@article{oai:repo.qst.go.jp:00047677,
 author = {Berger, Thomas and Burmeister, Sonke and Matthia, Daniel and Przybyla, Bartos and Reitz, Gunthe and Bilski, Pawel and Hajek, Michael and Sihver, Lembit and Szabo, Julianna and Ambrozova, Iva and Vanhavere, Filip and Gaza, Ramona and Semones, Edward and Yukihara, Eduardo and Benton, Eric and Uchihori, Yukio and Kodaira, Satoshi and Kitamura, HIsashi and Boehme, Matthias and Ｂｅｒｇｅｒ Ｔｈｏｍａｓ and Ｂｕｒｍｅｉｓｔｅｒ Ｓｏｎｋｅ and Ｐｒｚｙｂｙｌａ Ｂａｒｔｏｓ and Ｒｅｉｔｚ Ｇｕｎｔｈｅｒ and Ｂｉｌｓｋｉ Ｐａｗｅｌ and Ｈａｊｅｋ Ｍｉｃｈａｅｌ and Ｓｉｈｖｅｒ Ｌｅｍｂｉｔ and イバ アンブロツォヴァ and Ｖａｎｇａｖｅｒｅ Ｆｉｌｉｐ and Ｓｅｍｏｎｅｓ Ｅｄｗａｒｄ and Ｙｕｋｉｈａｒａ Ｅｄｕａｒｄｏ and Ｂｅｎｔｏｎ Ｅｒｉｃ and 内堀 幸夫 and 小平 聡 and 北村 尚},
 journal = {Journal of Space Weather and Space Climate},
 month = {Mar},
 note = {The natural radiation environment in Low Earth Orbit (LEO) differs significantly in composition and energy from that found on Earth. The space radiation field consists of high energetic protons and heavier ions from Galactic Cosmic Radiation (GCR), as well as of protons and electrons trapped in the Earth’s radiation belts (Van Allen belts). Protons and some heavier particles ejected in occasional Solar Particle Events (SPEs) might in addition contribute to the radiation exposure in LEO. All sources of radiation are modulated by the solar cycle. During solar maximum conditions SPEs occur more frequently with higher particle intensities. Since the radiation exposure in LEO exceeds exposure limits for radiation workers on Earth, the radiation exposure in space has been recognized as a main health concern for humans in space missions from the beginning of the space age on. Monitoring of the radiation environment is therefore an inevitable task in human spaceflight. Since mission profiles are always different and each spacecraft provides different shielding distributions, modifying the radiation environment measurements needs to be done for each mission. The experiments “Dose Distribution within the ISS (DOSIS)” (2009–2011) and “Dose Distribution within the ISS 3D (DOSIS 3D)” (2012–onwards) onboard the Columbus Laboratory of the International Space Station (ISS) use a detector suite consisting of two silicon detector telescopes (DOSimetry TELescope = DOSTEL) and passive radiation detector packages (PDP) and are designed for the determination of the temporal and spatial variation of the radiation environment. With the DOSTEL instruments’ changes of the radiation composition and the related exposure levels in dependence of the solar cycle, the altitude of the ISS and the influence of attitude changes of the ISS during Space Shuttle dockings inside the Columbus Laboratory have been monitored. The absorbed doses measured at the end of May 2016 reached up to 286 μGy/day with dose equivalent values of 647 μSv/day.},
 pages = {A8-1--A8-19},
 title = {DOSIS & DOSIS 3D: radiation measurements with the DOSTEL instruments onboard the Columbus Laboratory of the ISS in the years 2009–2016},
 volume = {7},
 year = {2017}
}