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38 results for “dynamos”
Dataset for the Roles of Cloud Radiative Forcing in the Onset of MJO in DYNAMO
<p><strong>A journal paper "Roles of Cloud Radiative Forcing in the Onset of MJO in DYNAMO" details the method to create the data.</strong></p> <p>Readme</p> <p>The modeling and observed dataset for generating the figures in this paper is stored here. </p> <p>Contact</p> <p>For any questions related to the dataset, please contact the authors of the paper. </p>
Inlist Files for Effects of Full Sphere Convection On M-Dwarf Dynamo Action, Flux Emergence, and Spin-Down
<p>Inlist files for a model of a ZAMS 0.3 M_sun star used as background for global convection simulations in <em>Effects of Full Sphere Convection On M-Dwarf Dynamo Action, Flux Emergence, and Spin-Down</em>. Run using MESA version r12115.</p>
Dataset for the manuscript "Helical and nonhelical dynamos in thin accretion discs"
<p>Dataset and post-processing scripts for the manuscript "Helical and nonhelical dynamos in thin accretion discs".</p>
Datasets for ``The effect of a dynamo-generated field on the Parker wind''
<pre>This directory contains an index.html file with links to the run directories for Runs A-C and idl plotting routines with secondary data for the other figures for the paper "The effect of a dynamo-generated field on the Parker wind" by Jakab & Brandenburg.</pre>
Supplementary data for "History and future of the Martian dynamo and implications of a hypothetical solid inner core"
<p>This dataset contains the results of the calculations we carried out for the submitted manuscript titled "History and future of the Martian dynamo and implications of a hypothetical solid inner core". The data are organized into the following three groups: 1) radial_profiles; 2) histories; and 3) parameter_space_exploration. The first group, "radial_profiles", describes the radial density structure, and corresponding profiles of pressure, gravity, enclosed mass, and thermal expansivity for our simplified models of Earth and Mars. The second group, "histories", contains the results of our thermal evolution calculations for our reference Earth case and our five reference cases for Mars. For each case, there is a header file describing the input parameters, the derived parameters, and the contents of the accompanying tables of values. The third group, "parameter_space_exploration", contains the data that is partially illustrated in Figures 11-16, in which we show various outcomes across a wide range of multidimensional parameter space. All files are in ASCII format. Header files explain their contents in plain language and/or with reference to variables described in the paper. Data tables are tab-delimited.</p>
An example of ECMWF Deterministic Model analysis data for DYNAMO
<p>The full dataset is hosted by Earth Observing Laboratory at the National Center for Atmospheric Research. This is only one example used to compute momentum budget associated with the Madden-Julian Oscillation during DYNAMO. </p>
Simulation data-set for ApJ Article: "Confinement of the Solar Tachocline by a Non-Axisymmetric Dynamo"
<p>This dataset contains the input files (including a last Checkpoint snapshot, so the simulation can be restarted), and basic simulation information (Rayleigh data products, time-averaged data products, and basic plots) for each of the 12 simulations discussed in the ApJ journal article, "Confinement of the Solar Tachocline by a Non-Axisymmetric Dynamo". Each simulation has a separate .zip file that can be downloaded either on its own or together with the rest of the simulation suite. The structure and contents of the resulting directory (after unzipping) is described in detail in the "README" .pdf document. </p><p>Note that the magnetic cases have custom diagnostic outputs and the main_input file (as directly given here) must be run using Loren Matilsky's personal branch of the code:<a href=" https://github.com/illorenzo7/Rayleigh/tree/meprodsubcurvnobinrz"> https://github.com/illorenzo7/Rayleigh/tree/meprodsubcurvnobinrz</a>. Otherwise, the MHD cases can be run with the current main branch of the Rayleigh code (<a href="https://github.com/geodynamics/Rayleigh">https://github.com/geodynamics/Rayleigh</a>), as long as some small modifications to the main_input file (described in the "README" document) are made first. </p>
Supplementary materials for the manuscript "Run-away transition to turbulent strong-field dynamo"
<p>Supplementary materials for the manuscript "Run-away transition to turbulent strong-field dynamo" including simulation data and Jupyter notebooks to read them</p>
Nonkinematic solar dynamo models with double-cell meridional circulation
<p>MESA inlists for <a href="https://ui.adsabs.harvard.edu/#abs/2018JASTP.179..185P/abstract">Nonkinematic solar dynamo models with double-cell meridional circulation</a></p>
Dataset for "Mars' axial and reversing dynamo recorded in a magnetized impact crater 4.2 billion years ago"
<p>This dataset is for the research titled "<em><strong>Mars’ axial and reversing dynamo recorded in a magnetized impact crater 4.2 billion years ago</strong></em>".</p> <ul> <li>Please ensure that all files are placed in the same directory</li> <li><strong>ESD.m</strong> contains all the procedures needed to invert crustal magnetization from crustal magnetic field data. </li> <li>The remaining files are crustal magnetic field datasets generated by IDL, which are used as input for <strong>ESD.m</strong>.</li> <li>For MATLAB users, it is necessary to install the <strong><em>restore_idl</em></strong> package to read these IDL-generated files within MATLAB.</li> </ul> <p>Don't hesitate to email me (jfqin@berkeley.edu) if you have any trouble running this code.</p>
Supporting data for "Magnetic Archaeology of Early-Type Stellar Dynamos"
<p>Supporting data for "Magnetic Archaeology of Early-Type Stellar Dynamos". The `run_grid.sh` script runs a grid of models generated by copying and modifying entries in the `template` folder. The various python scripts provide a way of generating the figures in our manuscript.</p>
Supplmental Material to Nature of Intense Magnetism and Differential Rotation In Convective Dynamos of M-Dwarf Stars With Tachoclines
<p>Inlists and source files used for the MESA model in the paper "Nature of Intense Magnetism and Differential Rotation In Convective Dynamos of M-Dwarf Stars With Tachoclines"</p> <p>This work employed MESA version 10398.</p>
Rayleigh Inlists and Checkpoints for Effects of Full Sphere Convection On M-Dwarf Dynamo Action, Flux Emergence, and Spin-Down
<p>Input files, checkpoints, and summary data for the three primary Rayleigh global convection simulations highlighted in Bice & Toomre 2023b, <em>Effects of Full Sphere Convection On M-Dwarf Dynamo Action, Flux Emergence, and Spin-Down</em>. </p>
Dataset of "Parameter regimes of hemispherical dynamo waves in a spherical shell from 3D MHD simulations" submitting to JGR: Planets
<p>Simulation data using Magic code. In the "general properties" part, basic properties (e.g., Pm, Rm, Rol, wave frequency, regime types....) are compressed into 3 python numpy .npz files, according to different Ekman number. For the regime types, we use 0 for failed dynamos, 1 for dipoles, 2 for global waves, 3 for hemispherical waves and 4 for multipolar solutions. In the "cases" part, we include raw output from Magic code for certain cases shown in the article.</p>
On the Combined Role of Cosmic Rays andSupernova-Driven Turbulence for Galactic Dynamos
<p>"b_data_cr.h5" contains the data from the model CR</p>
Dynamo: a Tailored Lifestyle Promotion Intervention Among Pediatric Patients With Cardiometabolic Risk Factors
ClinicalTrials.gov study NCT01736748. IPD Sharing: Not stated. Countries: 1. Publications: 0.
DynaMO, a package identifying transcription factor binding sites in dynamical ChIPSeq/RNASeq datasets, identifies transcription factors driving yeast ultradian and mammalian circadian cycles
GEO Series GSE72263. Saccharomyces cerevisiae. 30 samples. Type: Expression profiling by high throughput sequencing; Genome binding/occupancy profiling by high throughput sequencing.
scripts to reproduce simulations from Simulations of dynamo action in slowly rotating M dwarfs: Dependence on dimensionless parameters
<p>Scripts with .in and .local files to re-run the simulations presented in the paper Simulations of dynamo action in slowly rotating M dwarfs: Dependence on dimensionless parameters.</p>
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