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Determination of the influence of primary protons on the assessed neutron doses in the ISS

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Title: Determination of the influence of primary protons on the assessed neutron doses in the ISS


1
Determination of the influence of primary protons
on the assessed neutron doses in the ISS
ID 236, Neutron Dosimetry
R J Tanner, L G Hager and J S Eakins INTS24,
Bologna, September 2008
2
HPA PADC dosemeter EuCPD
EuCPD
  • Routine issue for neutron personal dosimetry
    electrochemical etch rear face
  • Calibrated for neutrons 173 MeV
  • Electrochemical etch produces indistinguishable
    tracks for neutrons, direct protons, and heavy
    ions
  • Forms a component of European Crew Personal
    Dosimeter to assess neutron dose equivalent only

3
Representative neutron energy distributions
4
Methods need to get rid of the charged particles
  • Simple method to get neutron dose

But, charged particles are recorded by other
elements of the dosemeter these can be detected
via entry and exit tracks, NCP
5
Residual range vs Emax in PADC
If E gt Emax then LET lt LETcrit
6
Calculated protons inside ISS Columbus module
GCR
SAA Belt
(T Ersmark PhD thesis, June 2006, Royal Institute
of Technology, Stockholm)
7
The problem
  • Need to avoid overestimates of the dose to
    astronauts on the ISS because a component of the
    reported neutron dose is due to charged particles
  • A correction is required the charged particles
    only exceed LETcrit near the end of their range
  • A gt 2 particles can be excluded by detection of
    entry and exit tracks
  • Can estimate the number of tracks caused by
    protons if we know the LETcrit for protons
  • Shortage of available proton beams

8
Detector stack arrangement for HIMAC irradiations
  • HIMAC irradiations provided data for 4He, 12C and
    56Fe in May 2008
  • Prior data for 20Ne
  • PMMA block in the beam to ensure ions stop in the
    PADC stack
  • Data allow etchable range of an ion to be
    estimated
  • LETcrit can be inferred

Ions
9
HIMAC 4He 105.6 MeV into PADC
2.5 m air
577.14 MeV a 116.8 mm PMMA
  • 116.8 mm PMMA
  • Trim does not include air
  • Straggling modelled well

10
4He Etchable range in PADC
Etchable 4He tracks
Quoted Fluence
D
Stack
Rcrit
D dosemeter thickness Rcrit etchable length
of track (i.e. LET gt LETcrit) F fluence
11
HIMAC 12C 1493 MeV into PADC
12
HIMAC 56Fe 9.727 GeV into PADC
Quoted F 5000 cm-2Measured F 3900 cm-2
13
LET threshold in PADC
  • Uncertainties yet to be determined
  • The LET for 56Fe will always be very high and
    will exceed the etching threshold, at any energy
  • Therefore the 56Fe measurement is a measure of
    the total fluence

14
Angle of incidence, ? vs Ep
Analysis needs refinement. qc is probably in the
35o 50o range
  • Envelope defines the energy range of etchable
    tracks
  • Assume dosemeter mounted on an ICRU tissue sphere
    inside ISS
  • Calculate tissue depth traversed to the detector
    surface for all incident angles
  • Calculate for each q, the energy range which
    produces etchable tracks

15
Revised estimate of etchable proton tracks
1.96 cm-2 d-1 3.5 d-1 (read area 1.767 cm2)
16
Neutron dose estimateMATROSHKA 2A
i.e. 31 lower than the uncorrected doses
17
Summary
  • The HPA PADC dosemeter can be used for the
    determination of the neutron dose in low earth
    orbit, but requires
  • subtraction of high energy ions with Zgt2
  • direct protons a-particles
  • So far the assessment has considered subtraction
    of
  • Z gt 2 ions by measurement after secondary
    chemical etch 17
  • Direct protons by calculation 14
  • Still to be considered
  • a-particles

18
Future Work
  • Determine experimentally the maximum proton
    energy threshold of detection currently assumed
    800 keV at the detector surface, equivalent to
    about 30 keV µm-1
  • Determine experimentally the critical angle for
    protons as a function of energy
  • Simulate the results obtained using TRIM
  • Use a more realistic shape in the calculations
    than the ICRU sphere
  • Perform a full uncertainty analysis

19
Acknowledgements
  • We would like to acknowledge the help of
  • Tore Ersmark formerly of Royal Institute of
    Technology, Stockholm, for the calculated proton
    spectra
  • Staff at DLR, Cologne, Germany for assistance in
    arranging the measurement programme
  • Staff at HIMAC, Chiba, Japan for providing the
    irradiation facilities
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