Electron Electromagnetic Ion Cyclotron diffusion coefficients calculated from Van Allen Probe observations
Electromagnetic Ion Cyclotron (EMIC) wave are important for the losses of ultra-relativistic electrons from the Earth's radiation belts. In this work, statistical EMIC diffusion coefficients are calculated from Van Allen Probe A observations of EMIC waves from the entire mission. The diffusion coefficient calculations include the observed L* and activity dependent distributions in plasma density and wave spectra so that the wave-particle interactions modelled are representative of those in the radiation belts. These diffusion coefficients can be included into global radiation belt simulations such as the BAS radiation belt model. The study is published in Ross et al 2021, JGR: Space Physics.
Funding was provided by National Environment Research Council Highlight Topic grant NE/P01738X/1 (Rad-Sat), National Environment Research Council grant NE/R016445/1 and NE/R016038/1.
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- Date (Creation)
- 2021-11-02
- Date (Revision)
- 2021-11-02
- Date (Publication)
- 2021-11-02
- Date (released)
- 2021-11-02
- Edition
- 1.0
- Unique resource identifier
- https://doi.org/10.5285/cc48c65d-5395-45a1-a60a-3a4b987fd673
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- doi
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- GB/NERC/BAS/PDC/01580
- Codespace
- https://data.bas.ac.uk/
- Unique resource identifier
- NE/P01738X/1
- Codespace
- award
- Unique resource identifier
- NE/R016445/1
- Codespace
- award
- Unique resource identifier
- NE/R016038/1
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- Other citation details
- Please cite this item as: Ross, J., & Glauert, S. (2021). Electron Electromagnetic Ion Cyclotron diffusion coefficients calculated from Van Allen Probe observations (Version 1.0) [Data set]. NERC EDS UK Polar Data Centre. https://doi.org/10.5285/cc48c65d-5395-45a1-a60a-3a4b987fd673
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https://www.bas.ac.uk/team/business-teams/information-services/uk-polar-data-centre/
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- asNeeded As needed
- Maintenance note
- completed Completed
- Theme
-
- Electromagnetic Ion Cyclotron Waves
- Radiation belts
- Van Allen Probes
- ultra-relativistic electrons
- Place
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- 3.0 <= L* <= 5.5 Van Allen Radiation Belts
- GEMET - INSPIRE themes, version 1.0
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- Data supplied under Open Government Licence v3.0
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- Spatial representation type
- textTable Text, table
- Metadata language
- engEnglish
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- Climatology, meteorology, atmosphere
- Begin date
- 2012-09-01
- End date
- 2019-10-31
- Supplemental Information
- It is recommended that careful attention be paid to the contents of any data, and that the author be contacted with any questions regarding appropriate use. If you find any errors or omissions, please report them to polardatacentre@bas.ac.uk.
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Methodology:
Data sources:
* OMNIWeb (https://omniweb.gsfc.nasa.gov) for the geomagnetic and solar wind indices.
* Van Allen Probes data the Level 3 and Level 4 EMFISIS magnetometer data obtained from http://emfisis.physics.uiowa.edu/data/index.
Data collection:
Code: BAS-RBM (Glauert, S. A., Horne, R. B., and Meredith, N. P. (2014), Three-dimensional electron radiation belt simulations using the BAS Radiation Belt Model with new diffusion models for chorus, plasmaspheric hiss, and lightning-generated whistlers, J. Geophys. Res. Space Physics, 119, 268- 289, doi:10.1002/2013JA019281.)
Code: PADIE (Glauert, S. A., and Horne, R. B. (2005), Calculation of pitch angle and energy diffusion coefficients with the PADIE code, J. Geophys. Res., 110, A04206, doi:10.1029/2004JA010851.)
Data quality:
The magnetometer data using in the study are converted in to spectra following the procedure described in the accompanying paper. EMIC waves were identified in the resulting spectra using a visual identification and machine learning, the method excluded features that cannot reliably be identified as EMIC waves.
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- 2021-11-02
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