Characterization and Directional Visualization of Space Radiation Quanta in Low Earth Orbit with the compact Spacecraft Payload SATRAM

Similar documents
Study of the radiation fields in LEO with the Timepix detector

MIRAM Miniaturized Radiation Monitor

Advacam, Prague, Czech Republic. Nuclear Physics Institute, Czech Academy of Sciences, Prague, Czech Republic

Measurement of the Ionizing Energy Depositions after Fast Neutron Interactions in Silicon

Detection of X-ray spectra and images by Timepix

Energy calibration of the threshold of Medipix for ATLAS

Scientific astrophysical payloads for pico and nano-satellites

Abstract: J. Urbar [1], J. Scheirich [2], J. Jakubek [3] MEDIPIX CR tracking device flown on ESA BEXUS-7 stratospheric balloon flight

Analysis of Carbon Ion Fragmentation and Angular Fragment Distributions using a flexible set-up

Hard X-ray Vela supernova observation on rocket experiment WRX-R

COMMISSIONING TESTS OF THE NEW NEUTRON RADIOGRAPHY FACILITY AT THE LVR-15 REACTOR ABSTRACT

Mass Determination of Rn and Hg isotopes using MASHA

The Silicon-Tungsten Tracker of the DAMPE Mission

Design, Fabrication and Performance of the Silicon Charge Detector for the ISS-CREAM

analysing data from the LUCID experiment

Characterization of 3D thermal neutron semiconductor detectors

TIMEPIX3 First measurements and characterization of a hybrid pixel detector working in event driven mode

Integral in Orbit* The Integral satellite was launched on 17 October 2002, at

DOUBLE BETA DECAY OF 106 Cd - EXPERIMENT TGV (Telescope Germanium Vertical) EXPERIMENT SPT (Silicon Pixel Telescope)

M. Martišíková 1,3, C. Granja 2, J. Jakůbek 2, B. Hartmann 1,3, K. Gwosch 1, P. Soukup 2 and O. Jäkel 1,3,5

SYNTHESIS OF SUPERHEAVY ELEMENTS USING THE MASS SPECTROMETER MASHA

Tritel: 3D Silicon Detector Telescope used for Space Dosimetry. Tamás Pázmándi, Attila Hirn, Sándor Deme, István Apáthy, Antal Csőke, *László Bodnár

The NUCLEON Space Experiment Preliminary Results. Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, , Russia

Development of a Silicon PIN Diode X-Ray Detector

PROBA 1. F. Teston ESA/ESTEC D/TEC-EL

CMOS Pixel Sensor for a Space Radiation Monitor with very low cost, power and mass. Outline:

Monitoring solar energetic particles with ESA SREM units

CZENDA the Czech Experimental Novel Dosimetry Assembly aboard the BION-M2 Russian satellite

PoS(Vertex 2016)004. ATLAS IBL operational experience

Special SLS Symposium on Detectors

Your Partner in Environment Monitoring

PoS(HQL 2012)021. The LHCb upgrade. Tomasz Szumlak 1

Identifying Particle Trajectories in CMS using the Long Barrel Geometry

Radiation Environments, Effects and Needs for ESA Missions

SEP Protons in GEO with the ESA MultiFunctional Spectrometer

Characterization of the 3 MeV Neutron Field for the Monoenergetic Fast Neutron Fluence Standard at the National Metrology Institute of Japan

CRaTER Science Requirements

Update on Calibration Studies of the Canadian High-Energy Neutron Spectrometry System (CHENSS)

Analysis distribution of galactic cosmic rays particle energy with polar orbit satellite for Geant4 application

Light ion recoil detector

The Cosmic Ray Telescope for the Effects of Radiation (CRaTER) Investigation for the Lunar Reconnaissance Orbiter

PoS(TIPP2014)033. Upgrade of MEG Liquid Xenon Calorimeter. Ryu SAWADA. ICEPP, the University of Tokyo

Fast-Neutron Production via Break-Up of Deuterons and Fast-Neutron Dosimetry

An InGrid based Low Energy X-ray Detector for the CAST Experiment

Overview of the ISS radiation environment observed during EXPOSE- R2 mission in

Solar particle events contribution in the space radiation exposure on electronic equipment

NGRM Next Generation Radiation Monitor new standard instrument for ESA

PoS(PD07)020. Timing Properties of MCP-PMT. Kenji Inami. Nagoya university, Nagoya, Japan

Time variations of proton flux in the Earth inner radiation belt for years based on the PAMELA and the ARINA data

Background optimization for a new spherical gas detector for very light WIMP detection

Results from Silicon Photo-Multiplier neutron irradiation test

Dark Matter Particle Explorer: The First Chinese Cosmic Ray and Hard γ-ray Detector in Space

Thesis and PhD themes

XMASS 1.5, the next step of the XMASS experiment

Non-collision Background Monitoring Using the Semi-Conductor Tracker of ATLAS at LHC

Soft error rate estimations of the Kintex-7 FPGA within the ATLAS Liquid Argon (LAr) Calorimeter

CCD readout of GEM-based neutron detectors

LASER-COMPTON SCATTERING AS A POTENTIAL BRIGHT X-RAY SOURCE

The PAMELA Satellite Experiment: An Observatory in Space for Particles, Antiparticles and Nuclei in the Cosmic Rays

Estec final presentation days 2018

PoS(Baldin ISHEPP XXII)065

New irradiation zones at the CERN-PS

Solar Energetic Particles measured by AMS-02

on behalf of CAST Collaboration

Simulation of Radiation Monitors for Future Space Missions

SREM: 8 years experience of radiation monitoring with a standard instrument

CRaTER Pre-Environmental Review (I-PER) Science Requirements Update

Radiation Transport Tools for Space Applications: A Review

PoS(idm2008)010. The PICASSO Dark Matter Search Project. A. Davour for the PICASSO collaboration Queen s University

Letter to the Editor. Astronomy. Astrophysics. Radiation environment along the INTEGRAL orbit measured with the IREM monitor

Geant4 simulation of SOI microdosimetry for radiation protection in space and aviation environments

Portable, Low-cost Proportional Counters for Space, Atmospheric and Ground based Applications

Comparison of the Photo-peak Efficiencies between the Experimental Data of 137 Cs Radioactive Source with Monte Carlo (MC) Simulation Data

Investigation of nuclear Equation of State (EoS) is an attractive subject not only for nuclear

Capabilities and Performance of the High-Energy Energetic-Particles Instrument for the Parker Solar Probe Mission

Update on the In-orbit Performances of GIOVE Clocks

The Compact Muon Solenoid Experiment. Conference Report. Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland

Development of High-Z Semiconductor Detectors and Their Applications to X-ray/gamma-ray Astronomy

Measurement of nuclear recoil responses of NaI(Tl) crystal for dark matter search

Alignment of the ATLAS Inner Detector tracking system

Recent Activities on Neutron Standardization at the Electrotechnical Laboratory

Development of a Radiation Hard CMOS Monolithic Pixel Sensor

A Study On Radioactive Source Imaging By Using A Pixelated CdTe Radiation Detector

Timepix pixel detectors

Simultaneous Investigation of Galactic Cosmic Rays on Aircrafts and on International Space Station

THE MICRO ADVANCED STELLAR COMPASS FOR ESA S PROBA 2 MISSION

MONTE-CARLO SIMULATIONS OF TIME- RESOLVED, OPTICAL READOUT DETECTOR for PULSED, FAST-NEUTRON TRANSMISSION SPECTROSCOPY (PFNTS)

Measurement of Tritium in Helium

DARWIN: dark matter WIMP search with noble liquids

Study of Edgeless TimePix Pixel Devices. Dylan Hsu Syracuse University 4/30/2014

Bubble Chambers for Direct Dark Matter Searches in COUPP

A Survey of Spacecraft Charging Events on the DMSP Spacecraft in LEO

Energy response for high-energy neutrons of multi-functional electronic personal dosemeter

PoS(ICRC2015)641. Cloud Monitoring using Nitrogen Laser for LHAASO Experiment. Z.D. Sun 1,Y. Zhang 2,F.R. Zhu 1 for the LHAASO Collaboration

RADIATION DAMAGE IN HST DETECTORS

Presentation by Indian Delegation. to 49 th STSC UNCOPUOS. February 2012 Vienna

Performance of high pressure Xe/TMA in GEMs for neutron and X-ray detection

November 2013 analysis of high energy electrons on the Japan Experimental Module (JEM: Kibo)

H. Koshiishi, H. Matsumoto, A. Chishiki, T. Goka, and T. Omodaka. Japan Aerospace Exploration Agency

1. Motivation & Detector concept 2. Performance 3. Applications 4. Summary

Transcription:

Characterization and Directional Visualization of Space Radiation Quanta in Low Earth Orbit with the compact Spacecraft Payload SATRAM 1, Stepan Polansky, Stanislav Pospisil, Zdenek Vykydal, Daniel Turecek Institute of Experimental and Applied Physics (IEAP), Czech Technical University in Prague (CTU) Horska 3a/22, 128 00 Prague 2, Czech Republic E-mail: carlos.granja@utef.cvut.cz Alan Owens, Karim Mellab, Petteri Nieminen European Space Research & Technology Centre (ESTEC), European Space Agency (ESA) Postbus 299, NL-2200 AG Noordwijk, The Netherlands Zdenek Dvorak, Marek Simcak, Zdenek Kozacek #, Petr Vana #, Jan Mares # Czech Space Research Center (CSRC) Janska 12, 602 00 Brno, Czech Republic In this contribution the response of the SATRAM/Timepix spacecraft payload to space radiation in Low Earth Orbit in the form of full Timepix frames along a single satellite orbit is presented. The compact light weight SATRAM payload has been operating in open space onboard ESA s Proba-V satellite in low Earth orbit since 7 th May 2013. The embedded Timepix chip can determine the composition and spectral characteristics of ionizing radiation in the satellite environment together with visualization of single particle tracks. The device provides single quantum X-ray photon and charged particle counting for high sensitivity detection, high resolution tracking and directional visualization of energetic charged particles over a wide dynamic range of particle fluxes, energies and broad field of view. In addition to the visualization of the varying radiation environment along a single satellite orbit also preliminary evaluated results in the form of total particle flux maps (navigation correlated spatial and time distributions) along the satellite orbit for a period of 19 days in October 2014 are included. The 23rd International Workshop on Vertex Detectors 15-19 September 2014 Macha Lake, The Czech Republic 1 Speaker; # former staff Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. http://pos.sissa.it

1. Introduction The Space Application of Timepix Radiation Monitor (SATRAM) is a compact low-mass and low-power spacecraft payload operating in open space on board in the ESA s Proba-V satellite [1]. Launched on 7 th May 2013, the satellite is deployed in Low Earth Orbit (LEO) at an altitude 820 km (sun synchronous polar orbit tilted at 98.8º). SATRAM provides highsensitivity wide-dynamic range radiation monitoring enhanced with particle track visualization of the charged events and low-energy X-ray field along the satellite orbit. The Timepix detector [2] determines over a wide range of particle fluxes, energies and broad field of view [3] the composition (particle species) and spectral characterization (de/dx) of the mixed field radiation environment [4]. The per-pixel energy sensitivity provides linear energy transfer (LET) spectra with enhanced particle-type resolving power and directional sensitivity for energetic charged particles. Results include spatial- and time-dependent distributions of the radiation environment along the satellite orbit. The motivation for this work and a more detailed description of the payload instrument (design, operation, response) have been presented [5] where preliminary results in the form spatial Earth maps of total radiation dose rate were included. In this contribution a short description of the core detector technology (Timepix chip) and of the spacecraft payload (SATRAM) is given. Results presented are in the form of visualization of the mixed radiation field in the environment of the satellite along a single orbit showing the full frames of the embedded Timepix detector at selected navigation stamps. In addition, the preliminary maps (spatial, time distributions) of total particle flux measured along the satellite orbit for a period of 19 days collected in October 2014 are included. 2. The hybrid semiconductor pixel detector Timepix The position-sensitive semiconductor detectors of the Medipix family [2,6], developed in frame of the MEDIPIX Collaboration provide high sensitivity (single-particle/quantum counting), wide-dynamic range, high spatial resolution and noiseless (dark-current free) detection. The hybrid architecture enables using sensors of defined media (e.g., Si, CdTe, GaAs) and thicknesses (e.g., 300 um, 700 um, 1000 and 1500 um). The detector consists of a matrix of 256 256 (total of 65.536) pixels, pixel pitch size 55 µm and full sensitive area 14 mm 14 mm (1.98 cm 2 ) see Fig. 1. Based on the Medipix2 [6] device, Timepix [2] provides extended functionality at the level of the per-pixel integrated electronic chain. Each pixel of the Timepix detector can be independently configured to operate in counting mode (the counter is incremented by one when the per-pixel deposited energy of the interacting particle crosses a threshold level), energy mode (called Time-over-Threshold (ToT) mode where the counter is incremented continuously as long as the signal is above threshold) and Time mode (called Time-of-Arrival (ToA) mode where the counter is incremented continuously from the time the first hit arrives until the closure of the shutter or end of the time window or acquisition exposure). Equipped with a 300 µm thick silicon sensor, Timepix is sensitive to X-rays (highest efficiency in the range 5 25 kev) and charged particles (100% detection efficiency) with a detection threshold of 4 kev. 2

Fig. 1: Illustration (a) at the pixel scale (pixel pitch size 55 µm) of (b) the Timepix detector consisting of a semiconductor sensor (silicon with thickness 300 µm) bump bonded to the integrated ASIC readout chip of 256 256 pixels (total 65.356 channels). Full detector size (c): 14 mm 14 mm. 3. Timepix/SATRAM spacecraft payload The Space Application of Timepix based Radiation Monitor (SATRAM) is a technology demonstration payload as a spacecraft platform device on-board ESA s Proba V satellite which was launch on 7 th May 2013. The payload contains an FPGA controlling the Timepix detector and provides communication with the spacecraft, along with housekeeping, data compression and configuration. Including the Aluminum alloy compartment the payload has dimensions 108 mm 63 mm 56 mm (see Fig. 2) and total weight 380 g including the shielding box. Fig. 2: SATRAM payload (a) attached to ESA s Proba-V satellite (b) prior launch by ESA s Vega-2 rocket. For comparison, Proba-V satellite size: 80 cm 80 cm 100 cm and mass: 138 kg. The plastic side panels with handles are protective covers which were removed before flight. The entrance window in front of the Timepix chip is of 0.5 mm thick Al. The payload features 28 V voltage input and power consumption 3 W. The energy calibration of the Timepix detector was performed with X-ray and alpha particle radioactive sources. Tests and detector response characterization were done also with a radionuclide neutron source (AmBe) and low- 3

energy light ion (proton, deuterium and alpha particle) beams and mono-energetic fast neutron sources from the Van de Graaff accelerator at the IEAP CTU in Prague. 4. Detection and track visualization of space radiation in open space The detection and visualization of space radiation in the form of individual Timepix frames of the radiation environment along the Proba-V satellite orbit are shown in Figs 3-7. The perpixel energy measured is displayed in color in log scale. The frames displayed are labelled according to navigation stamp (geographical position and time) as indicated in Fig. 8. The varying acquisition time of the collected frames (indicated in Figs 3-7) is taken into account in deriving the corresponding particle fluxes (see Sec. 5) as shown in Fig. 8 and Fig. 9. Particle species are distinguished into main types such as light and heavy charged particles. For energetic charged particles also direction is registered (detailed analysis is in progress). 5. Particle flux along the satellite orbit SATRAM can continuously sample the radiation field along the satellite path as shown in Fig. 8 and Fig. 9 where the measured total particle flux is displayed for one orbit (100 minutes) and 19 days (period 1-19 Oct. 2014), respectively. The correlated spatial and time distributions are shown in log scale. The presented quantity (particle flux) varies up to six orders of magnitude over the high intensity radiation regions (regions near the poles and the South Atlantic Anomaly SAA). 6. Conclusions SATRAM is the first deployment of the Timepix detector in open space. The spacecraft payload has been successfully commissioned. Detailed data analysis is in progress. The response and track visualization of the varying radiation environment along a single orbit have been presented. The response of the payload with the embedded Timepix detector enables distinguishing the main particle type components present in the radiation environment observed (X-rays, light charged particles and heavy charged particles). Preliminary results have been presented in the form of detection and track visualization of single particles as well as qualitative characterization of the mixed radiation field in the open space environment. Further characterization of the radiation field includes analysis of angle of incidence (for energetic charged particles) and stopping power. Evaluated results include high sensitivity quantum imaging radiation dosimetry and integrated dose rate maps along the satellite orbit. Currently detailed data analysis is in progress including quantitative and time-dependent results on radiation particle composition, particle component fluxes and directional distributions for energetic charged particles. This work extends the use of Timepix into open space started from ground-based [3] and atmospheric/aerospace [7] applications. 4

Fig. 3: Quantum imaging detection of space radiation by Timepix/SATRAM payload for selected frames (see labels in Fig. 8 showing the corresponding navigation stamp). Data displayed in Timepix s Timeover-threshold (ToT) mode (per-pixel energy displayed in log scale) with varying acquisition time as indicated. Only part of the sensor matrix (200 200 pixels) is displayed (11 mm 11 mm = 1.21 cm 2 ). 5

Fig. 4: Same as Fig. 3 continuation. 6

Fig. 5: Same as Fig. 3 continuation. 7

Fig. 6: Same as Fig. 3 continuation. 8

Fig. 7: Same as Fig. 3 continuation. 9

Fig. 8: Flux of all particles registered by SATRAM/Timepix along one orbit of the Proba-V satellite (100 minutes in the period 00:00 thru 01:40 h on 19 th Oct 2014). The spatial (top) and time (bottom) distributions are displayed in log scale. Selected frames (see labels) are displayed in Figs. 3-7. Acknowledgments Research performed in frame of the CERN Medipix Collaboration. Project funded by the European Space Agency, Grant No. 4000105089/11/NL/CBi (641-120004M). Testing and calibration verification measurements of Timepix chips were performed at the Van de Graaff light ion accelerator of the IEAP CTU in Prague in frame of the MSMT Grant Research Infrastructure No. LM2011030 of the Ministry of Education, Youth and Sports of the Czech Republic. The cooperation with Qinetiq operating the Proba-V satellite is gratefully acknowledged. References [1] B. Sean, The mission of Proba-V, ESA Bulletin, European Space Agency 153 (2013) 10-21 (see http://esamultimedia.esa.int/docs/proba/bulletin_proba-v.pdf). [2] X. Llopart, M. Campbell, E. Heijne, et al., Timepix, a 65 k programmable pixel readout chip for arrival time, energy and/or photon counting measurements, Nucl. Instr. and Meth. in Phys. Res. A 581 (2007) 485-494. [3] E.H.M. Heijne, R. Ballabriga, M. Campbell, et al. Measuring radiation environment in LHC or anywhere else, on your computer screen with Medipix, Nucl. Instr. and Methods A 699 (2013) 198-204. [4] Z. Vykydal, J. Bouchami, M. Campbell, et al., The Medipix2-based network for measurement of spectral characteristics and composition of radiation in ATLAS detector, Nucl. Instr. Meth. Phys. Res. A 607 (2009) 35-37. 10

[5] C. Granja, S. Polansky, Z. Vykydal, et al., Directional Visualization of Space Radiation Quanta with Timepix/SATRAM Spacecraft Payload on board ESA Proba-V Satellite, Proc. of Science PoS (X LASNPA) 003 (2014). [6] X. Llopart, M. Campbell, R. Dinapoli, et al., Medipix2: a 65-k pixel readout chip with 55 um square elements working in single photon counting mode, IEEE Trans. Nucl. Sci. 49 (2002) 2279-2283. [7] C. Granja, S. Pospisil, Quantum dosimetry and online visualization of X-ray and charged particle radiation in aircraft at flight altitudes with the pixel detector Timepix, Adv. Space Res. 54 (2014) 241-251. 11

12 Fig. 9. Same as Fig. 8 for a 19 day period (1-19 Oct 2014). Particle flux displayed in color log scale. Visualization of Space Radiation with SATRAM/Timepix payload in Open Space