نتایج جستجو برای: mass budget

تعداد نتایج: 509221  

2013
Stephen E. Schauer Teresa A. Golden Delwin S. Merchant Biranchi N. Patra Jean D. Lang Sumita Ray Bulbul Chakravarti Deb Chakravarti Animesh Ray

Stephen E. Schauer, Teresa A. Golden, Delwin S. Merchant, Biranchi N. Patra, Jean D. Lang, Sumita Ray, Bulbul Chakravarti, Deb Chakravarti, and Animesh Ray Department of Biology, University of Rochester, Rochester, NY 14627, USA and Keck Graduate Institute, 535 Watson Drive, Claremont, CA 91711, USA Address communication to: Animesh Ray, Keck Graduate Institute, Claremont, CA 91711; Phone: (909...

Journal: :CoRR 2015
Daniel H. Biedermann Felix Dietrich Oliver Handel Peter M. Kielar Michael J. Seitz

The document serves as a reference for researchers trying to capture a large portion of a mass event on video for several hours, while using a very limited budget.

1998
B. Fuchs C. Flynn

Based on the recent discoveries of free floating brown dwarfs we derive estimates of the local mass density of this population of objects. Mass density estimates from various surveys span the range 0.03 to 0.005 M pc−3. These estimates are compared with the local mass densities of the other constituents of the galactic disk and, in particular, with the dynamically determined total local mass de...

Journal: :Journal of Japan Society of Civil Engineers, Ser. B2 (Coastal Engineering) 2016

2005
P. J. Clarke D. A. Lavallée G. Blewitt T. M. van Dam J. M. Wahr

[1] Increasingly, models of surface mass loads are used either to correct geodetic time coordinates by removing seasonal and other ‘‘noise’’, or for comparison with other geodetic parameters. However, models of surface loading obtained by simply combining the mass redistribution due to individual phenomena will not in general be selfconsistent, in that (i) the implied global water budget will n...

2008
T. F. Laganá E. S. Cypriano

Context. The luminous material in clusters of galaxies exists in two forms: the visible galaxies and the X-ray emitting intra-cluster medium. The hot intra-cluster gas is the major observed baryonic component of clusters, about six times more massive than the stellar component. The mass contained within visible galaxies is approximately 3% of the dynamical mass. Aims. Our aim was to analyze bot...

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