首页> 外文会议>Earth Observing Systems XI >Data processing and in-flight calibration systems for OMI-EOS-Aura
【24h】

Data processing and in-flight calibration systems for OMI-EOS-Aura

机译:OMI-EOS-Aura的数据处理和飞行中校准系统

获取原文
获取原文并翻译 | 示例

摘要

The OMI instrument that flies on the EOS Aura mission was launched in July 2004. OMI is a UV-VIS imaging spectrometer that measures in the 270 — 500 nm wavelength range. OMI provides daily global coverage with high spatial resolution. Every orbit of 100 minutes OMI generates about 0.5 GB of Level 0 data and 1.2 GB of Level 1 data. About half of the Level 1 data consists of in-flight calibration measurements. These data rates make it necessary to automate the process of in-flight calibration. For that purpose two facilities have been developed at KNMI in the Netherlands: the OMI Dutch Processing System (ODPS) and the Trend Monitoring and In-flight Calibration Facility (TMCF). A description of these systems is provided with emphasis on the use for radiometric, spectral and detector calibration and characterization. With the advance of detector technology and the need for higher spatial resolution, data rates will become even higher for future missions. To make effective use of automated systems like the TMCF, it is of paramount importance to integrate the instrument operations concept, the information contained in the Level 1 (meta-)data products and the inflight calibration software and system databases. In this way a robust but also flexible end-to-end system can be developed that serves the needs of the calibration staff, the scientific data users and the processing staff. The way this has been implemented for OMI may serve as an example of a cost-effective and user friendly solution for future missions. The basic system requirements for in-flight calibration are discussed and examples are given how these requirements have been implemented for OMI. Special attention is paid to the aspect of supporting the Level 0-1 processing with timely and accurate calibration constants.
机译:履行EOS Aura任务的OMI仪器于2004年7月推出。OMI是一种UV-VIS成像光谱仪,可在270-500 nm波长范围内进行测量。 OMI提供具有高空间分辨率的每日全球覆盖。每100分钟的运行一次OMI都会生成约0.5 GB的0级数据和1.2 GB的1级数据。 1级数据中约有一半由飞行中的校准测量组成。这些数据速率使得有必要使飞行中的校准过程自动化。为此,在荷兰的KNMI开发了两个设施:OMI荷兰处理系统(ODPS)和趋势监测和飞行中校准设施(TMCF)。对这些系统的描述着重于辐射度,光谱和检测器的校准与表征。随着探测器技术的进步以及对更高空间分辨率的需求,未来的任务数据速率将变得更高。为了有效利用TMCF等自动化系统,集成仪器操作概念,级别1(元)数据产品以及机内校准软件和系统数据库中包含的信息至关重要。这样,可以开发出功能强大但又灵活的端到端系统,以满足校准人员,科学数据用户和处理人员的需求。对于OMI实施此方法的方式可以用作未来任务的经济高效且用户友好的解决方案的示例。讨论了飞行中校准的基本系统要求,并举例说明了如何针对OMI实施这些要求。要特别注意以及时准确的校准常数支持0-1级处理的方面。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号