively, the preferred orientation could be induced by flow in the asthenosphere, so the fast direction of anisotropy would coincide with the direction of flow but might differ from the direction of plate motion (Tanimoto and Anderson, 1984). Azimuthal anisotropy in the uppermost mantle may also be related to past and present deformation of the lithosphere (Fuchs, 1983).…”
Section: Introductionmentioning
confidence: 99%
“…It may be related to passive motion of the lithosphere over the stationary asthenosphere, in which case, the most likely location for anisotropy would be in the transition zone between the two shells and the fast direction of anisotropy would be close to that of plate motion (Leven et al, 1981). Alternatively, the preferred orientation could be induced by flow in the asthenosphere, so the fast direction of anisotropy would coincide with the direction of flow but might differ from the direction of plate motion (Tanimoto and Anderson, 1984). Azimuthal anisotropy in the uppermost mantle may also be related to past and present deformation of the lithosphere (Fuchs, 1983).…”
Section: Introductionmentioning
confidence: 99%
“…is parallel to current plate motion (Tanimoto and Anderson 1984). For investigating the intermediate depth range, recent studies have analysed surface waves at shorter periods of ∼18-50 s either by measuring group velocities from onland records (Smith et al 2004) or by measuring phase velocities from records of ocean bottom seismometers (OBSs; Forsyth & Li 2005;Weeraratne et al 2007).…”
Section: Introductionmentioning
confidence: 99%
“…This deformation can result in textural changes (lattice preferred orientation, crystal preferred orientation, and shape preferred orientation) of rocks that may affect their physical properties, such as seismic velocity, electrical conductivity, and viscosity. It is well known that lattice preferred orientation of olivine can be imaged seismically (e.g., Tanimoto and Anderson 1984;Nicolas and Christensen 1987;Montagner and Guillot 2002). If well imaged, patterns and depth distribution of seismic anisotropy can be used to constrain patterns of flow either occurring at present in the asthenosphere or in the past, preserved as the fabric frozen into the lithosphere, and accordingly to provide insight into models of lithospheric formation and evolution (e.g., Blackman and Kendall 2002).…”
Section: Introductionmentioning
confidence: 99%