%
% CAUTION!!!
% Entries will appear in the order the are entered in this file.
%
% Add Publications for 2016 ONLY
%
@Article{Featherstone+Hindman2016,
  author="Featherstone, N. A.
  and Hindman, B. W.",
  title="The Emergence Of Solar Supergranulation As A Natural Consequence Of Rotationally Constrained Interior Convection",
  journal="The Astrophysical Journal",
  year="2016",
  volume="830",
  number="1",
  pages="L15",
  optkeywords="Rayleigh",
  optnote="exported from refbase (https://geodynamics.org/cig/refbase/show.php?record=1442), last updated on Mon, 10 Apr 2017 11:05:43 -0700",
  issn="2041-8213",
  doi="10.3847/2041-8205/830/1/L15",
  opturl="http://stacks.iop.org/2041-8205/830/i=1/a=L15?key=crossref.b9fcd6b0ca6169fe7d0be8513d56f369"
}

@Article{Featherstone_Hindmam_2016,
    author = "Featherstone, N.A. and Hindman, B.W.",
    title="The Spectral Amplitude Of Stellar Convection And Its Scaling In The High-Rayleigh-Number Regime",
    year="2016",
    journal="The Astrophysical Journal",
    volume="818",
    number="1",
    pages="32",
    optkeywords="Rayleigh",
    issn="1538-4357",
    doi="http://doi.org/10.3847/0004-637X/818/1/32",
    opturl="http://stacks.iop.org/0004-637X/818/i=1/a=32?key=crossref.a90f82507dd0eeb7a6e7562d1e4b0210"
}

@Article{Matsui_etal_2016,
	 author = "Matsui, H. and Heien, E. and Aubert, J. and Aurnou, J.M. and Avery, M. and Brown, B. and Buffett, B.A. and Busse, F. and Christensen, U.R. and Davies, C.J. and Featherstone, N. and Gastine, T. and Glatzmaier, G.A. and Gubbins, D. and Guermond, J.-L. and Hayashi, Y.-Y. and Hollerbach, R. and Hwang, L.J. and Jackson, A. and Jones, C.A. and Jiang, W. and Kellogg, L.H. and Kuang, W. and Landeau, M. and Marti, P.H. and Olson, P. and Ribeiro, A. and Sasaki, Y. and Schaeffer, N. and Simitev, R.D. and Sheyko, A. and Silva, L. and Stanley, S. and Takahashi, F. and Takehiro, S.-ichi and Wicht, J. and Willis, A.P.",
	  title="Performance benchmarks for a next generation numerical dynamo model",
	 year="2016",
	 journal="Geochemistry, Geophysics, Geosystems",
	 volume="17",
	 number="5",
	 pages="1586-1607",
	 optkeywords="Calypso",
	 issn="1525-2027",
	 doi="http://doi.org/10.1002/2015GC006159",
	 opturl="http://doi.wiley.com/10.1002/2015GC006159"
}

@Article{OMara_etal2016,
  author="O'Mara, B.
  and Miesch, M. S.
  and Featherstone, N. A.
  and Augustson, K. C.",
  title="Velocity amplitudes in global convection simulations: The role of the Prandtl number and near-surface driving",
  journal="Advances in Space Research",
  year="2016",
  optkeywords="Rayleigh",
  optnote="exported from refbase (https://geodynamics.org/cig/refbase/show.php?record=1121), last updated on Thu, 21 Apr 2016 10:52:02 -0700",
  issn="0273-1177",
  doi="10.1016/j.asr.2016.03.038",
opturl="http://linkinghub.elsevier.com/retrieve/pii/S0273117716300953"
}
%
% CAUTION!!!
% Entries will appear in the order the are entered in this file.
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% Add Publications for 2018 ONLY
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@Article{Karak_etal2018,
author="Karak, B. B.
and Miesch, M.
and Bekki, Y.",
title="Consequences of high effective Prandtl number on solar differential rotation and convective velocity",
journal="Physics of Fluids",
year="2018",
volume="30",
number="4",
pages="046602",
optkeywords="Rayleigh",
optnote="exported from refbase (https://geodynamics.org/cig/refbase/show.php?record=1614), last updated on Tue, 19 Jun 2018 19:49:37 -0700",
issn="1070-6631",
doi="10.1063/1.5022034",
opturl="http://aip.scitation.org/doi/10.1063/1.5022034"
}

@Article{Miquel_etal2018,
author="Miquel, B.
and Xie, J-H
and Featherstone, N.
and Julien, K.
and Knobloch, E.",
title="Equatorially trapped convection in a rapidly rotating shallow shell",
journal="Physical Review Fluids",
year="2018",
volume="3",
number="5",
optkeywords="Rayleigh",
optnote="exported from refbase (https://geodynamics.org/cig/refbase/show.php?record=1616), last updated on Tue, 19 Jun 2018 19:51:40 -0700",
issn="2469-990X",
doi="10.1103/PhysRevFluids.3.053801",
opturl="https://link.aps.org/doi/10.1103/PhysRevFluids.3.053801"
}

@Article{Orvedahl_etal2018,
author="Orvedahl, R. J.
and Calkins, M. A.
and Featherstone, N. A.
and Hindman, B. W.",
title="Prandtl-number Effects in High-Rayleigh-number Spherical Convection",
journal="The Astrophysical Journal",
year="2018",
volume="856",
number="1",
pages="13",
optkeywords="Rayleigh",
abstract="Convection is the predominant mechanism by which energy and angular momentum are transported in the outer portion of the Sun. The resulting overturning motions are also the primary energy source for the solar magnetic field. An accurate solar dynamo model therefore requires a complete description of the convective motions, but these motions remain poorly understood. Studying stellar convection numerically remains challenging; it occurs within a parameter regime that is extreme by computational standards. The fluid properties of the convection zone are characterized in part by the Prandtl number \#\#IMG\#\# [http://ej.iop.org/images/0004-637X/856/1/13/apjaaaeb5ieqn1.gif] \${\backslash}Pr \$ {\^A}~={\^A}~$\nu$ / $\kappa$ , where $\nu$ is the kinematic viscosity and $\kappa$ is the thermal diffusion; in stars, \#\#IMG\#\# [http://ej.iop.org/images/0004-637X/856/1/13/apjaaaeb5ieqn2.gif] \${\backslash}Pr \$ is extremely low, \#\#IMG\#\# [http://ej.iop.org/images/0004-637X/856/1/13/apjaaaeb5ieqn3.gif] \${\backslash}Pr \${\^A}~??{\^A}{\^A}{\^A}~10 -7 . The influence of \#\#IMG\#\# [http://ej.iop.org/images/0004-637X/856/1/13/apjaaaeb5ieqn4.gif] \${\backslash}Pr \$ on the convective motions at the heart of the dynamo is not well understood since most numerical studies are limited to using \#\#IMG\#\# [http://ej.iop.org/images/0004-637X/856/1/13/apjaaaeb5ieqn5.gif] \${\backslash}Pr \${\^A}~??{\^A}{\^A}{\^A}~1. We systematically vary \#\#IMG\#\# [http://ej.iop.org/images/0004-637X/856/1/13/apjaaaeb5ieqn6.gif] \${\backslash}Pr \$ and the degree of thermal forcing, characterized through a Rayleigh number, to explore its influence on the convective dynamics. For sufficiently large thermal driving, the simulations reach a so-called convective free-fall state where diffusion no longer plays an important role in the interior dynamics. Simulations with a lower \#\#IMG\#\# [http://ej.iop.org/images/0004-637X/856/1/13/apjaaaeb5ieqn7.gif] \${\backslash}Pr \$ generate faster convective flows and broader ranges of scales for equivalent levels of thermal forcing. Characteristics of the spectral distribution of the velocity remain largely insensitive to changes in \#\#IMG\#\# [http://ej.iop.org/images/0004-637X/856/1/13/apjaaaeb5ieqn8.gif] \${\backslash}Pr \$ . Importantly, we find that \#\#IMG\#\# [http://ej.iop.org/images/0004-637X/856/1/13/apjaaaeb5ieqn9.gif] \${\backslash}Pr \$ plays a key role in determining when the free-fall regime is reached by controlling the thickness of the thermal boundary layer.",
optnote="exported from refbase (https://geodynamics.org/cig/refbase/show.php?record=1615), last updated on Wed, 27 Mar 2019 13:53:43 -0700",
doi="10.3847/1538-4357/aaaeb5",
opturl="http://stacks.iop.org/0004-637X/856/i=1/a=13"
}
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% CAUTION!!!
% Entries will appear in the order the are entered in this file.
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% Add Publications for 2019 ONLY
%
@Article{Buffett+Matsui2019,
author="Buffett, B.
and Matsui, H.",
title="Equatorially trapped waves in Earth{\textquoteright}s core",
journal="Geophysical Journal International",
year="2019",
volume="218",
number="2",
pages="1210--1225",
optkeywords="Rayleigh",
optnote="exported from refbase (https://geodynamics.org/cig/refbase/show.php?record=1739), last updated on Thu, 20 Jun 2019 08:58:07 -0700",
issn="0956-540X",
doi="10.1093/gji/ggz233",
opturl="https://academic.oup.com/gji/article/218/2/1210/5491334"
}
