Comparisons of High‐Linear Energy Transfer Spectra on the ISS and in Deep Space-Reference-Cited by-同舟云学术

Comparisons of High‐Linear Energy Transfer Spectra on the ISS and in Deep Space

Published:2019-03 Issue:3 Volume:17 Page:396-418
ISSN:1542-7390
Container-title:Space Weather
language:en
Short-container-title:Space Weather

Author:

Zeitlin C.¹^ORCID,Narici L.²³,Rios R. R.¹,Rizzo A.²,Stoffle N.¹,Hassler D. M.⁴^ORCID,Ehresmann B.⁴^ORCID,Wimmer‐Schweingruber R. F.⁵^ORCID,Guo J.⁵^ORCID,Schwadron N. A.⁶^ORCID,Spence H. E.⁶^ORCID

Affiliation:

1. Leidos Innovations Corporation Houston TX USA

2. Department of PhysicsUniversity of Rome Tor Vergata Rome Italy

3. INFN Tor Vergata Rome Italy

4. Planetary Science DivisionSouthwest Research Institute Boulder CO USA

5. Department of Extraterrestrial PhysicsChristian Albrechts University Kiel Germany

6. Department of PhysicsUniversity of New Hampshire Dover NH USA

Funder

Agenzia Spaziale Italiana

European Space Agency

Deutsches Zentrum für Luft- und Raumfahrt

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2018SW002103

Reference63 articles.

1. Conversion between different forms of LET

2. DOSIS & DOSIS 3D: long-term dose monitoring onboard the Columbus Laboratory of the International Space Station (ISS)

3. Straggling in thin silicon detectors

4. The HEAO-3 Cosmic Ray Isotope spectrometer

5. The deep space galactic cosmic ray lineal energy spectrum at solar minimum

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