GRANDlib: A simulation pipeline for the Giant Radio Array for Neutrino Detection (GRAND)

Autor: GRAND Collaboration, Batista, Rafael Alves, Benoit-Lévy, Aurélien, Bister, Teresa, Bohacova, Martina, Bustamante, Mauricio, Carvalho, Washington, Chen, Yiren, Cheng, LingMei, Chiche, Simon, Colley, Jean-Marc, Correa, Pablo, Laurenciu, Nicoleta Cucu, Dai, Zigao, de Almeida, Rogerio M., de Errico, Beatriz, de Jong, Sijbrand, Neto, João R. T. de Mello, de Vries, Krijn D., Decoene, Valentin, Denton, Peter B., Duan, Bohao, Duan, Kaikai, Engel, Ralph, Erba, William, Fan, Yizhong, Ferrière, Arsène, Gou, QuanBu, Gu, Junhua, Guelfand, Marion, Guo, Jianhua, Guo, Yiqing, Guépin, Claire, Gülzow, Lukas, Haungs, Andreas, Havelka, Matej, He, Haoning, Hivon, Eric, Hu, Hongbo, Huang, Xiaoyuan, Huang, Yan, Huege, Tim, Jiang, Wen, Koirala, Ramesh, Kong, ChuiZheng, Kotera, Kumiko, Köhler, Jelena, Lago, Bruno L., Lai, Zhisen, Coz, Sandra Le, Legrand, François, Leisos, Antonios, Li, Rui, Li, Xingyu, Li, YiFei, Liu, Cheng, Liu, Ruoyu, Liu, Wei, Ma, Pengxiong, Macias, Oscar, Magnard, Frédéric, Marcowith, Alexandre, Martineau-Huynh, Olivier, McKinley, Thomas, Minodier, Paul, Mitra, Pragati, Mostafá, Miguel, Murase, Kohta, Niess, Valentin, Nonis, Stavros, Ogio, Shoichi, Oikonomou, Foteini, Pan, Hongwei, Papageorgiou, Konstantinos, Pierog, Tanguy, Piotrowski, Lech Wiktor, Prunet, Simon, Qian, Xiangli, Roth, Markus, Sako, Takashi, Schoorlemmer, Harm, Szálas-Motesiczky, Dániel, Sławiński, Szymon, Tian, Xishui, Timmermans, Anne, Timmermans, Charles, Tobiska, Petr, Tsirigotis, Apostolos, Tueros, Matías, Vittakis, George, Wang, Hanrui, Wang, Jiale, Wang, Shen, Wang, Xiangyu, Wang, Xu, Wei, Daming, Wei, Feng, Wu, Xiangping, Wu, Xuefeng, Xu, Xin, Xu, Xing, Yang, Fufu, Yang, Lili, Yang, Xuan, Yuan, Qiang, Zarka, Philippe, Zeng, Houdun, Zhang, Chao, Zhang, Jianli, Zhang, Kewen, Zhang, Pengfei, Zhang, Qingchi, Zhang, Songbo, Zhang, Yi, Zhou, Hao

The operation of upcoming ultra-high-energy cosmic-ray, gamma-ray, and neutrino radio-detection experiments, like the Giant Radio Array for Neutrino Detection (GRAND), poses significant computational challenges involving the production of numerous si

Externí odkaz: http://arxiv.org/abs/2408.10926

Observations of Forbush Decreases of cosmic ray electrons and positrons with the Dark Matter Particle Explorer

Autor: Alemanno, Francesca, An, Qi, Azzarello, Philipp, Barbato, Felicia Carla Tiziana, Bernardini, Paolo, Bi, XiaoJun, Cai, MingSheng, Casilli, Elisabetta, Catanzani, Enrico, Chang, Jin, Chen, DengYi, Chen, JunLing, Chen, ZhanFang, Cui, MingYang, Cui, TianShu, Cui, YuXing, Dai, HaoTing, De Benedittis, Antonio, De Mitri, Ivan, de Palma, Francesco, Deliyergiyev, Maksym, Di Santo, Margherita, Ding, Qi, Dong, TieKuang, Dong, ZhenXing, Donvito, Giacinto, Droz, David, Duan, JingLai, Duan, KaiKai, D'Urso, Domenico, Fan, RuiRui, Fan, YiZhong, Fang, Fang, Fang, Kun, Feng, ChangQing, Feng, Lei, Fusco, Piergiorgio, Gao, Min, Gargano, Fabio, Gong, Ke, Gong, YiZhong, Guo, DongYa, Guo, JianHua, Han, ShuangXue, Hu, YiMing, Huang, GuangShun, Huang, XiaoYuan, Huang, YongYi, Ionica, Maria, Jiang, Wei, Kong, Jie, Kotenko, Andrii, Kyratzis, Dimitrios, Li, ., Lei, ShiJun, Li, WenHao, Li, WeiLiang, Li, Xiang, Li, XianQiang, Liang, YaoMing, Liu, ChengMing, Liu, Hao, Liu, Jie, Liu, ShuBin, Liu, Yang, Loparco, Francesco, Luo, ChuanNing, Ma, Miao, Ma, PengXiong, Ma, Tao, Ma, XiaoYong, Marsella, Giovanni, Mazziotta, Mario Nicola, Mo, Dan, Niu, XiaoYang, Pan, Xu, Parenti, Andrea, Peng, WenXi, Peng, XiaoYan, Perrina, Chiara, Qiao, Rui, Rao, JiaNing, Ruina, Arshia, Salinas, MariaMunoz, Shangguan, Zhi, Shen, WeiHua, Shen, ZhaoQiang, Shen, ZhongTao, Silveri, Leandro, Song, JingXing, Stolpovskiy, Mikhail, Su, Hong, Su, Meng, Sun, HaoRan, Sun, ZhiYu, Surdo, Antonio, Teng, XueJian, Tykhonov, Andrii, Wang, JinZhou, Wang, LianGuo, Wang, Shen, Wang, ShuXin, Wang, XiaoLian, Wang, Ying, Wang, YanFang, Wang, YuanZhu, Wei, DaMing, Wei, JiaJu, Wei, YiFeng, Wu, Di, Wu, Jian, Wu, LiBo, Wu, Sha Sha, Wu, Xin, Xia, ZiQing, Xu, EnHeng, Xu, HaiTao, Xu, ZhiHui, Xu, ZunLei, Xue, GuoFeng, Xu, ZiZong, Yang, HaiBo, Yang, Peng, Yang, YaQing, Yao, Hui Jun, Yu, YuHong, Yuan, GuanWen, Yuan, Qiang, Yue, Chuan, Zang, JingJing, Zhang, ShengXia, Zhang, WenZhang, Zhang, Yan, Zhang, Yi, Zhang, YongJie, Zhang, YunLong, Zhang, YaPeng, Zhang, YongQiang, Zhang, ZhiYong, Zhang, Zhe, Zhao, Cong, Zhao, HongYun, Zhao, XunFeng, Zhou, ChangYi, Zhu, Yan, Chen, Wei, Feng, Li, Luo, Xi, Zhu, ChengRui

The Forbush Decrease (FD) represents the rapid decrease of the intensities of charged particles accompanied with the coronal mass ejections (CMEs) or high-speed streams from coronal holes. It has been mainly explored with ground-based neutron monitor

Externí odkaz: http://arxiv.org/abs/2110.00123

Charge measurement of cosmic ray nuclei with the plastic scintillator detector of DAMPE

Autor: Dong, Tiekuang, Zhang, Yapeng, Ma, Pengxiong, Zhang, Yongjie, Bernardini, Paolo, Ding, Meng, Guo, Dongya, Lei, Shijun, Li, Xiang, De Mitri, Ivan, Peng, Wenxi, Qiao, Rui, Di Santo, Margherita, Sun, Zhiyu, Surdo, Antonio, Wang, Zhaomin, Wu, Jian, Xu, Zunlei, Yu, Yuhong, Yuan, Qiang, Yue, Chuan, Zang, Jingjing, Zhang, Yunlong

Publikováno v: In Astroparticle Physics February 2019 105:31-36