标题： Mirya-m1宇宙射线探测器：特征与第一年观测结果 显示英文标题

标题： The Mirya-m1 Cosmic Ray Detector: Features and First Year Observations

摘要： 我们介绍了Mirya-m1宇宙射线探测器，这是土耳其唯一且最大的用于空间天气研究的宇宙射线探测器。Mirya-m1是根据穆顿撞击示踪仪和观测仪（MITO）（Ayuso等人，2021年）模型和建造的，位于土耳其埃尔祖鲁姆的土耳其国家天文台东方安纳托利亚天文台（DAG）站点，海拔3099米。这一高度使Mirya-m1成为全球海拔最高的宇宙射线探测器之一。该探测器由两个堆叠的闪烁计数器组成，每个计数器测量尺寸为1x1米，并且它们之间垂直距离为1.36米。每个闪烁计数器由四个H1411型Hamamatsu光电倍增管监测，能够精确检测和测量入射宇宙射线产生的光。在这项研究中，我们展示了2024年收集的数据，其中包括在2024年3月和5月检测到的两次Forbush减小事件。这些重要的检测结果证明了Mirya-m1能够为空间天气研究提供有价值的数据，确立了它作为该地区宇宙射线研究关键仪器的潜力。 显示英文摘要

摘要： We introduce the Mirya-m1 Cosmic Ray Detector, the largest and only cosmic ray detector in Turkiye designed for space weather research. Mirya-m1, modeled and built after the Muon Impact Tracer and Observer (MITO) (Ayuso et al. 2021), is located at the Eastern Anatolia Observatory (DAG) site of the Turkiye National Observatories in Erzurum, Turkiye, at an altitude of 3099 meters. This elevation positions Mirya-m1 among the highest-altitude cosmic ray detectors globally. The detector consists of two stacked scintillator counters, each measuring 1x1 meters, separated by a vertical distance of 1.36 meters. Each scintillator is monitored by four H1411 Hamamatsu photomultiplier tubes, enabling precise detection and measurement of light by incident cosmic rays. In this study, we present the data collected throughout 2024, which includes the detection of two Forbush decrease events in March and May 2024. These significant detections demonstrate the capability of Mirya-m1 to contribute valuable data for space weather research, establishing its potential as a critical instrument for cosmic ray studies in the region.