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Autor:
Whitehouse, S. G.
The aim of this thesis is to seek a low-dimensional description of baroclinic instability in general, and of the Martian atmosphere in particular, where both forcing and spatial resonance are relevant to the dynamics of the system being analysed. The
Externí odkaz:
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.301652
We present the gravitational wave (GW) analysis of an extensive series of 3D MHD core-collapse simulations. Our 25 models are launched from a 15 solar mass progenitor, a spherically symmetric effective general relativistic potential, the Lattimer-Swe
Externí odkaz:
http://arxiv.org/abs/1001.1570
Publikováno v:
Class.Quant.Grav.27:114101,2010
We have performed a set of 11 three-dimensional magnetohydrodynamical core collapse supernova simulations in order to investigate the dependencies of the gravitational wave signal on the progenitor's initial conditions. We study the effects of the in
Externí odkaz:
http://arxiv.org/abs/0912.1455
Publikováno v:
Astrophys.J.Suppl.195:20,2011
FISH is a fast and simple ideal magneto-hydrodynamics code that scales to ~10 000 processes for a Cartesian computational domain of ~1000^3 cells. The simplicity of FISH has been achieved by the rigorous application of the operator splitting techniqu
Externí odkaz:
http://arxiv.org/abs/0910.2854
Publikováno v:
Astronomy and Astrophysics, 2010, 517A, 80F
Massive stars end their life in an explosion event with kinetic energies of the order 1 Bethe. Immediately after the explosion has been launched, a region of low density and high entropy forms behind the ejecta which is continuously subject to neutri
Externí odkaz:
http://arxiv.org/abs/0908.1871
Autor:
Fishley, W., Nandra, R., Carluke, I., Partington, P. F., Reed, M. R., Kramer, D. J., Wilson, M. J., Hubble, M. J. W., Howell, J. R., Whitehouse, S. L., Petheram, T. G., Kassam, A-A. M.
Publikováno v:
Bone & Joint Open; Jun2024, Vol. 5 Issue 6, p514-523, 10p
Akademický článek
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We discuss the formation of stellar mass black holes via protoneutron star (PNS) collapse. In the absence of an earlier explosion, the PNS collapses to a black hole due to the continued mass accretion onto the PNS. We present an analysis of the emitt
Externí odkaz:
http://arxiv.org/abs/0809.5129
Publikováno v:
Journal of Healthcare Leadership, Vol Volume 11, Pp 75-80 (2019)
Eric Scher,1,2 Sarah Whitehouse,1 Meredith Van Harn,3 John Bollinger,4 Bret Stevens,1 Kathy Macki,5 Deborah Saoud,5 Kimberly Baker-Genaw1,21Department of Medical Education, Henry Ford Health System, Detroit, MI, USA; 2Department of Medicine, Henry Fo
Externí odkaz:
https://doaj.org/article/2ae7d20faeb4437299a03025ace888d3