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Phys. J. C (2022) 82:1019  \n[https://doi.org/10.1140/epjc/s10052-022-10883-z](https://doi.org/10.1140/epjc/s10052-022-10883-z)  \nSpecial Article-Tools for Experiment and Theory  \nThe ARTI framework: cosmic rays atmospheric background simulations  \nChristian Sarmiento-Cano 1,a, Mauricio Suárez-Durán2 ,3 ,b, Rolando Calderón-Ardila4 ,5 ,c, Adriana Vásquez-Ramírez 1,d, Andrei Jaimes-Motta 1,e, Luis A. Núñez 1,6 ,f, Sergio Dasso7 ,8 ,g, Iván Sidelnik9 , 10 ,h, Hernán Asorey4 , 11 , 12 ,i, For the LAGO Collaboration  \n1 Escuela de Física, Universidad Industrial de Santander, Carrera 27 calle 9 Ciudad Universitaria, Bucaramanga, Colombia  \n2 Université Libre de Bruxelles, Boulevard du Triomphe, ACC.2 1050 Bruxelles, Belgium  \n3 Departamento de Fisica y Geología, Universidad de Pamplona, Km 1 Vía Bucaramanga Ciudad Universitaria Pamplona-Norte de Santander, Pamplona, Colombia  \n4 Instituto de Tecnologías en Deteccióny Astropartículas (CNEA, CONICET, UNSAM), Comisión Nacional de Energía Atómica, Centro Atómico Constituyentes, Av. Gral Paz 1499,(1650) Villa Maipú, Argentina  \n5 Instituto Sábato, Comisión Nacional de Energía Atómica, Centro Atómico Constituyentes, Av. Gral Paz 1499,(1650) Villa Maipú, Argentina  \n6 Departamento de Física, Universidad de Los Andes, Núcleo Universitario Pedro Rincón Gutiérrez, La Hechicera, 5101 Mérida, Venezuela  \n7 Departamento de Ciencias de la Atmósfera y los Océanos-Grupo LAMP, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Intendente Güiraldes 2160, Pabellón cero-infinito, Ciudad Universitaria (C1428EGA), Buenos Aires, Argentina  \n8 Instituto de Astronomía y Física del Espacio-LAMP Group, Universidad de Buenos Aires Consejo Nacionall de Investigaciones Científicas y Técnicas, Intendente Güiraldes 2160, Pabellón Cero-Infinito, Ciudad Universitaria (C1428EGA), Buenos Aires, Argentina  \n9 Departamento de Física de Neutrones, Comisión Nacional de Energía Atómica, Centro Atómico Bariloche, Av. E Bustillo 9500,(8400) San Carlos de Bariloche, Argentina  \n10 Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Buenos Aires, Argentina  \n11 Departamento de Física Médica, Comisión Nacional de Energía Atómica, Centro Atómico Bariloche, Av. E Bustillo 9500,(8400) San Carlos de Bariloche, Argentina  \n12 Unidad de Informática Científica (temporal stay), CIEMAT, Av Complutense 40,(28040) Madrid, Spain  \nReceived: 8 December 2021 / Accepted: 7 October 2022 / Published online: 12 November 2022 © The Author(s) 2022  \nAbstract ARTIis a complete framework designed to simulate the signals produced by the secondary particles emerging from the interaction of single, multiple, and even from the complete flux of primary cosmic rays with the atmosphere. These signals are simulated for any particle detector located at any place (latitude, longitude and altitude), including the real-time atmospheric, geomagnetic and detector conditions. Formulated through a sequence of codes written in C++, For-  \nThe LAGO Collaboration, see the complete list of authors andinstitutions at [http://lagoproject.net/collab.html](http://lagoproject.net/collab.html).  \na  \nb  \nc  \nd  \ne-mail: [christian.sarmiento@correo.uis.edu.co](christian.sarmiento@correo.uis.edu.co)  \n[e-mail:](e-mail: mauricio.suarezduran@ulb.be)[ mauricio.suarezduran@ulb.be](e-mail: mauricio.suarezduran@ulb.be)  \ne-mail: [rolando.calderon@iteda.cnea.gov.ar](rolando.calderon@iteda.cnea.gov.ar)  \ne-mail: [adriana2168921@correo.uis.edu.co](adriana2168921@correo.uis.edu.co)  \n[e](e e-mail: mottandrei2@gmail.com)[ e-mail:](e e-mail: mottandrei2@gmail.com)[ mottandrei2@gmail.com](e e-mail: mottandrei2@gmail.com)  \nfe-mail: [lnunez@uis.edu.co](lnunez@uis.edu.co)  \ng  \nh  \ne-mail: [sdasso@at.fcen.uba.ar](sdasso@at.fcen.uba.ar)  \ne-mail: [sidelnik@cnea.gov.ar](sidelnik@cnea.gov.ar)  \n[i](i e-mail: hernan.asorey@iteda.cnea.gov.ar)[ e-mail:](i e-mail: hernan.asorey@iteda.cnea.gov.ar)[ hernan.asorey@iteda.cnea.gov.ar](i e-mail: hernan.asorey@iteda.cn","cbCaicKWxyX5hVWs","https://ap.wps.com/l/cbCaicKWxyX5hVWs","pdf",1978824,17,"English","# Abstract\n## Introduction","[{\"question\":\"What does the ARTI framework simulate?\",\"answer\":\"ARTI simulates signals produced by secondary particles generated when primary cosmic rays interact with the atmosphere, including the detector response under various conditions.\"},{\"question\":\"Can ARTI model detector setups at different geographic locations?\",\"answer\":\"Yes. ARTI simulates signals for any particle detector location defined by latitude, longitude, and altitude, incorporating real-time atmospheric and geomagnetic conditions.\"},{\"question\":\"How is ARTI structured in terms of simulation tools?\",\"answer\":\"ARTI integrates multiple simulation environments—specifically MagnetoCosmics, CORSIKA, and Geant4—to evaluate geomagnetic field effects, atmospheric showers, and detector responses.\"}]","The ARTI framework - cosmic rays atmospheric background simulations | PDF",43]