Calibration of the operative cosmic ray detector at Marambio Base in the Antarctic Peninsula

N. A. Santos, S. Dasso, A. Gulisano, O. Areso, Matías Pereira
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Abstract

During 2019 an Antarctic Space Weather Laboratory was deployed at Marambio base in the Antarctic Peninsula. The main instrument installed was a cosmic ray detector based on water Cherenkov radiation (WCD). This detector is the first permanent Antarctic node of the LAGO (Latin American Giant Observatory) Collaboration. Long-term calibrated observations of the WCD will be presented here. Finally, the global galactic cosmic rays variability observed with the WCD will be compared with observations of a neutron monitor with similar rigidity cut off than the Marambio site.
南极半岛马兰姆比奥基地宇宙射线探测器的校准
2019年,在南极半岛的马拉比奥基地部署了一个南极空间天气实验室。安装的主要仪器是基于水切伦科夫辐射(WCD)的宇宙射线探测器。这个探测器是LAGO(拉丁美洲巨人天文台)合作的第一个永久南极节点。这里将介绍WCD的长期校准观测结果。最后,用WCD观测到的全球星系宇宙射线变异性将与与Marambio站点具有类似刚性切断的中子监测仪的观测结果进行比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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