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12 results for “ring current”
Data for: Ring Current Electron Precipitation During the 17 March 2013 Geomagnetic Storm: Underlying Mechanisms and Their Effect on the Atmosphere
<p>All data are included as MATLAB figure files, png files and MATLAB MAT files.</p><p>File precipitated_flux.mat contains a 4-D array of values of precipitated electron flux in [1/(s cm^2 keV)] for 289 time points from 16 March 2013 to 19 March 2013, with a 15 min time step; 100 values of energy in a range from 10 keV to 1 MeV, with a 10 keV step; on a spatial grid of 28 by 49 (P, R).</p><p>netCDF data can be opened with a variety of software tools, including Matlab, Origin or Python.</p>
Does ring current heating generate the observed O+ shell?: Numerical information for the figures
<p>This archive contains data files needed to reproduce selected figures from the following manuscript:</p> <p>Does ring current heating generate the observed O+ shell?<br> by J. Krall, J. D. Huba, and M.-C. Fok</p> <p>This manuscript was submitted to Geophyscial Research Letters in April, 2020</p> <p>In addition, this archive contains CIMI code output giving Coulomb heating losses from the ring current<br> and a SAMI3 subroutine that describes the heating function used to mimic ring current heating.</p>
Stormtime ring current heating of the ionosphere and plasmasphere Numerical information for the figures
<p>This archive contains data files needed to reproduce selected figures from the following manuscript:</p> <p>Stormtime ring current heating of the ionosphere and plasmasphere<br> by J. Krall, M.-C. Fok, J. D. Huba, and A. Glocer</p> <p>This manuscript was submitted to Journal of Geophysical Research: Space<br> Physics in February, 2022</p> <p>Specifically, this archive contains one IDL file for each figure. If run, the<br> IDL script reads one or more of the datasets and re-creates the figure.<br> Each IDL script is a text-formatted file with a header that explains each file.<br> Individual datasets are either text-formatted or unformatted FORTRAN data<br> files. Also included is a namelist file giving SAMI3 input parameters.</p>
The contribution of plasma sheet bubbles to stormtime ring current buildup and evolution of the energy composition
<p>Supporting information for "The contribution of plasma sheet bubbles to stormtime ring current buildup and evolution of the energy composition" by Sciola et al. 2023 submitted to the Journal of Geophysical Research: Space Physics</p>
Optimized geometries for Global Aromatic Ring Currents in Neutral Porphyrin Nanobelts
<p>Optimized geometries for Global Aromaticity in Neutral Porphyrin Nanobelts</p>
Dataset of "Quantifying the Effects of Magnetic Field Line Curvature Scattering on Radiation Belt and Ring Current Particles"
<p>Dataset of "Quantifying the Effects of Magnetic Field Line Curvature Scattering on Radiation Belt and Ring Current Particles".</p><p>The following contains the simulation data used for drawing.</p>
Processed Data for Ring Current Oxygen Ion ANN Model
<p>Processed data, including:</p> <p>the coordinate of Van Allen Probe B in SM coordinates.</p> <p>Geomagnetic indices (Sym-H, SME and F10.7).</p> <p>log10 O+ fluxes, here the unit of 38 keV and 52 keV O+ (measured by HOPE) is s-1 cm-2 ster-1 keV-1, the unit of other energy channels (measured by RBSPICE) is s-1 cm-2 MeV-1.</p>
Dataset for the 2024 Ring Current Paper
<p>The dataset inlcudes the outputs of iPic3D (EcSIM) that were used in the Rusaitis et al. (2024).</p>
Processed data of "Observations of Ring Current Proton Fast Local Loss Associated with Deepening Local Minimum in Phase Space Density in Earth's Inner Magnetosphere"
<p>The dataset includs the processed observation data of "Observations of Ring Current Proton Fast Local Loss Associated with Deepening Local Minimum in Phase Space Density in Earth’s Inner Magnetosphere". *.sav files are the phase space densities of protons and the corresponding adiabatic invariants (μ, K, and L*) which are calculated under the T89D magnetic field model (using the observation data measured by the RBSPICE on the Van Allen Probes from 24th to 26th Jun 2017), which are used to plot Figure 1. The data in Processed data for Figures 2-5.zip are the processed data for Figures 2-5. </p>
The relation among the ring current, subauroral polarization stream, and the geospace plume: MAGE Simulation of the March 31 2001 Super Storm
<p>Open data for Figure 3 to Figure 11 in manuscript, "The relation among the ring current, subauroral polarization stream, and the geospace plume: MAGE Simulation of the March 31 2001 Super Storm".</p> <p>The data was generated by the Multiscale Atmosphere Geospace Environment model.</p> <p>The manuscript is submitted to JGR for review.</p>
Data for paper "The Effect of Energetic Ion Dispersionless Injections on the Ring Current Dynamics"
<p>The injection list and processed statistical data of paper "The Effect of Energetic Ion Dispersionless Injections on the Ring Current Dynamics.</p>
Quantifying the effect of magnetic field line curvature scattering on the loss of ring current ions
<p>The datas used for the paper of "Quantifying the effect of magnetic field line curvature scattering on the loss of ring current ions"</p> <p>The file contains three folders data_kp4, data_kp5, data_kp6 for the simulations under Kp index of 4,5 and 6 respectively. Each of them contains subfolders with name including _He_, _o_, and _proton_ for the species of proton, He+ and O+ respectively. Under these subfolders there are several subfolders for the simulations under different initial equatorial x-position at the midnight. Each of them contains folders with name of data appended with numbers. Under these folders there are three important files of ini_params.dat, fin_param.dat, tdrift.dat, screenoutput.txt.</p> <p><strong>init_params.dat </strong>contains ten numbers of: energy in MeV, equatorial pitch angle in degree, initial positions Lx, y, z, radius of curvature <span class="math-tex">\(R_{c}\)</span>, <span class="math-tex">\(\kappa\)</span>, <span class="math-tex">\(\zeta_{1}, \zeta_{2}, \eta\)</span>. The last four parameters are the kappa parameter and the parameters in Young et al. 2002 used for formulating empirical formula for the single field line curvature scattering.</p> <p><strong>fin_params.dat contains five colum data: </strong>particle tag number, status if the particle (0 stay until the end of the simulations, 1 lost to the inner boundary, 2 lost to the outer boundary, 3 stopped as trapped), time of loss in second or end of simulations if stayed until the end, number of mirrorings, <span class="math-tex">\(<\frac{(\frac{\delta \mu}{\mu})^2}{2 t}>\)</span></p> <p><strong>tdrif.dat</strong> contains two column data of : particle tag number and the time in second to complete the first full drift.</p> <p><strong>screenoutput.txt </strong>contains text information of the run</p>
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