English
 
Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
  Contamination in electron observations of the silicon detector onboard Cluster/RAPID/IES instrument in Earth's radiation belts and ring current

Kronberg, E. A., Rashev, M. V., Daly, P. W., Shprits, Y., Turner, D. L., Drozdov, A., Dobynde, M., Kellerman, A. C., Fritz, T. A., Pierrard, V., Borremans, K., Klecker, B., Friedel, R. (2016): Contamination in electron observations of the silicon detector onboard Cluster/RAPID/IES instrument in Earth's radiation belts and ring current. - Space Weather, 14, 6, 449-462.
https://doi.org/10.1002/2016SW001369

Item is

Files

show Files
hide Files
:
1574892.pdf (Publisher version), 3MB
Name:
1574892.pdf
Description:
-
Visibility:
Public
MIME-Type / Checksum:
application/pdf / [MD5]
Technical Metadata:
Copyright Date:
-
Copyright Info:
-
License:
-

Locators

show

Creators

show
hide
 Creators:
Kronberg, E. A.1, Author
Rashev, M. V.1, Author
Daly, P. W.1, Author
Shprits, Yuri2, Author              
Turner, D. L.1, Author
Drozdov, A.1, Author
Dobynde, M.1, Author
Kellerman, A. C.1, Author
Fritz, T. A.1, Author
Pierrard, V.1, Author
Borremans, K.1, Author
Klecker, B.1, Author
Friedel, R.1, Author
2.8 Magnetospheric Physics, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum, Author              
Affiliations:
1External Organizations, ou_persistent22              
22.3 Earth's Magnetic Field, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum, ou_146030              

Content

show
hide
Free keywords: -
 Abstract: Since more than 15 years, the Cluster mission passes through Earth's radiation belts at least once every two days for several hours, measuring the electron intensity at energies from 30 to 400 keV. This data has previously been considered not usable due to contamination caused by penetrating energetic particles (protons at >100 keV and electrons at >400 keV). In this study, we assess the level of distortion of energetic electron spectra from the RAPID/IES detector, determining the efficiency of its shielding. We base our assessment on the analysis of experimental data and a radiation transport code (Geant4). In simulations, we use the incident particle energy distribution of the AE9/AP9 radiation belt models. We identify the Roederer L-values, L⋆, and energy channels that should be used with caution: at 3≤L⋆≤4, all energy channels (40 – 400 keV) are contaminated by protons (≃230 to 630 keV and >600 MeV); at L⋆≃1 and 4–6, the energy channels at 95 – 400 keV are contaminated by high energy electrons (>400 keV). Comparison of the data with electron and proton observations from RBSP/MagEIS indicates that the subtraction of proton fluxes at energies ≃ 230–630 keV from the IES electron data adequately removes the proton contamination. We demonstrate the usefulness of the corrected data for scientific applications.

Details

show
hide
Language(s): eng - English
 Dates: 2016
 Publication Status: Finally published
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: DOI: 10.1002/2016SW001369
GFZPOF: p3 PT1 Global Processes
 Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show
hide
Title: Space Weather
Source Genre: Journal, SCI, Scopus, oa ab 2020
 Creator(s):
Affiliations:
Publ. Info: -
Pages: - Volume / Issue: 14 (6) Sequence Number: - Start / End Page: 449 - 462 Identifier: CoNE: https://gfzpublic.gfz-potsdam.de/cone/journals/resource/journals459