10.5285/27A89A5F-CA5D-471A-A0E7-060D0911B2D1
Lozinski, Alexander
Alexander
Lozinski
0000-0002-6508-487X
British Antarctic Survey
Horne, Richard
Richard
Horne
0000-0002-0412-6407
British Antarctic Survey
Glauert, Sarah
Sarah
Glauert
0000-0003-0149-8608
British Antarctic Survey
Del Zanna, Giulio
Giulio
Del Zanna
0000-0002-4125-0204
University of Cambridge
Claudepierre, Seth
Seth
Claudepierre
0000-0001-5513-5947
University of California, Los Angeles
Solutions to BAS-PRO model runs for Modelling 1-10MeV Proton Phase Space Density
NERC EDS UK Polar Data Centre
2021
"EARTH SCIENCE","SUN-EARTH INTERACTIONS","SOLAR ENERGETIC PARTICLE FLUX","PROTON FLUX"
BAS-PRO proton solution flux
Lozinski, Alexander
Alexander
Lozinski
0000-0002-6508-487X
British Antarctic Survey
Lozinski, Alexander
Alexander
Lozinski
0000-0002-6508-487X
British Antarctic Survey
Horne, Richard
Richard
Horne
0000-0002-0412-6407
British Antarctic Survey
Glauert, Sarah
Sarah
Glauert
0000-0003-0149-8608
British Antarctic Survey
Del Zanna, Giulio
Giulio
Del Zanna
0000-0002-4125-0204
University of Cambridge
Claudepierre, Seth
Seth
Claudepierre
0000-0001-5513-5947
University of California, Los Angeles
UK Polar Data Centre
Natural Environment Research Council, UK Research & Innovation
UK Polar Data Centre
Natural Environment Research Council, UK Research & Innovation
UK Polar Data Centre
Natural Environment Research Council, UK Research & Innovation
2014-01-01/2018-02-01
2021-09-20
2021-05-11
2021-09-20
2021-09-30
en
BAS-PRO proton solution flux
https://sat-risk.ac.uk/
https://www.bas.ac.uk/project/rad-sat/
789 files
4.5 GB
text/plain
1.0
Open Government Licence V3.0
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.
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.
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.
1.15 <= L-shell <= 2
Natural Environment Research Council, UK Research & Innovation
https://ror.org/02b5d8509
NE/R009457/1
NPIF studentships for Cambridge ESS DTP
Natural Environment Research Council, UK Research & Innovation
https://ror.org/02b5d8509
NE/R016038/1
National Capability - Polar Expertise Supporting UK Research
Natural Environment Research Council, UK Research & Innovation
https://ror.org/02b5d8509
NE/R016445/1
British Antarctic Survey - National and Public Good activity
Natural Environment Research Council, UK Research & Innovation
https://ror.org/02b5d8509
NE/V00249X/1
Satellite Radiation Risk Forecasts (Sat-Risk)
Natural Environment Research Council, UK Research & Innovation
https://ror.org/02b5d8509
NE/P01738X/1
Modelling the acceleration, transport and loss of radiation belt electrons to protect satellites from space weather (Rad-Sat)
Science and Technology Facilities Council, UK Research & Innovation
https://ror.org/057g20z61
ST/P000665/1
UNDERSTANDING THE DYNAMICAL SOLAR ATMOSPHERE
Science and Technology Facilities Council, UK Research & Innovation
https://ror.org/057g20z61
ST/T000481/1
Understanding the chromosphere-corona interface in the Solar Orbiter and DKIST era
National Aeronautics and Space Administration
https://ror.org/027ka1x80
NNX17AF10G
Data Upgrade: Calibrating Van Allen Probe Measurements of 1-20 MeV Protons