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30 results for “radiation belt”
Global occurrence of higher-bands ECH waves in radiation belts based on a novel noise reduction algorithm
<p>The database of ECH waves based on observations from Van Allen Probes between September 17, 2012 and October 13, 2019. The probe and the year of observations are marked in the data file names. The columns from left to right are: the mean value of the SuperMAG electrojet index in the previous hour, L-Shell, the magnetic local time, the magnetic latitude, the wave amplitude of band 1to band 4.</p>
Does Uranus' asymmetric magnetic field produce a relatively weak proton radiation belt?
<p>Derived data shown in figures and computer code for the publication in Geophysical Research Letters.</p>
MHD/PSD data: Simulation of Radiation Belt Wave-Particle Interactions in an MHD-particle Framework
<p>MHD and phase space density simulation results.</p>
Archimedean Spiral Distribution of Energetic Particles in Earth's Inner Radiation Belt
<p>There are three data packets in total, which are idealized RCM simulation output files related to electron distribution function and spectra for Figure 2, realistic RCM simulation output files related to electron distribution function and spectra for Figure 3, and idealized RCM simulation output files related to predicted proton distribution function and spectra for Extended Data Figure 1.</p> <p>The names of RCM simulation output files specify the simulation time in a format of "hhmmss". </p> <p>In the output files for electron or proton distribution function, the stored quantities are: "I","J","COLAT","ALOCT","BNDLOC","XMIN","YMIN","VM","FTV", "BMIN","V", "BIRK(N.H)", "EETA", "VEFF","W,eV","flux","df","P". </p> <p>In the idealized RCM simulation output files for electron or proton spectra, the stored quantities are: "I","Energy_channel","Energy","Xmin","Ymin","Diff_flux(1/keV/cm2/s/sr)","Bz". </p> <p>In the realistic RCM simulation output files for electron spectra, the stored quantities are: "Energy_channel","Positions","Energy","SC_X","SC_Y","SC_L","EQ_X","EQ_Y","EQ_Z","Diff_flux(1/keV/cm2/s/sr)","Bz"</p> <p> </p>
Archimedean Spiral Distribution of Energetic Particles in Earth's Inner Radiation Belt
<p>There are three data packets in total, which are idealized RCM simulation output files related to electron distribution function and spectra for Figure 2, realistic RCM simulation output files related to electron distribution function and spectra for Figure 3, and idealized RCM simulation output files related to predicted proton distribution function and spectra for Figure 4.</p> <p>The names of RCM simulation output files specify the simulation time in a format of "hhmmss". </p> <p>In the output files for electron or proton distribution function, the stored quantities are: "I","J","COLAT","ALOCT","BNDLOC","XMIN","YMIN","VM","FTV", "BMIN","V", "BIRK(N.H)", "EETA", "VEFF","W,eV","flux","df","P". </p> <p>In the idealized RCM simulation output files for electron or proton spectra, the stored quantities are: "I","Energy_channel","Energy","Xmin","Ymin","Diff_flux(1/keV/cm2/s/sr)","Bz". </p> <p>In the realistic RCM simulation output files for electron spectra, the stored quantities are: "Energy_channel","Positions","Energy","SC_X","SC_Y","SC_L","EQ_X","EQ_Y","EQ_Z","Diff_flux(1/keV/cm2/s/sr)","Bz"</p>
Data required to determine a catalog of radiation belt enhancement events
<p>These are the data that accompany a paper titled "Defining Radiation Belt Enhancement Events Based on Probability Distributions" by the same authors listed here. The paper will be submitted to the journal Space Weather.</p> <p>The data consist of text data files of radiation belt electron data. Each file includes a description of the contents on lines beginning with the character, #. The files are:</p> <p>LANL-GEO 1.8-3.5 MeV Data.txt which contains daily and satellite-averaged 1.8-3.5 MeV electron data from the LANL-GEO instruments. The data span 1989 through 2018.</p> <p>GOES 2 MeV Data.txt which contains daily values of maximum >2 MeV electron fluxes from the NOAA goes satellites in the same format as the file LANL-GEO 1.8-3.5 MeV Data.txt</p> <p>LANL-GEO Event Distribution.txt and GOES Event Distribution.text which contain the number of radiation belt electron events that are identified using a variable threshold flux value to define the events. </p> <p>LANL-GEO Event-Day Distribution.txt and GOES Event-Day Distribution.text which contain the number of days when radiation belt electron fluxes exceed a given threshold flux value.</p> <p>Catalog of Events.pdf which is a catalog of moderate, strong, and intense radiation belt enhancement events for the 1989 through 2018. </p> <ul> <li>Moderate Events are defined as those that occur on average 100 times per 11-year solar cycle, Flux > 5.37 (cm2-s-sr-keV)<sup>-1</sup></li> <li>Strong Events are defined as those that occur on average 100 times per 11-year solar cycle, Flux > 17.8 (cm2-s-sr-keV)<sup>-1</sup></li> <li>Strong Events are defined as those that occur on average 100 times per 11-year solar cycle, Flux ≳ 46.7 (cm2-s-sr-keV)<sup>-1</sup></li> </ul> <p>These data files can be used reproduce our analysis or, more importantly, they can be used for additional studies of the causes and consequences of radiation belt enhancement events.</p>
Simulation data for "Modeling radiation belt dynamics using a positivity-preserving finite volume method on general meshes"
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Simulation data and code for "Modeling radiation belt dynamics using a positivity-preserving finite volume method on general meshes"
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Empirically estimated electron lifetimes in the Earth's radiation belts: 1. Observations
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Empirically estimated electron lifetimes in the Earth's radiation belts: 2. Comparison with theory
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