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  • American Geophysical Union (AGU)  (2)
  • English  (2)
  • 1990-1994  (2)
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  • American Geophysical Union (AGU)  (2)
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Language
  • English  (2)
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  • 1990-1994  (2)
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  • 1
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1994
    In:  Journal of Geophysical Research: Planets Vol. 99, No. E1 ( 1994-01-25), p. 2063-2071
    In: Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 99, No. E1 ( 1994-01-25), p. 2063-2071
    Abstract: The physics of hypervelocity impacts into foams is of interest because of the possible application to interplanetary dust particle (IDP) capture by spacecraft. We present a model for the phenomena occurring in such impacts into low‐density organic polymer foams. Particles smaller than foam cells behave as if the foam is a series of solid slabs and are fragmented and, at higher velocities, thermally altered. Particles much larger than the foam cells behave as if the foam were a continuum, allowing the use of a continuum mechanics model to describe the effects of drag and ablation. Fragmentation is expected to be a major process, especially for aggregates of small grains. Calculations based on these arguments accurately predict experimental data and, for hypothetical IDPs, indicate that recovery of organic materials will be low for encounter velocities greater than 5 km s −1 . For an organic particle 100 μm in diameter, ∼35% of the original mass would be collected in an impact at 5 km s −1 , dropping to ∼10% at 10 km s −1 and ∼0% at 15 km s −l . For the same velocities the recovery ratios for troilite (FeS) are ∼95%, 65%, and 50%, and for olivine (Mg 2 SiO 4 ) they are ∼98%, 80%, and 65%, demonstrating that inorganic materials are much more easily collected. The density of the collector material has only a second‐order effect, changing the recovered mass by 〈 10% of the original mass.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1994
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  • 2
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1994
    In:  Journal of Geophysical Research: Solid Earth Vol. 99, No. B3 ( 1994-03-10), p. 4273-4284
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 99, No. B3 ( 1994-03-10), p. 4273-4284
    Abstract: An equation of state is presented for liquid iron based on published ultrasonic, thermal expansion, and enthalpy data at 1 bar and on pulse‐heating and shock wave compression and sound speed data up to 10 Mbar. The equation of state parameters, centered at 1 bar and 1811 K (the normal melting point of iron), are density, ρ 0 = 7019 kg/m 3 , isentropic bulk modulus, K S 0 = 109.7 GPa, and the first‐and second‐pressure derivatives of K S , K ′ S 0 = 4.66 and K ″ S 0 = −0.043 GPa −1 . A parameterization of the Grüneisen parameter γ as a function of density ρ and specific internal energy E is γ = γ 0 + γ′(ρ/ρ 0 ) n ( E ‐ E 0 ) where γ 0 = 1.735, γ′ = −0.130 kg/MJ, n = −1.87, and E 0 is the internal energy of the liquid at 1 bar and 1811 K. The model gives the temperature dependence of γ at constant volume as (∂γ/∂ T ) v |1bar,1811K = −8.4 × 10 −5 K −1 . The constant volume specific heat of liquid Fe at core conditions is 4.0–4.5 R. The model gives excellent agreement with measured temperatures of Fe under shock compression. Comparison with a preliminary reference Earth model indicates that the light component of the core does not significantly affect the magnitude of the isentropic bulk modulus of liquid Fe but does decrease its pressure derivative by ∼10%. Pure liquid Fe is 3–6% more dense than the inner core, supporting the presence of several percent of light elements in the inner core.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1994
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    detail.hit.zdb_id: 3094104-0
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    detail.hit.zdb_id: 161666-3
    detail.hit.zdb_id: 161667-5
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    detail.hit.zdb_id: 161665-1
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    SSG: 16,13
    Location Call Number Limitation Availability
    BibTip Others were also interested in ...
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