Correlations between topography and intraflow width behavior in Martian and terrestrial lava flows

Citation
Mn. Peitersen et Da. Crown, Correlations between topography and intraflow width behavior in Martian and terrestrial lava flows, J GEO R-PLA, 105(E2), 2000, pp. 4123-4134
Citations number
39
Categorie Soggetti
Space Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
ISSN journal
21699097 → ACNP
Volume
105
Issue
E2
Year of publication
2000
Pages
4123 - 4134
Database
ISI
SICI code
0148-0227(20000225)105:E2<4123:CBTAIW>2.0.ZU;2-Q
Abstract
Local correlations between topography and width behavior within lava flows at Puu Oo, Mount Etna, Glass Mountain, Cerro Bayo, Alba Patera, Tyrrhena Pa tera, Elysium Mons, and Olympus Mons were investigated. For each flow, widt h and slope data were both referenced via downflow distance as a sequence o f points; the data were then divided into collections of adjacent three-poi nt features and two-point segments. Four discrete types of analyses were co nducted: (1)Three-point analysis examined positional correlations between w idth and slope features, (2) two-point analysis did the same for flow segme nts, (3) mean slope analysis included segment slope comparisons, and (4) su dden width behavior analysis measured abruptness of width changes. The dist ribution of types of correlations compared to random combinations of featur es and segments does not suggest a significant correlation between flow wid ths and local underlying slopes and indicates that for these flows at least , other factors have more influence on changes in width than changes in und erlying topography. Mean slopes underlying narrowing, widening, and constan t flow width segments were calculated. An inverse correlation between slope and width was found only at Mount Etna, where slopes underlying narrowing segments were greater than those underlying widening in 62% of the examined flows. For the majority of flows at Mount Etna, Puu Oo, and Olympus Mons. slopes were actually greatest under constant width segments; this may imply a topographically dependent resistance to width changes. The rate of chang e of width was also examined. Sudden width changes are relatively common at Puu Oo, Mount Etna, Elysium Mons, and Tyrrhena Patera and relatively rare at Glass Mountain, Cerro Bayo Olympus Mons, and Alba Patera. After correcti on for mapping scale, Puu Oo, Mount Etna, Olympus Mons, and Alba Patera app ear to fall on the same trend; Glass Mount exhibits unusually small amounts of sudden width behavior, and Tyrrhena Patera exhibits a relatively large number of sudden width behavior occurrences.