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3 results for “shallow heating”
Onset of electron captures and shallow heating in magnetars
<p>The loss of magnetic pressure accompanying the decay of the magnetic field in a magnetar may trigger exothermic electron captures by nuclei in the shallow layers of the outer crust. The threshold density and pressure, as well as the maximum amount of heat that can be possibly released were calculated for different nuclei. The Landau-Rabi quantization of electron motion was taken into account using approximate analytical formulas. Results were obtained using experimental atomic masses and the <span class="math-tex">\(Q_\beta\)</span> values (included recommended ones) from the <a href="http://amdc.in2p3.fr/web/masseval.html">2016 Atomic Mass Evaluation</a> supplemented with the atomic mass model <a href="https://link.aps.org/doi/10.1103/PhysRevC.88.024308">HFB-24</a> available on the <a href="http://www.astro.ulb.ac.be/bruslib/">BRUSLIB</a> database.</p> <p>Each file contains data for electron captures by nuclei with the specified charge number Z and mass number A. The columns are as follows: </p> <ul> <li>magnetic field strengh in units of <span class="math-tex">\(B_{\rm rel}=\dfrac{m_e^2 c^3}{e \hbar}\approx 4.41\times 10^{13}\, \rm G\)</span></li> <li>the pressure in dyn cm<sup>-2</sup></li> <li>the mass density in g cm<sup>-3</sup></li> <li>the heat per nucleon in MeV.</li> </ul> <p>The files with (without) label 'ex' contain results for ground state to excited state (ground state) transitions.</p>
Differing temperature regimes have no impact on the heat stress response of shallow and upper mesophotic populations of a temperate calcareous sponge
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Supporting data for "Shallow convective heating in weak temperature gradient balance explains mesoscale vertical motions in the trades" (previously for ch. 5 of "Mesoscale Cloud Patterns in the Trade-Wind Boundary Layer")
<p>This contains both the data and scripts required to produce the figures in the preprint "Shallow convective heating in weak temperature gradient balance explains mesoscale vertical motions in the trades". The scripts labeled 1-5 produce the main figures; the other scripts produce supporting data or figures.</p> <p>Earlier versions of this dataset contained the scripts and data supporting Ch. 5 of the PhD thesis "Mesoscale Cloud Patterns in the Trade-Wind Boundary Layer". The scripts labeled 1-5 produce the main figures; the other scripts produce either the underlying data, or supporting figures (prefix S). </p>
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