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DYASTIMA: Simulating Air Showers in the Atmosphere of a Planet

机译:Dodastima:在行星的气氛中模拟空气淋浴

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As primary cosmic rays interact with the upper layers of the atmosphere of a planet, air showers of secondary cosmic ray particles are created. The modelling of these secondary cascades is of great importance for Space Weather studies. DYnamic Atmospheric Shower Tracking Interactive Model Application-DYASTIMA is a Monte Carlo simulation of the cascades produced in the atmosphere of a planet due to cosmic ray propagation. It is a standalone software application, based on a very friendly graphical user interface (GUI) and is implemented in Geant4 by the Athens Cosmic Ray Group. In order to perform a simulation, the primary cosmic ray spectra, the solar activity, the characteristics of the planet, the composition of the planet's atmosphere as well as the atmospheric profile are taken into account. As a result, DYASTIMA output provides all the necessary information about the secondary particles. DYASTIMA simulations have been used successfully for the atmospheres of Earth and Venus. Moreover, DYASTIMA-R, which is an additional simulation integrated into DYASTIMA software, performs radiation dosimetry calculations in the different atmospheric layers. More specifically, DYASTIMA-R provides the dose rate and the equivalent dose rate for various flight scenarios during different solar activity conditions and Space Weather phenomena. The simulations are being validated according to the recommendations set forth in 1CRP 137 and ICRU 84 documents. These results are very useful for the aviation community for the determination of the biological effects of the ionizing space radiation on aircrews and passengers. The application of DYASTIMA and DYASTIMA-R on other planets can provide useful insights for the radiation accumulation of space crews during missions. It is foreseen that DYASTIMA will be provided through the European Space Agency Space Situational Awareness (ESA SSA) Space Radiation Expert Service Centre (http://swe.ssa.esa.int/space-radiation) as a federated product. Th
机译:由于初级宇宙射线与行星气氛的上层相互作用,产生次级宇宙射线颗粒的空气淋浴。这些二级瀑布的建模对于空间天气研究非常重要。动态大气淋浴跟踪交互式模型应用程序 - DODastima是由于宇宙射线繁殖引起的星球大气中产生的级联的蒙特卡罗模拟。基于非常友好的图形用户界面(GUI),它是一个独立的软件应用程序,并由雅典宇宙射线组在Geant4中实现。为了执行模拟,初级宇宙射线光谱,太阳能活动,行星的特性,地球的大气的组成以及大气剖面都被考虑在内。结果,Dodastima输出提供有关二次粒子的所有必要信息。 Dodastima模拟已成功用于地球和金星的大气。此外,Dodastima-R是集成到Dyastima软件中的额外模拟,在不同的大气层中进行辐射剂量测定计算。更具体地,Dodastima-R在不同的太阳能条件和空间天气现象期间提供了各种飞行情景的剂量率和等同剂量率。根据1CRP 137和ICRU 84文档中规定的建议进行验证。这些结果对于航空界非常有用,用于确定电离空间辐射对机组和乘客的生物效应。 Domastima和Dyastima-R在其他行星上的应用可以为在任务期间的空间船员的辐射积累提供有用的见解。预见到朝鲜航天局空间情境意识(ESA SSA)空间辐射专家服务中心(http://swe.ssa.esa.int/space-radiation)作为联合产品,将提供朝多案。钍

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