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Letteratura scientifica selezionata sul tema "Meteorites Mathematical models"

Autore: Grafiati

Pubblicato: 4 giugno 2021

Ultima modifica: 31 gennaio 2023

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Articoli di riviste sul tema "Meteorites Mathematical models"

1

Ballentine, Chris J., and Greg Holland. "What CO 2 well gases tell us about the origin of noble gases in the mantle and their relationship to the atmosphere." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 366, no. 1883 (September 30, 2008): 4183–203. http://dx.doi.org/10.1098/rsta.2008.0150.

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Study of commercially produced volcanic CO 2 gas associated with the Colorado Plateau, USA, has revealed substantial new information about the noble gas isotopic composition and elemental abundance pattern of the mantle. Combined with published data from mid-ocean ridge basalts, it is now clear that the convecting mantle has a maximum 20 Ne/ 22 Ne isotopic composition, indistinguishable from that attributed to solar wind-implanted (SWI) neon in meteorites. This is distinct from the higher 20 Ne/ 22 Ne isotopic value expected for solar nebula gases. The non-radiogenic xenon isotopic composition

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2

Grigorian, Samvel S. "The cometary nature of the Tunguska meteorite: on the predictive possibilities of mathematical models." Planetary and Space Science 46, no. 2-3 (February 1998): 213–17. http://dx.doi.org/10.1016/s0032-0633(97)00110-4.

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3

Russell, Sara S., Katherine H. Joy, Teresa E. Jeffries, Guy J. Consolmagno, and Anton Kearsley. "Heterogeneity in lunar anorthosite meteorites: implications for the lunar magma ocean model." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 372, no. 2024 (September 13, 2014): 20130241. http://dx.doi.org/10.1098/rsta.2013.0241.

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The lunar magma ocean model is a well-established theory of the early evolution of the Moon. By this model, the Moon was initially largely molten and the anorthositic crust that now covers much of the lunar surface directly crystallized from this enormous magma source. We are undertaking a study of the geochemical characteristics of anorthosites from lunar meteorites to test this model. Rare earth and other element abundances have been measured in situ in relict anorthosite clasts from two feldspathic lunar meteorites: Dhofar 908 and Dhofar 081. The rare earth elements were present in abundanc

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4

Smolka, Anselm. "Natural disasters and the challenge of extreme events: risk management from an insurance perspective." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 364, no. 1845 (June 28, 2006): 2147–65. http://dx.doi.org/10.1098/rsta.2006.1818.

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Loss statistics for natural disasters demonstrate, also after correction for inflation, a dramatic increase of the loss burden since 1950. This increase is driven by a concentration of population and values in urban areas, the development of highly exposed coastal and valley regions, the complexity of modern societies and technologies and probably, also by the beginning consequences of global warming. This process will continue unless remedial action will be taken. Managing the risk from natural disasters starts with identification of the hazards. The next step is the evaluation of the risk, w

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Sarafian, Adam R., Erik H. Hauri, Francis M. McCubbin, Thomas J. Lapen, Eve L. Berger, Sune G. Nielsen, Horst R. Marschall, Glenn A. Gaetani, Kevin Righter, and Emily Sarafian. "Early accretion of water and volatile elements to the inner Solar System: evidence from angrites." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 375, no. 2094 (April 17, 2017): 20160209. http://dx.doi.org/10.1098/rsta.2016.0209.

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Inner Solar System bodies are depleted in volatile elements relative to chondrite meteorites, yet the source(s) and mechanism(s) of volatile-element depletion and/or enrichment are poorly constrained. The timing, mechanisms and quantities of volatile elements present in the early inner Solar System have vast implications for diverse processes, from planetary differentiation to the emergence of life. We report major, trace and volatile-element contents of a glass bead derived from the D'Orbigny angrite, the hydrogen isotopic composition of this glass bead and that of coexisting olivine and sili

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Tesi sul tema "Meteorites Mathematical models"

1

Grant, Stephen Ian. "Medium frequency radar studies of meteors." 2003. http://thesis.library.adelaide.edu.au/public/adt-SUA20040224.152811.

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"July 2003." Includes bibliographical references (leaves 459-484) Electronic publication; full text available in PDF format; abstract in HTML format. Details the application of a medium frequency Doppler radar to observations of meteorites entering the Earth's atmosphere. Techniques were developed that verified system performance was to specification Electronic reproduction.[Australia] :Australian Digital Theses Program,2001. xx, 485 leaves : ill. ; 30 cm.

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Libri sul tema "Meteorites Mathematical models"

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Observatory, Smithsonian Astrophysical, ed. Mineralogic and petrologic studies of meteorites and lunar samples: Grant NAGW 3451, final progress report, for the period 01 February 1993 through 30 September 1997. Cambridge, Mass: Smithsonian Institution, Astrophysical Observatory, 1998.

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Capitoli di libri sul tema "Meteorites Mathematical models"

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Adam, John A. "Tsunamis." In Rays, Waves, and Scattering. Princeton University Press, 2017. http://dx.doi.org/10.23943/princeton/9780691148373.003.0013.

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Abstract (sommario):

This chapter describes a mathematical model of tsunami propagation (transient waves). A tsunami is a series of ocean waves triggered by large-scale disturbances of the ocean, including earthquakes, as well as landslides, volcanic eruptions, and meteorites. Tsunamis have very long wavelengths (typically hundreds of kilometers). They have also been called “tidal waves” or “seismic sea waves,” but both terms are misleading. The chapter first considers the boundary-value problem before modeling two special cases of tsunami generation, one due to an initial displacement on the free surface and the other due to tilting of the seafloor. It also discusses surface waves on deep water and how fast the wave energy propagates and concludes with an analysis of leading waves due to a transient disturbance.

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