1
... (Bath) at 30 and 37 °C, and determined the relative abundance of ¹²CH₄, ¹³CH₄, ¹²CH₃D, and ¹³CH₃D (a...
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2
...Very red featureless asteroids (spectroscopic D-types) are expected to have formed in the outer...
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3
...We present a solver for the 2D high-frequency Helmholtz equation in heterogeneous acoustic media...
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4
... enables us to access the flow via 3D particle tracking velocimetry and therefore to obtain truly three...
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6
...We have developed rapid 3-D dc resistivity forward modeling and inversion algorithms that use...
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10
...Determining the correct number of layers as input for 1D resistivity inversion is important...
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11
...Reliable 3D imaging is a required tool for developing models of complex geologic structures...
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12
... mitigate the impact of missing traces. We considered the prestack data as a 5D multidimensional array...
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13
by Seager, Sara, Deming, Drake
Published 2012
... or rule one out on the non-transiting short-period super Earth GJ 876d. The limiting factor in our...
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14
by Toksoz, M. Nafi, Zhang, Yang
Published 2012
... thoroughly. We applied the finite-element method to compute the static effective elastic properties from 3D...
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16
...We have developed crustal minimum 1-D P- and S-wave velocity models of the collision zone between...
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18
20
... R ⊕, and a mean density of 4.9 ± 2.4 g cm[superscript 3]. The two outer planets "c" and "d" are both...
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