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NIRS ISRL Intercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray with Heavy Ion Beams At NIRS Y.Uchihori, K.Fujitaka, N.Yasuda, (National Institute of Radiological Sciences, Japan) and E.Benton (Eril Research Inc., USA)

NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

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Page 1: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams

InterComparison for Cosmic-ray with Heavy Ion Beams At NIRS

Y.Uchihori, K.Fujitaka, N.Yasuda, (National Institute of Radiological Sciences, Japan)

andE.Benton (Eril Research Inc., USA)

Page 2: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLObjectives of ICCHIBAN

• Establish and characterize a heavy ion “reference standard” against which space radiation instruments can be calibrated.

• Determine the response of space radiation dosimeters to heavy ions of charge and energy similar to that found in the galactic cosmic radiation (GCR) spectrum.

• Aid in reconciling differences in measurements made by various radiation instruments during space flight.

Page 3: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLICCHIBAN Runs

• Opportunity for two or three runs per year.

• 1st ICCHIBAN: active detectors, shake down run

• 2nd ICCHIBAN: passive detectors

• Participants/Detectors not included in first two runs will have opportunity later.

Page 4: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLIntercomparison Program

Page 5: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLHIMAC (Heavy Ion Medical Accelerator in Chiba)

Available Ionsp, He, C, Ne, Si, Ar, Fe, Kr, Xe, …

Energies125~800MeV/u

SynchrotronLinear Accelerator 2 Rings

Page 6: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLHIMAC Cancer Therapy

Dose distribution of various radiations

Neutron

ray

Proton

Carbon

Depth from Surface of Body (cm)

Cancer

Rel

ativ

e D

ose

(%)

Bolus

Bolus

Carbon

Carbon

Cancer

Spinal Cord

About 1000 patients had treatment in HIMAC.

Page 7: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLOperation of HIMAC

• During day time on week day, HIMAC ion beams are used for the treatment of patients.

• During night time on week day or day time on weekend, they are used for the biology and physics experiments.

nightdaynightdaynightdaynightdaynightdaynightdaynightday

SunSatFriThuWedTueMon

Treatment Maintenance No Service

Physics and Biology Experiments are available.

Page 8: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLIrradiation Room in HIMAC

• Treatment Rooms for Patient --- 3 rooms

• A Biological Experiment Room (BIO)

• Physics Experiment Rooms– Direct Beam Courses --- 2 courses (PH1, PH2)– Secondary Beam Courses --- 2 courses (SB2, SB3)

(Upper Ring)

(Lower Ring)

(Upper & Lower Ring)

Treatment Room

Page 9: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLICCHIBAN Working Group

• Yukio Uchihori (Project Coordinator), NIRS, Japan• Kazunobu Fujitaka (Chair), NIRS, Japan• Nakahiro Yasuda (Deputy Project Coordinator), NIRS, Japan• Eric Benton (Deputy Project Coordinator), Eril Research, USA• Tadayoshi Doke, Waseda University, Japan• Hisashi Kitamura, NIRS, Japan• Tatsumi Koi, NIRS, Japan• Masashi Takada, NIRS, Japan• Cary Zeitlin, LBNL, USA

Page 10: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLOrganizing Committee of WRMISS Intercomparison

• Guenther Reitz (Chair), German Aerospace Center (DLR), Germany

• Kazunobu Fujitaka, National Institute of Radiological Sciences (NIRS), Japan

• Jack Miller, Lawrence Berkeley National Laboratory, USA• Thomas Borak (Liaison with WG), Colorado State

University, USA• Rudolf Beaujean, University of Kiel, Germany

Page 11: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLParticipants for 1st ICCHIBAN (to date)

Detector TypeDetector NameNationParticipants

Silicon Stack DetectorGrand Base DetectorsUSAC. Zeitlin & J. Miller

CR-39 + TLDCR-39 + TLDUSAE. Benton

CR-39 + TLDCR-39 + TLDJapanY. Tawara & N. Yasuda

Mobile Si DosimeterLiulin-4JJapanY. Uchihori

TEPC + Silicon&CTEPC + CPDSUSAJSC, NASA

Silicon Stack DetectorDOSTELGermanR. Beaujean & G. Reitz

Silicon Stack DetectorRRMD-IIIJapanT. Doke

Page 12: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLSchedule of 1st ICCHIBAN

2nd Group

1st Group

2nd Group

1st Group

Fe(400MeV/u)20:00~7:00WedFeb. 13

Fe(400MeV/u)20:00~7:00TueFeb. 12

C(400MeV/u)20:00~7:00MonFeb. 11

C(400MeV/u)20:00~7:00SunFeb. 10

Page 13: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLRequirement for Participants after Experiments

• LET or y Distribution

• Mean Quality Factors

• Dose (to Tissue) per 106 Particles

• Dose Equivalent per 106 Particles

• To be determined

Page 14: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLAvailable Beam in 1st ICCHIBAN

• HIMAC Committee realized importance of our project and approved 4 nights ~ 40 hours for 1st ICCHIBAN runs.

• 2 nights for Carbon (400MeV/u) and 2 nights for Iron (400MeV/u) are available.

• Beam Intensity will be tuned 3x102 particles per spill. 1 spill every 3.3 sec. Spill distribution is about 0.7 sec.

• The beam spot will be tuned as 20 mm diameter circles.

Page 15: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLBeam Characteristics to be provided to participants

• Actual Beam Energy at Detector

• Geometric Beam Profile (We can provide position of each particle.)

• Time Structure of Beam

• Fluence and Average Beam Intensity

Page 16: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLReference Measurements

• Single Spill Profile --- ZnS Fluorescence Sheet + Video Camera• Average Beam Profile --- CR-39• Real Time Beam Profile --- PSD• Beam Intensity --- Plastic Scintillation Counter• Total Beam Energy --- Silicon Stack

Reference Measurement

SC PSD Silicon Stack

Page 17: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLTrigger System

Page 18: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLExposures of dosimeters

• Dosimeters will be irradiated for direct beam after transmitting a thin scintillation counter. The scintillation counter will count the beam intensity and give trigger signal for the dosimeter if required.

• Detectors can be rotated with the Theta stage and it will be irradiated with several incident angles.

Direct Beam

SC PSD Dosimeter

XZ stage

Theta stage

Page 19: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLFlow Chart of ICCHIBAN Exposure

?

Page 20: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLTime Schedule

Suggestions for next accelerator run,(i.e. ions, energy, dates)Jun. 15, 2002

3rd ICCHIBAN Experiment(End, 2002)

2nd ICCHIBAN Experiments(For Passive Detectors)May, 2002

Preliminary Report of data Apr. 30, 2002

1st ICCHIBAN ExperimentFeb. 10-13, 2002

Procedure for Radiation Control, Visiting Researcher and Hotel reservationNov. 30, 2001

2nd CircularOct. 15, 2001

6th WRMISS Workshop at OxfordSep. 12, 2001

EventDate

will continue for two more years

Page 21: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRL2nd ICCHIBAN Experiments

• 2nd ICCHIBAN Experiment will be held on May, 2002 and it will be concentrated with “Passive Detectors”. These exposures will be done in “Biology Room (BIO)”.

• Possibility to include “unknown ions” (blind exposures) in addition to “known ions”.

• Participants with passive detectors need not attend in person (send detectors to ICCHIBAN WG).

Page 22: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLPre-Experiment

• Aug. 8th, 2001• Iron 500 MeV/u• Intensity ~ 103~6 particles

per spill• Beam Profile ~ 2cm circle

• Detectors– Silicon stack detector– CR-39– Liulin-4J

Page 23: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLPSD Position Resolution

Page 24: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLCR-39 and PSD

40 mm

10 mm

PSD

CR-39

Scanning region

Page 25: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLCall for ICCHIBAN

• We hope this project will succeed and it will contribute to our understanding of space radiation instruments.

• We are eager for your participation to ICCHIBAN.

• If you have interest in ICCHIBAN, please contact me ( [email protected] ).

Page 26: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLRICH (Ring Image Cherenkov)

( )β

θλ

λ n1cos =

dxdnc

zedxdN νβ

πν

−= 222

22 112

θ

TransparentMaterial

High EnergyCharged Particle

N:Number of Photons

ν:Frequency of Light

z:Charge of Particle

b : Velocity of Particle(v/c)

n:Refractive Index

Page 27: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLRICH Setup

PSD

Black Box

SC PSDRadiator MAPMT

SC : Scintillation Counter

PSD : Position Sensitive Si Detector

MAPMT : Multi-Anode Photo-Multiplier Tube RadiatorMAPMT

Page 28: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLVelocity Distribution by RICH

395MeV/u 405MeV/u

Velocity Distributions Observed by RICH for Si beam.Both results for 405MeV/u and 395MeV/u are shown.

Δβ / β~0.2%

Page 29: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLLiulin-4J

MDU MDU

XY-Theta Stage

10cm

30 - 70 MeV Proton Beam

Computer Controlled XZ Stage and Theta Stage

Beam Pipe

Beam Pipe

Page 30: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLLiulin-4J Calibration

0 1 2 3 4 5101

102

103

104

105

106

Deposited Energy in MeV

Num

ber

of E

vent

s

0 deg45 deg

60 deg

75 deg

° Experiment− Simulation

0 2000 4000 6000 8000 10000 120000

50

100

150

200

Estimated Deposited Energy in keV

AD

C C

hann

els

MDU-1MDU-2MDU-3MDU-4

Exposure Angle 0 deg 45 deg 60 deg

Alpha particles

Protons

Y=Xx0.0123

GEANT4

Page 31: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLHIMAC Exposures

0 50 100 150 200 2500

1000

2000

3000

4000

5000

6000

ADC Ch.

Num

ber o

f Eve

nts

MDU-1C(400)

Ne(400)

0 5000 10000 15000 200000

50

100

150

200

250

Deposited Energy (keV)AD

C C

h.

Y=Xx0.0123

Ne(400)

C(400)He

p

0 50 100 150 200 2500

500

1000

1500

2000

ADC Ch.

Num

ber

of E

vent

s

Ne(400MeV/u) Acryl 10mm, 0.75deg

Ne

CLi

Be BN

O

F

Page 32: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLDiamond Detector

• Artificial diamond detector is developed with collaboration with Kanagawa Univ., Japan.

• Diamond has characters which is radiation hardness, low noise and tissue equivalent.

• The energy resolution of diamond detector is corresponding to surface barrier silicon detector.

• Because of tissue equivalent, diamond detector will be used as radiation protection monitor.

Page 33: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLPhoswich Neutron Detector

Plastic Scintillator Liquid Organic Scintillator

Light Guide PMT

Neutrons

Protons

By Masashi Takada

Page 34: NIRS ISRL with Heavy Ion Beams › ENG › rd › 1ban › publication › ...NIRS ISRLIntercalibration of Space Radiation Monitors with Heavy Ion Beams InterComparison for Cosmic-ray

NIRS ISRLScintillation Fiber Detector

By Tatsumi Koi