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SPACE ORBITING SPECTROSCOPY TO CHARACTERIZE AEROSOL EMISSIONS OF MEXICO'S POPOCATEPETL VOLCANO

机译:空间轨道光谱学表征墨西哥气溶胶火山气溶胶的排放

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In order to determine the concentration of particles in aerosols, the best sensors identified to date are spectrographic systems or multispectral sensor arrays. A multispectral sensor array requires a maximum of one unit (10 cm3 footprint) in the design of our cubesat monitoring system. La Universidad Popular Aut onoma del Estado de Puebla (UPAEP) is designing a three unit 3U (10 x 10 x 30 cm footprint) cubesat for earth observations, specifically around Puebla and the surrounding volcanic area. A synchronous orbit with a solar inclination of about 98 degrees and between 400-800 km above the earth allows the 3U satellite to pass over the same latitude at the same time every day allowing for the use of a sunlit view of the earth's surface in both visible and infrared wavelengths. UPAEP's 3U cubesat will be designed with a 1) base unit system, 2) an attitude control system and 3) a spectroscopy system unit. This proposal focuses on the development and integration of a multispectral imaging system in a 3U CubeSat using spatial spectroscopy in a series of up to 20 spectral bands within the spectral range of 500-900 nm. The size of the data files collected by the generator can be adjusted to spectral images ranging in sizes of 10 to 500 MB. Consideration of the size of files to be transmitted is a concern due to data transmission rates to the ground station. For example, an orbital altitude of 500 to 800 kilometers, with only one earth station requires a reduction in the number of spectral images taken and transmitted during line of site data collection. The imaging transmission system will choose the strategy of processing the multispectral images on the CubeSats onboard computer and sending results in much smaller data packages (figure 2). All information retrieved at the ground station will serve as a data repository for analysis of climate changes; for the analysis of the volcanic activity of Popocatepetl, and as an additional source of data analysis to the SERVIR research community.
机译:为了确定气溶胶中颗粒的浓度,迄今为止确定的最佳传感器是光谱系统或多光谱传感器阵列。在我们的cubesat监视系统的设计中,多光谱传感器阵列最多需要一个单元(占地10 cm3)。普埃布拉州立大学人口普查局(UPAEP)正在设计一个3单位的3U(10 x 10 x 30厘米足迹)立方体卫星,用于地球观测,尤其是在普埃布拉及其周围火山地区。同步轨道的太阳倾斜角约为98度,并且位于地球上方400-800公里之间,因此3U卫星每天都可以在同一时间通过同一纬度,从而可以在两个方向上使用地球表面的阳光照射可见光和红外波长。 UPAEP的3U cubesat将使用1)基本单元系统,2)姿态控制系统和3)光谱系统单元进行设计。该建议着重于在500-900 nm光谱范围内的多达20个光谱带的空间光谱学中,在3U CubeSat中开发和集成多光谱成像系统。可以将生成器收集的数据文件的大小调整为10到500 MB范围内的光谱图像。由于到地面站的数据传输速率,需要考虑要传输的文件的大小。例如,只有一个地球站的轨道高度为500至800公里,这需要减少在现场数据收集过程中拍摄和发送的光谱图像的数量。成像传输系统将选择在车载CubeSats计算机上处​​理多光谱图像并以较小的数据包发送结果的策略(图2)。在地面站检索到的所有信息都将用作分析气候变化的数据库;用于分析Popocatepetl的火山活动,以及作为SERVIR研究社区的数据分析的另一来源。

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