Emplacement of the Rocche Rosse rhyolite lava flow (Lipari, Aeolian Islands)
نویسندگان
چکیده
منابع مشابه
Emplacing a Cooling-Limited Rhyolite Lava Flow: Similarities with Basaltic Lava Flows
Accurate forecasts of lava flow length rely on estimates of eruption andmagma properties and, potentially more challengingly, on an understanding of the relative influence of characteristics such as the apparent viscosity, the yield strength of the flow core, or the strength of the lava’s surface crust. For basaltic lavas, the relatively high frequency of eruptions has resulted in numerous oppo...
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[1] Channeled lava flows, hundreds of kilometers long, are common on the lower flanks of the Tharsis Montes on Mars. Our analysis of a 690-km-long lava flow along the southwest perimeter of Ascraeus Mons shows that it was emplaced on low local slopes (<0.3 ), with a deep channel ( 20 m), and at high effusion rates (19,000–29,000 m/s) calculated from the Graetz number. These parameters are simil...
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Three long lava flows on Mars, Venus, and the Moon were examined in order to evaluate their possible emplacement rate and condition. On the Moon, flows o f the lay1 (phase 111) effusion within the Imbrium impact basin were examined using Apollo photography. The longest phase 111 flow can be followed for 250 km, terminating -400 km from the probable source vent. This flow has a width of 10 t o 2...
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The size and shape of the chromosomes, as well as the chromosomal domains that compose them, are determinants in the distribution and interaction between the bivalents within the nucleus of spermatocytes in prophase I of meiosis. Thus the nuclear architecture characteristic of the karyotype of a species can be modified by chromosomal changes such as Rb chromosomes. In this study we analysed the...
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ژورنال
عنوان ژورنال: Bulletin of Volcanology
سال: 2018
ISSN: 0258-8900,1432-0819
DOI: 10.1007/s00445-018-1222-4