title={The energetic particle detector-energetic particle instrument suite for the solar orbiter mission},
author={Rodr{\'\i}guez-Pacheco, J and Wimmer-Schweingruber, RF and Mason, GM and Ho, GC and S{\'a}nchez-Prieto, S and Prieto, M and Mart{\'\i}n, C and Seifert, H and Andrews, GB and Kulkarni, SR and others},
journal={Astronomy \& Astrophysics},
volume={642},
pages={A7},
year={2020},
publisher={EDP Sciences}
}
@book{knoll2000radiation,
title={Radiation detection and measurement},
author={Knoll, Glenn F},
year={2000},
publisher={John Wiley \& Sons}
}
@phdthesis{elftmann2020high,
title={The High Energy Telescope on Solar Orbiter: Development and Validation of the Onboard Data Processing},
author={Elftmann, Robert},
year={2020},
school={Kiel University}
}
@book{longair2011high,
title={High energy astrophysics},
author={Longair, Malcolm S},
year={2011},
publisher={Cambridge university press}
}
@book{grupen2018einstieg,
title={Einstieg in die Astroteilchenphysik: Grundlagen, Messungen und Ergebnisse aktueller Forschung},
author={Grupen, Claus},
year={2017},
publisher={Springer-Verlag}
}
@misc{kolanoskiSkript,
title={Einf{\"u}hrung in die Astroteilchenphysik},
title={The Regener-Pfotzer Maximum during a Total Solar Eclipse},
author={McIntosh, Gordon and Swanson, Alaina and Taylor, Liam and Agrimson, Erick Paul and Smith, Kaye and Xiong, Alynie},
journal={Journal of High Altitude Ballooning},
volume={1},
number={1},
year={2021},
publisher={Iowa State University Digital Press}
}
@article{kunow1988costep,
title={COSTEP: a comprehensive suprathermal and energetic particle analyzer for SOHO},
author={Kunow, Horst and Fischer, Harald and Green, Guenter and Mueller-Mellin, Reinhold and Wibberenz, Gerd and Holweger, Hartmut and Evenson, Paul and Meyer, Jean-Paul and Hasebe, Nabuyuki and Vonrosenvinge, Tycho},
journal={ESA, the SOHO mission. Scientific and technical aspects of the instruments},
year={1988}
}
@Inbook{Zilles2017,
author="Zilles, Anne",
title="Introduction to Cosmic Rays and Extensive Air Showers ",
bookTitle="Emission of Radio Waves in Particle Showers: Validation of Microscopic Simulations with the SLAC T-510 Experiment and their Potential in the Future Square Kilometre Array",
year="2017",
publisher="Springer International Publishing",
address="Cham",
pages="1--13",
abstract="Cosmic rays are highly energetic particles from the outer space, hitting the Earth's atmosphere every day.",
isbn="978-3-319-63411-1",
doi="10.1007/978-3-319-63411-1_1",
url="https://doi.org/10.1007/978-3-319-63411-1_1"
}
@Inbook{Simpson1983,
author="Simpson, J. A.",
title="Introduction to the Galactic Cosmic Radiation",
bookTitle="Composition and Origin of Cosmic Rays",
year="1983",
publisher="Springer Netherlands",
address="Dordrecht",
pages="1--24",
abstract="Although the astrophysical sites for the cosmic radiations and their acceleration mechanisms are still not firmly established, this radiation has turned out to be a vital contributor to our understanding of high energy phenomena in our galaxy. For example, the cosmic rays constitute approximately one-third of the energy density of the interstellar medium and, on a galactic scale, they form a relativistic gas whose pressure is important to take into account in the dynamics of galactic magnetic fields. The electronic component is a source of bremsstrahlung and synchrotron radiation which reveals the configurations and intensities of large scale galactic and stellar magnetic fields. The cosmic ray nuclei are the only direct and measurable sample of matter from outside the solar system. It is a unique sample since it includes all of the elements from Hydrogen up to the actinides. The isotopic abundances and elemental abundances of these nuclei convey not only the ``imprint'' of their nucleosynthesis origins at astrophysical sites in the galaxy, but also, through their radioactive species, reveal the time required for their acceleration and the history of their propagation in interstellar magnetic fields.",
isbn="978-94-009-7166-0",
doi="10.1007/978-94-009-7166-0_1",
url="https://doi.org/10.1007/978-94-009-7166-0_1"
}
@phdthesis{bornfleth2023,
author = {Pierre Bornfleth},
title = {Simulation von Chaosjr mit Geant4},
school = {Christian-Albrechts-Universität zu Kiel},
abstract = {Geant4 is a toolkit for simulating the passage of particles through matter. It includes a complete range of functionality including tracking, geometry, physics models and hits. The physics processes offered cover a comprehensive range, including electromagnetic, hadronic and optical processes, a large set of long-lived particles, materials and elements, over a wide energy range starting, in some cases, from 250eV and extending in others to the TeV energy range. It has been designed and constructed to expose the physics models utilised, to handle complex geometries, and to enable its easy adaptation for optimal use in different sets of applications. The toolkit is the result of a worldwide collaboration of physicists and software engineers. It has been created exploiting software engineering and object-oriented technology and implemented in the C++ programming language. It has been used in applications in particle physics, nuclear physics, accelerator design, space engineering and medical physics.}
author = {Z.-N. Shen and G. Qin and Pingbing Zuo and Fengsi Wei},
title = {Modulation of Galactic Cosmic Rays from Helium to Nickel in the Inner Heliosphere},
journal = {The Astrophysical Journal},
abstract = {Galactic cosmic-ray (GCR) helium and heavier ions are important sources of space radiation, and their elemental spectra and composition can help us better understand the transport in both the galaxy and the heliosphere. A model based on the numerical solution of Parker’s transport equation is used to study the modulation of GCR helium and heavier ions in the inner heliosphere. The model incorporates a modified Parker heliospheric magnetic field, time-dependent diffusion and drift model, time-delayed heliosphere, and randomly determined solar magnetic polarity during solar maximum. We set the outer boundary of modulation at 85 au, and the reference unmodulated GCR energy spectra for GCR helium and heavier ions, which are assumed to have a general form, are determined by fitting the numerical results to the selected GCR measurements, e.g., BESS, ACE/CRIS, HEAO-3-C2, etc. In addition, we use the Sun’s polar magnetic field data from NSO/NISP to determine the possibility of A > 0 during the recent solar maximum, and it gives an improved numerical result during the period 2013–2015. Finally, the fitted unmodulated GCR energy spectra are used to study the long-term modulation of GCRs of helium and heavier ions, and the computed results show good agreement with various GCR measurements.}
}
@article{vaisanen2023revised,
title={Revised reconstruction of the heliospheric modulation potential for 1964--2022},
author={V{\"a}is{\"a}nen, Pauli and Usoskin, Ilya and K{\"a}hk{\"o}nen, Riikka and Koldobskiy, Sergey and Mursula, Kalevi},
journal={Journal of Geophysical Research: Space Physics},
author={Domingo, V and Fleck, B and Poland, Arthur I},
journal={Solar Physics},
volume={162},
pages={1--37},
year={1995},
publisher={Springer}
}
@article{abe2016measurements,
title={Measurements of cosmic-ray proton and helium spectra from the BESS-Polar long-duration balloon flights over Antarctica},
author={Abe, Koh and Fuke, Hideyuki and Haino, Sadakazu and Hams, T and Hasegawa, M and Horikoshi, A and Itazaki, A and Kim, KC and Kumazawa, Teruyuki and Kusumoto, A and others},
journal={The Astrophysical Journal},
volume={822},
number={2},
pages={65},
year={2016},
publisher={IOP Publishing}
}
@misc{usoskin2023,
title={Cosmic ray modulation potential (Phi) reconstructed from ground-based neutron-monitor data.},
abstract = {This study presents the development of large-area (18cm×18cm×2cm), high refractive index (n∼1.05) hydrophobic silica aerogel tiles for use as Cherenkov radiators. These transparent aerogel tiles will be installed in a Cherenkov detector for the next-generation accelerator-based particle physics experiment Belle II, to be performed at the High Energy Accelerator Research Organization (KEK) in Japan. Cracking has been eliminated from the prototype aerogel tiles by improving the supercritical carbon dioxide (scCO2) extraction procedure when drying the wet gel tiles. Finally, a method of mass-producing aerogel tiles for the actual detector was established. It was confirmed that the experimentally manufactured aerogel tiles meet the required optical and hydrophobic characteristics and have a uniform tile density.}
title={Latitudinal effect on the position of Regener--Pfotzer maximum investigated by balloon flight HEMERA 2019 in Sweden and balloon flights FIK in Czechia},
author={Ambro{\v{z}}ov{\'a}, Iva and K{\'a}kona, Martin and Dvo{\v{r}}{\'a}k, Roman and K{\'a}kona, Jakub and Lu{\v{z}}ov{\'a}, Martina and Povi{\v{s}}er, Martin and Sommer, Marek and Velychko, Olena and Ploc, Ond{\v{r}}ej},
journal={Radiation Protection Dosimetry},
volume={199},
number={15-16},
pages={2041--2046},
year={2023},
publisher={Oxford University Press}
}
@phdthesis{doensdorf2014phd,
title={Development of a Phoswich Detector for Neutron Dose Rate Measurements in the Earth's Atmosphere},
author={D\"onsdorf, Esther Miriam},
year={2014},
school={Kiel University}
}
@phdthesis{moeller2013phd,
title={Measurement of the Radiation Exposure for High Altitude Flights in the Polar Region},
