Spectroscopy and Spectral Analysis, Volume. 42, Issue 1, 203(2022)
Using Onion-Peeling Method to Inverse Ozone Density Based on the Stellar Occultation Technology in the Near Space Region
Figures & Tables(7)
Fig. 2. The transmission of Alp Gru star in 20~40 km in June 1, 2003 by GOMOS
Fig. 4. The comparison of the inversed ozone densities above 50 km
Fig. 5. The comparison of the inversed ozone densities below 50 km
Table 1. The Primary parameter of GOMOS
View tableView in ArticleTable 1. The Primary parameter of GOMOS
性质/模块 参数 尺寸, 功耗, 传输速度 175 kg, 200 W, 226 kbit·s-1 望远镜 30 cm×20 cm 指向系统 追踪恒星100 Hz; 稳定性优于40微弧 覆盖角度 方位角-10°~90°, 仰角62°~68° 目标恒星 视星等m=-1.4~5, 温度T=3 000~30 000 K 紫外-可见光光谱仪 波段248~690 nm, 分辨率0.8 nm, 采样率2 Hz 红外光谱仪 波段750~776和916~956 nm, 分辨率0.13 nm, 采样率2 Hz 光度计 蓝色: 470~520 nm, 红色: 650~700 nm, 采样率1 kHz
Table 2. The situation of inversed occultation events
View tableView in ArticleTable 2. The situation of inversed occultation events
事件号 事件文件编号 开始时间/UTC 结束时间/UTC 光照情况 目标恒星 测量层数 1 7 946 20:48:14 20:49:12 夜间 9Alp CMa 115 2 7 288 15:46:23 15:47:22 夜间 9Alp CMa 117 3 7357 10:44:38 10:45:28 夜间 9Alp CMa 101
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. Using Onion-Peeling Method to Inverse Ozone Density Based on the Stellar Occultation Technology in the Near Space Region[J]. Spectroscopy and Spectral Analysis, 2022, 42(1): 203
Paper Information
Category: Research Articles
Received: Dec. 2, 2020
Accepted: --
Published Online: Mar. 31, 2022
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