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    The high-energy proton fluxes in the SAA observed with REM aboard the MIR orbital station

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    Buhler(2002a).pdf (699.4Kb)
    Authors
    Bühler, P.
    Zehnder, A.
    Kruglanski, M.
    Daly, E.
    Adams, L.
    Show allShow less
    Discipline
    Physical sciences
    Subject
    Electrons
    High energy physics
    Particle detectors
    Protons
    Space stations
    Space radiation environment
    Cosmic rays
    proton
    article
    Atlantic Ocean
    comparative study
    electron
    Flight Experiment
    instrumentation
    long duration
    manned
    microclimate
    Mir Project
    radiation dose
    radiation monitoring
    radiation protection
    solar energy
    South America
    space flight
    statistical model
    weightlessness
    Flight Experiment
    long duration
    manned
    Mir Project
    Atlantic Ocean
    Electrons
    Extraterrestrial Environment
    Models, Statistical
    Protons
    Radiation Dosage
    Radiation Monitoring
    Radiation Protection
    Solar Activity
    South America
    Space Flight
    Spacecraft
    Weightlessness
    Audience
    Scientific
    Date
    2002
    Metadata
    Show full item record
    Description
    During two years, from November 1994 to 1996, the particle detector REM measured the highly energetic electron and proton environment at the outside of the MIR orbital station. Using mission averaged data we investigate various aspects of the proton fluxes in the SAA. Comparison with the radiation belt model AP8 reveal important differences.
    Citation
    Bühler, P.; Zehnder, A.; Kruglanski, M.; Daly, E.; Adams, L. (2002). The high-energy proton fluxes in the SAA observed with REM aboard the MIR orbital station. , Radiation Measurements, Vol. 35, Issue 5, 489-497, DOI: 10.1016/S1350-4487(02)00079-3.
    Identifiers
    uri: https://orfeo.belnet.be/handle/internal/5234
    doi: http://dx.doi.org/10.1016/S1350-4487(02)00079-3
    scopus: 2-s2.0-0036772036
    Type
    Article
    Peer-Review
    Yes
    Language
    eng
    Links
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