Browsing Physics & Atmospheric Science by Title
Now showing items 513-532 of 532
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Unusually low ozone, HCl, and HNO3 column measurements at Eureka, Canada during winter/spring 2011
(2012)No abstract available. -
Unusually low ozone, HCl, and HNO3 column measurements at Eureka, Canada during winter/spring 2011
(2012)No abstract available. -
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An upper limit to [C II] emission in a z ~= 5 galaxy
(2005-05-01)Low-ionization-state far-infrared (FIR) emission lines may be useful diagnostics of star-formation activity in young galaxies, and at high redshift may be detectable from the ground. In practice, however, very little is ... -
Use of carbon black to eliminate surface charging effects in photoelectron spectroscopy measurements of powders
(1997-10)No abstract available. -
Using [CI] to probe the Interstellar Medium in z~2.5 Sub-Millimeter Galaxies
(2013-07-24)We present new [CI](1-0) and 12CO(4-3) Plateau de Bure Interferometer observations of five Sub-Millimeter Galaxies (SMGs) and combine these with all available [CI](1-0) literature detections in SMGs to probe the gas ... -
Using SCUBA to place upper limits on arcsecond scale CMB anisotropies at 850 microns
(1999-09-19)The SCUBA instrument on the James Clerk Maxwell Telescope has already had an impact on cosmology by detecting relatively large numbers of dusty galaxies at high redshift. Apart from identifying well-detected sources, such ... -
Valence band of LiNixMn2-xO4 and its effects an the voltage profiles of LiNixMn2-xO4/Li electrochemical cells
(1996-12)No abstract available. -
Validation of ACE and OSIRIS ozone and NO2 measurements using ground-based instruments at 80 degrees N
(2012)No abstract available. -
Validation of NO2 and NO from the Atmospheric Chemistry Experiment (ACE)
(2008)No abstract available. -
The vertical structure of tropical convection and its impact on the budgets of water vapor and ozone
(2005-05)No abstract available. -
The vertical structure of tropical convection and its impact on the budgets of water vapor and ozone
(American Meteorological Society, 2005)Convective clouds in the Tropics that penetrate the boundary layer inversion preferentially detrain into a shallow outflow layer (2-5 km) or a deep outflow layer (10-17 km). The properties of these layers are diagnosed ... -
A Vigorous Starburst in the SCUBA Galaxy N2 850.4
(2003-07-11)We present optical and near-IR spectroscopy of a z=2.38 hyperluminous IR galaxy, covering the restframe wavelength range from 1000-5000A. It appears to comprise two components separated by less than 1" on the sky (<8kpc); ... -
Voltage-tunable singlet-triplet transition in lateral quantum dots
(2002-07)No abstract available. -
Wave-vector analysis of metallic surface energy
(1979-10/15)The exchange and correlation energy of a nonuniform electronic system can be decomposed into contributions of different wave-vector fluctuations. Both the long- and short-wavelength contributions to this energy can be ... -
Wave-vector decomposition of the exchange and correlation contributions to a metallic surface energy
(1980-04/15)The authors decompose the lowest-order nonlocal corrections to the local-density approximation to the exchange and correlation component of the metallic surface energy in terms its wave-vector components. Comparison with ... -
Weighing the Black Holes in z~2 Submillimeter-Emitting Galaxies Hosting Active Galactic Nuclei
(2008-05-01)We place direct observational constraints on the black-hole masses of the cosmologically important z~2 submillimeter-emitting galaxy (SMG; f850>4mJy) population, and use measured host-galaxy masses to explore their ... -
Westphal-MMD11: An interacting, submillimeter luminous Lyman break galaxy
(2002-6-10)We present new Hubble Space Telescope, high-resolution optical imaging of the submm luminous Lyman-break galaxy, Westphal-MMD11, an interacting starburst at z=2.979. The new imaging data, in conjunction with re-analysis ... -
The X-ray Spectral Properties of SCUBA Galaxies
(2005-10-20)Deep SCUBA surveys have uncovered a large population of massive submm galaxies (SMGs) at z>~1. Although it is generally believed that these galaxies host intense star-formation activity, there is growing evidence that a ...