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- W1660776007 abstract "Volcanism is widely distributed over the surfaces of the major terrestrial planets: Venus, Earth, and Mars. Anomalous centers of magmatic activity occur on each planet and are characterized by evidence for unusual concentrations of volcanic centers, long-lived activity, unusual rates of effusion, extreme size of volcanic complexes, compositionally unusual magmatism, and evidence for complex geological development. The purpose of this study is to compare the characteristics and distribution of these magmatic anomalies on Earth, Venus, and Mars in order to assess these characteristics as they may relate to global characteristics and evolution of the terrestrial planets." @default.
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- W1660776007 date "1993-01-01" @default.
- W1660776007 modified "2023-09-26" @default.
- W1660776007 title "Comparison of the distribution of large magmatic centers on Earth, Venus, and Mars" @default.
- W1660776007 hasPublicationYear "1993" @default.
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