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Now showing items 11-20 of 63
Generalizations of pp-wave spacetimes in higher dimensions
(2003-05)
No abstract available.
Sources of carbonaceous aerosols over the United States and implications for natural visibility
(2003-06)
No abstract available.
Tropical rainfall and boundary layer moist entropy
(2003-06)
No abstract available.
Crustal structure of the ocean-continent transition at Flemish Cap: Seismic refraction results
(2003-11)
[1] We conducted a seismic refraction experiment across Flemish Cap and into the deep basin east of Newfoundland, Canada, and developed a velocity model for the crust and mantle from forward and inverse modeling of data ...
Pattern formation inside bacteria: Fluctuations due to the low copy number of proteins
(2003-03)
No abstract available.
Direct observation of remanent magnetic states in epitaxial fcc Co small disks
(2003-04)
No abstract available.
Measurement of the Sunyaev-Zel'dovich Increment in Massive Galaxy Clusters
(2003-12)
We have detected the Sunyaev-Zel'dovich (SZ) increment at 850 microns in two galaxy clusters (Cl 0016+16 and MS 1054.4-0321) using SCUBA (Sub-millimetre Common User Bolometer Array) on the James Clerk Maxwell Telescope. ...
Diffusion of Asymmetric Swimmers
(American Physical Society, 2003)
Asymmetric swimmers that would move at a constant speed in perfect circles in the absence of fluctuations were studied. Particles moving at a constant speed with either a fixed or a Gaussian distributed magnitude of curvature ...
Crooked-line 2D seismic reflection imaging in crystalline terrains: Part 2, migration
(2003-01)
Seismic reflection surveys are frequently conducted over very complicated geological structure, but surveying often must be confined to existing crooked roads or tracks. Typically, data from such 2D crooked-line surveys ...
Submillimetre and far-infrared spectral energy distributions of galaxies: the luminosity-temperature relation and consequences for photometric redshifts
(2003-01)
The spectral energy distributions (SEDs) of dusty high-redshift galaxies are poorly sampled in frequency and spatially unresolved. Their form is crucially important for estimating the large luminosities of these galaxies ...