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Near space radiation dosimetry in Australian outback using a balloon borne energy compensated PIN diode detector
Institution:1. School of Physics (A28), The University of Sydney, NSW 2006, Australia;2. Detector and Sensor Group, West German Proton Therapy Centre Essen (WPE), Hufeland Strasse 55, 45147 Essen, Germany;3. School of Aerospace, Mechanical and Mechatronics Engineering, The University of Sydney, NSW 2006, Australia;4. Helmholtz Zentrum München, Institute of Radiation Protection, Ingolstädter Landstraße 1, 85758 Neuherberg, Germany;1. Department of Surgery, Duke University Medical Center, Durham, North Carolina;2. Department of Medicine, Duke University Medical Center, Durham, North Carolina;1. Centre de Recherche en Astronomie, Astrophysique et Géophysique, BP 63 Bouzareah, 16340 Algiers, Algeria;2. Sorbonne Université, Paris VI, UPMC, LPP 5 Place Jussieu, 75005 Paris, France;3. T/ICT4D, The Abdus Salam International Centre for Theoretical Physics, Trieste, Italy;4. Université des Sciences et de la Technologie, Alger, BP 32 El-Alia, Bab-Ezzouar, 16111 Algiers, Algeria;5. Institute for Scientific Research, Boston College, Boston, USA;1. IRAP/UPS/CNRS, 9 av. Colonel Roche, 31400 Toulouse, France;2. LESIA, Observatoire de Paris, 5, place Jules Janssen, 92195 Meudon, France;3. Noveltis, 153 Allée du Lac, 31670 Labège, France;4. CNES, 18 av. Edouard Belin, 31400 Toulouse, France;5. ONERA, 2 av. Edouard Belin, 31400 Toulouse, France;6. LATMOS/CNRS/UVSQ, 11 blvd d’Alembert, 78280 Guyancourt, France;7. AKKA, 6 rue Roger Camboulives, 31100 Toulouse, France;8. GFI, 1 av. général Eisenhower, 31100 Toulouse, France;1. Georgia State University, Department of Computer Science, United States;2. Montana State University, Department of Computer Science, United States;1. Physics Department, Faculty of Arts and Sciences, Uludag University, Gorukle Campus, 16059, Bursa, Turkey;2. Physics Department, Faculty of Arts and Sciences, Bitlis Eren University, 13000 Bitlis, Turkey
Abstract:This paper reports the near space ballooning experiment carried out at Australian outback town West Wyalong (33°51′S, 147°24′E) on 19 July 2015. Several dedicated electronic detectors including digital temperature and acceleration (vibration) sensors and an energy compensated PIN-diode gamma ray dosimeter were installed in a thermally insulated Styrofoam payload box. A 9 V Lithium-Polymer battery powered all the devices. The payload box was attached to a helium-filled latex weather balloon and set afloat. The balloon reached a peak burst altitude of 30 km and then soft-landed aided by a self-deploying parachute 66.2 km away form the launch site. The payload box was retrieved and data collected from the electronic sensors analysed. The integrated cosmic ray induced photon ambient dose equivalent recorded by the PIN diode detector was evaluated to be 0.36 ± 0.05 μSv. Furthermore, a high-altitude extended version of commercially available aviation dosimetry package EPCARD.Net (European Program package for the Calculation of Aviation Route Doses) was used to calculate the ambient dose equivalents during the balloon flight. The radiation environment originated from the secondary cosmic ray shower is composed of neutrons, protons, electrons, muons, pions and photons. The photon ambient dose equivalent estimated by the EPCARD.Net code found to be 0.47 ± 0.09 μSv. The important aspects of balloon based near-space radiation dosimetry are highlighted in this paper.
Keywords:Australian outback  Cosmic ray shower  EPCARD  Net  High-altitude balloon mission  Pfotzer-Maximum  PIN-diode dosimeter
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