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31 results for “electron precipitation”

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zenodo32/100

On the importance of using event-specific wave pitch angle diffusion rates in modeling diffuse electron precipitation

<p>These are simulation results from running RAM-SCB and GLOW models. Two simulations were conducted. One uses diffusion coefficients derived based on statistical wave properties (&quot;stat&quot;), and the other uses coefficients from event-specific simultaneous wave properties (&quot;event&quot;). Data include the precipitating electron flux, wave diffusion coefficients, and height profiles of ionospheric electron density.</p>

opencc-by-4.0Aug 2021View details →
zenodo32/100

Energetic electron precipitation induced by oblique whistler mode chorus emissions

<p>This dataset includes the simulation results of Green&#39;s function and convolution integrals for a paper submitted to JGR-Space Physics.</p> <p>&nbsp;</p>

opencc-by-4.0May 2021View details →
zenodo32/100

Data set of Precipitation rates of electrons interacting with lower-band chorus emissions in the inner magnetosphere

<p>Simulation data for paper entitled &quot;Precipitation rates of electrons interacting with lower-band chorus emissions in the inner magnetosphere&quot;</p>

opencc-by-4.0Dec 2022View details →
zenodo32/100

Simulation Results for "Characteristics of Electron Precipitation Directly Driven by Poloidal ULF waves"

<p>This dataset contains the simulation results and the corresponding code to produce the figures in the manuscript &quot;Characteristics of Electron Precipitation Directly Driven by Poloidal ULF waves&quot;. The name of each data file indicates its corresponding figure, and the Matlab code could be used to produce the figures in the manuscript.</p>

opencc-by-4.0Jan 2023View details →
zenodo28/100

Defense Meteorology Satellite Program (DMSP) Electron Precipitation (SSJ) Auroral Boundaries, 2010-2014

<p>This dataset contains comma seperated value (CSV) files describing the equatorward and poleward edges of the auroral oval in magnetic and geocentric coordinates as determined in Kilcommons et al. 2017 (https://doi.org/10.1002/2016JA023342), using the ssj_auroral_boundary Python package version 1 (https://doi.org/10.5281/zenodo.3267414) This dataset spans 15 satellite years 2010-2014, DMSP spacecraft flights 16, 17 and 18.</p>

opencc-by-4.0Aug 2019View details →
zenodo28/100

Data for "Unraveling the Atmospheric Energy Input and Ionization due to EMIC-Driven Electron Precipitation from ELFIN's Observations"

<p>Dataset relative to the paper&nbsp;"Unraveling the Atmospheric Energy Input and Ionization due to EMIC-Driven Electron Precipitation from ELFIN's Observations"</p><ol><li>case_study.zip: ELFIN&amp;POES conjunction<ol><li>POES flux is in&nbsp;#/s/cm2/sr/keV</li><li>ELFIN flux is in&nbsp;#/s/cm2/sr/MeV</li></ol></li><li>EMICdriven_events_atmospheres_temps: background atmosphere density &amp; temperature for all 144 events<ol><li>Density is in&nbsp;g/cm3</li></ol></li><li>EMICdriven_events_nflux_PA_en: ELFIN events number flux 0°-90°<ol><li>ELFIN flux is in&nbsp;#/s/cm2/sr/MeV (...nflux.csv files)</li><li>ELFIN pitch-angle is in degrees (...nflux_PA.csv files)</li></ol></li><li>EMICdriven_events_nflux_PA_en: ELFIN events number flux 0°-180°<ol><li>ELFIN flux is in&nbsp;#/s/cm2/sr/MeV (...nflux.csv files)</li><li>ELFIN pitch-angle is in degrees (...nflux_PA.csv files)</li></ol></li><li>energy_deposition.csv: energy deposition vs altitude</li><li>ionization_rates.csv: ionization rate vs altitude</li><li>lat_lon_ionization.csv: time of EMIC-driven events with lat/lon, ionization&amp;altitude peak and energy flux</li><li>avg_atm_density.csv: average background density</li><li>mean_PAD: mean PAD in&nbsp;#/s/cm2/sr/eV</li><li>median_PAD: median PAD in&nbsp;#/s/cm2/sr/eV</li></ol>

opencc-by-4.0Aug 2023View details →
zenodo24/100

Data for the paper "Impacts of soft electron precipitations on the neutral density and satellite drag during the 28-29 May 2010 geomagnetic storm"

<p>Data for the paper&nbsp;&quot;Impacts of soft electron precipitations on the neutral density and satellite drag during the 28-29 May 2010 geomagnetic storm&quot; by Qingyu Zhu, Yue Deng, Cheng Sheng, Phil Andersen and&nbsp;Aaron Bukowski</p> <p>GITM_3D.zip: GITM outputs at 12 UT, 05/29/2010 (Figure 3)</p> <p>HPs.zip: NOAA and Z2019 HP (Figure 1)</p> <p>rhos.zip: Neutral density along the GOCE orbit from observation, run1, run2, run3 and JB2008 model (Figures 2 and 4)</p>

opencc-by-4.0Jun 2020View details →
nasa16/100

RENU2 Electron Plasma Detector (EPLAS) Precipitating Electron Total Energy Flux, (H0), 42 ms Data

RENU2 Electron Plasma Detector (EPLAS) Precipitating Electron Total Energy Flux

restrictednotspecifiedApr 2025View details →
nasa12/100

DMSP F18 Special Sensor J, SESS/SSJ5, Precipitating Electrons and Ions Observed at 850 km, 1 s Data

Precipitating Electrons And ions observed at nominally 850 km Altitude and over a Range of Energies from 30 eV to 30 keV by using the Special Sensor J, SSJ, Instrument. Please contact Rob.Redmon@noaa.gov with Questions and Comments. Many Individuals made Important Contributions including: D. Hardy, E. Holeman, F. Rich, D. Ober, G. Wilson, J. Machuzak, K. Kadinsky-Cade, J. McGarity, W.F. Denig, K. Martin, R. Redmon, D. Knipp, L. Kilcommons.

restrictednotspecifiedApr 2025View details →
nasa12/100

DMSP F17 Special Sensor J, SESS/SSJ5, Precipitating Electrons and Ions Observed at 850 km, 1 s Data

Precipitating Electrons And ions observed at nominally 850 km Altitude and over a Range of Energies from 30 eV to 30 keV by using the Special Sensor J, SSJ, Instrument. Please contact Rob.Redmon@noaa.gov with Questions and Comments. Many Individuals made Important Contributions including: D. Hardy, E. Holeman, F. Rich, D. Ober, G. Wilson, J. Machuzak, K. Kadinsky-Cade, J. McGarity, W.F. Denig, K. Martin, R. Redmon, D. Knipp, L. Kilcommons.

restrictednotspecifiedApr 2025View details →
nasa12/100

DMSP F16 Special Sensor J, SESS/SSJ5, Precipitating Electrons and Ions Observed at 850 km, 1 s Data

Precipitating Electrons And ions observed at nominally 850 km Altitude and over a Range of Energies from 30 eV to 30 keV by using the Special Sensor J, SSJ, Instrument. Please contact Rob.Redmon@noaa.gov with Questions and Comments. Many Individuals made Important Contributions including: D. Hardy, E. Holeman, F. Rich, D. Ober, G. Wilson, J. Machuzak, K. Kadinsky-Cade, J. McGarity, W.F. Denig, K. Martin, R. Redmon, D. Knipp, L. Kilcommons.

restrictednotspecifiedApr 2025View details →

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International Brain Laboratory public data

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