Abstract:
This dataset contains solution data produced by the BAS-PRO proton radiation belt model for the study "Modelling Inner Proton Belt Variability at Energies 1 to 10MeV using BAS-PRO". The solution data is in the form of 3D grids describing phase space density computed during dynamic simulations of Earth's proton belt over the modelling period 2014 to 2018. Three model runs are included: SA19, J81 and S16. Files were produced in May 2021.
This work was funded by the Natural Environment Research Council (NERC) via Doctoral Training Programme NE/R009457/1. Richard B. Horne and Sarah A. Glauert were supported by NERC National Capability grants NE/R016038/1 and NE/R016445/1, and by NERC grant NE/V00249X/1 (Sat-Risk), and by Highlight Topic Grant NE/P01738X/1 (Rad-Sat). Giulio Del Zanna acknowledges support from STFC (UK) via the consolidated grants to the atomic astrophysics group (AAG) at DAMTP, University of Cambridge (ST/P000665/1 and ST/T000481/1). Seth G. Claudepierre acknowledges support from NASA Grant no. NNX17AF10G and from RBSP-ECT funding provided by JHU/APL Contract 967399 under NASA''s Prime Contract NAS5-01072.
Keywords:
BAS-PRO proton solution flux
Lozinski, A., Horne, R., Glauert, S., Del Zanna, G., & Claudepierre, S. (2021). Solutions to BAS-PRO model runs for Modelling 1-10MeV Proton Phase Space Density (Version 1.0) [Data set]. NERC EDS UK Polar Data Centre. https://doi.org/10.5285/27a89a5f-ca5d-471a-a0e7-060d0911b2d1
Use Constraints: | Data supplied under Open Government Licence v3.0 http://www.nationalarchives.gov.uk/doc/open-government-licence/version/3/. |
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Creation Date: | 2021-09-20 |
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Dataset Progress: | Complete |
Dataset Language: | English |
ISO Topic Categories: |
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Parameters: |
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Personnel: | |
Name | UK PDC |
Role(s) | Metadata Author |
Organisation | British Antarctic Survey |
Name | Alexander Lozinski |
Role(s) | Investigator, Technical Contact |
Organisation | British Antarctic Survey |
Name | Prof Richard Horne |
Role(s) | Investigator |
Organisation | British Antarctic Survey |
Name | Dr Sarah Glauert |
Role(s) | Investigator |
Organisation | British Antarctic Survey |
Name | Giulio Del Zanna |
Role(s) | Investigator |
Organisation | University of Cambridge |
Name | Seth Claudepierre |
Role(s) | Investigator |
Organisation | University of California, Los Angeles |
Parent Dataset: | N/A |
Quality: | The outer boundary is driven by fits to equatorial pitch angle distributions derived from the RBSPICE ISRHELT, MagEIS pix2 and REPT instruments, and is subject to some uncertainty. The phase space density of protons with dipole mirror points at 585km altitude or below is assumed to be zero. The phase space density at L < 1.15 is assumed to be zero. |
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Lineage: | Each solution directory contains two sets of grids describing phase space density multiplied by the proton rest mass cubed (units km-6 s3). One set of grids (dynamic output, files ending in 'dyn.txt') describes phase space density at regular epochs (listed in the axis_t_dyn.txt file) throughout the simulation period for energies 1-19MeV. The other set of grids (final output, files not ending in 'dyn.txt') describes phase space density at the final epoch of the simulation across the entire model grid. |
Temporal Coverage: | |
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Start Date | 2014-01-01 |
End Date | 2018-02-01 |
Location: | |
Location | N/A |
Detailed Location | 1.15 <= L-shell <= 2 |
Distribution: | |
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Distribution Media | Online Internet (HTTP) |
Distribution Size | 4.5 GB |
Distribution Format | N/A |
Fees | N/A |
Data Storage: | 789 ASCII text files totalling 4.5 GB |