Abstract
The results of statistical analyses performed on three published hotspot distributions suggest that significantly more hotspots occur as nearly antipodal pairs than is anticipated from a random distribution, or from their association with geoid highs and divergent plate margins. The observed number of antipodal hotspot pairs depends on the maximum allowable deviation from exact antipodality. At a maximum deviation of ≤700 km, 26% to 37% of hotspots form antipodal pairs in the published lists examined here, significantly more than would be expected from the general hotspot distribution. Two possible mechanisms that might create such a distribution include: (1) symmetry in the generation of mantle plumes, and (2) melting related to antipodal focusing of seismic energy from large‐body impacts.
Original language | English (US) |
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Pages (from-to) | 2011-2014 |
Number of pages | 4 |
Journal | Geophysical Research Letters |
Volume | 19 |
Issue number | 20 |
DOIs | |
State | Published - Oct 23 1992 |
ASJC Scopus subject areas
- Geophysics
- General Earth and Planetary Sciences