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Strong relativistic electron flux events in GPS orbit (2000 - 2020)

Relativistic electrons cause internal charging on satellites and are a significant space weather hazard. In this study we analyse approximately 20 years of data from the US Global Positioning System (GPS) satellite NS41 to determine the conditions associated with the largest daily averaged fluxes of E = 2.0 MeV relativistic electrons. The largest flux events at L = 4.5 and L = 6.5 were associated with moderate to strong coronal mass ejection (CME)-driven geomagnetic storms. However, the majority of the fifty largest flux events at L = 4.5 (30 out of 50) and L = 6.5 (37 out of 50) were associated with high speed solar wind streams from coronal holes. Both solar drivers are thus very important for relativistic electron flux enhancements in GPS orbit. The 1 in 3 year flux level was not exceeded following any of the fifteen largest geomagnetic storms as monitored by the Dst index (Disturbance storm time index), showing that the largest geomagnetic storms, most often associated with extreme space weather, do not result in significantly larger relativistic electron flux events in GPS orbit.





The datasets include a summary plot of the month associated with the largest flux of 2.0 MeV electrons in GPS orbit during the study period (Figure 1) and a summary plot of the month associated with the largest geomagnetic storm during the study period (Figure 2). The fifty largest 2.0 MeV flux events at L = 4.5 as a function of the minimum Dst of the associated storm are provided in Figure 3.csv, the peak 2.0 MeV electron fluxes associated with the fifteen largest geomagnetic storms at L = 4.5 as a function of the minimum Dst of each of the storms are provided in Figure 4.csv, and the fifty largest 2.0 MeV flux events at L = 4.5 and the sunspot number are provided as a function of time in Figure 5_events.csv and Figure_5_sunspots.csv respectively. The characteristic widths of the fifty largest flux enhancements at L = 4.5 and L = 6.5 are provided in Figure 6.csv. Finally, the fifty largest 2.0 MeV flux events at L = 6.5 as a function of the minimum Dst of the associated storm are provided in Figure 7.csv, the peak 2.0 MeV electron fluxes associated with the fifteen largest geomagnetic storms at L = 6.5 as a function of the minimum Dst of each of the storms are provided in Figure 8.csv, and the fifty largest 2.0 MeV flux events at L = 6.5 and the sunspot number as a function of time are provided in in Figure 9_events.csv and Figure_9_sunspots.csv respectively.





The research leading to these results has received funding from the Natural Environment Research Council (NERC) grants NE/V00249X/1 (Sat-Risk), NE/X000389/1 and NE/R016038/1.

Simple

Date (Creation)
2024-09-16
Date (Revision)
2024-09-16
Date (Publication)
2024-09-16
Date (released)
2024-09-16
Edition

1.0

Unique resource identifier
https://doi.org/10.5285/dd8dee98-b75e-4b2f-a002-3f00bcc29d35
Codespace

doi

Unique resource identifier
GB/NERC/BAS/PDC/01885
Codespace

https://data.bas.ac.uk/

Unique resource identifier
NE/X000389/1
Codespace

award

Unique resource identifier
NE/R016038/1
Codespace

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Other citation details

Please cite this item as: Meredith, N., Cayton, T., & Cayton, M. (2024). Strong relativistic electron flux events in GPS orbit (2000 - 2020) (Version 1.0) [Data set]. NERC EDS UK Polar Data Centre. https://doi.org/10.5285/dd8dee98-b75e-4b2f-a002-3f00bcc29d35

Credit

No credit.

Status
Completed
Point of contact
Organisation name Individual name Electronic mail address Role
British Antarctic Survey Meredith, Nigel Author
Cayton, Thomas Author

Cayton, Michael

Author
NERC EDS UK Polar Data Centre

PDCServiceDesk@bas.ac.uk

Point of contact
Maintenance and update frequency
As needed
Maintenance note
Completed
Global Change Master Directory (GCMD) Science Keywords
  • EARTH SCIENCE > Sun-earth Interactions > Solar Energetic Particle Flux > Electron Flux
  • EARTH SCIENCE > Solid Earth > Geomagnetism
Theme
  • Geomagnetic Storms

  • Medium Earth Orbit

  • Relativistic electrons

Place
  • Circular orbit of 20,200 km. Inclination: 55 degrees Magnetosphere (other)

GEMET - INSPIRE themes, version 1.0

  • Atmospheric conditions
  • Geology
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no limitations to public access
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no limitations
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License
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Open Government Licence v3.0
Use constraints
Other restrictions
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Data supplied under Open Government Licence v3.0

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None

Unique resource identifier
url
Codespace

url

Association Type
Larger work citation
Unique resource identifier
url
Codespace

url

Association Type
Cross reference
Unique resource identifier
url
Codespace

url

Association Type
Cross reference
Unique resource identifier
url
Codespace

url

Association Type
Cross reference
Spatial representation type
Text, table
Language
English
Character set
UTF8
Topic category
  • Climatology, meteorology, atmosphere
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W
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Begin date
2000-12-10
End date
2020-07-25
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.

Title

European Petroleum Survey Group (EPSG) Geodetic Parameter Registry

Date (Publication)
2008-11-12
Cited responsible party
Organisation name Individual name Electronic mail address Role

European Petroleum Survey Group

EPSGadministrator@iogp.org

Publisher
Unique resource identifier
urn:ogc:def:crs:EPSG::3031
Version

6.18.3

Distributor

Distributor contact
Organisation name Individual name Electronic mail address Role
NERC EDS UK Polar Data Centre

PDCServiceDesk@bas.ac.uk

Distributor
Distributor format
Name Version
text/csv
Units of distribution

bytes

Transfer size
589824
OnLine resource
Protocol Linkage Name

WWW:LINK-1.0-http--link

http://ramadda.data.bas.ac.uk/repository/entry/show?entryid=dd8dee98-b75e-4b2f-a002-3f00bcc29d35

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Dataset
Statement

Methodology:

The data used in this study were collected by the Burst Detector Dosimeter IIR (BDD-IIR) on board the US GPS satellite NS41. The data is publicly available from http://www.ngdc.noaa.gov/stp/space-weather/satellite-data/satellite-systems/gps/data/ns41. Full details of the subsequent analysis are given in Meredith et al. (2024).

Data collection:

BDD-IIR is a multi-purpose silicon detector system. It features 8 individual channels of a "shield/filter/sensor" design that permits the detector to sample roughly half the celestial sphere while at the same time shielding the silicon sensor elements from most of the incident particle flux.

Data quality:

The particle data have been calibrated and quality-controlled prior to release.

Metadata

File identifier
dd8dee98-b75e-4b2f-a002-3f00bcc29d35 XML
Metadata language
English
Character set
UTF8
Hierarchy level
Dataset
Hierarchy level name

dataset

Date stamp
2024-09-16
Metadata standard name

ISO 19115 Geographic Information - Metadata

Metadata standard version

ISO 19115:2003(E)

Metadata author
Organisation name Individual name Electronic mail address Role
NERC EDS UK Polar Data Centre

polardatacentre@bas.ac.uk

Point of contact
 
 

Overviews

Spatial extent

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Keywords

Geomagnetic Storms Medium Earth Orbit Relativistic electrons
GEMET - INSPIRE themes, version 1.0

Atmospheric conditions Geology
Global Change Master Directory (GCMD) Science Keywords

EARTH SCIENCE > Solid Earth > Geomagnetism EARTH SCIENCE > Sun-earth Interactions > Solar Energetic Particle Flux > Electron Flux


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