首页 | 本学科首页   官方微博 | 高级检索  
     检索      


The Mercury Dual Imaging System on the MESSENGER Spacecraft
Authors:S Edward Hawkins III  John D Boldt  Edward H Darlington  Raymond Espiritu  Robert E Gold  Bruce Gotwols  Matthew P Grey  Christopher D Hash  John R Hayes  Steven E Jaskulek  Charles J Kardian Jr  Mary R Keller  Erick R Malaret  Scott L Murchie  Patricia K Murphy  Keith Peacock  Louise M Prockter  R Alan Reiter  Mark S Robinson  Edward D Schaefer  Richard G Shelton  Raymond E Sterner II  Howard W Taylor  Thomas R Watters  Bruce D Williams
Institution:(1) The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA;(2) Applied Coherent Technology, Herndon, VA 20170, USA;(3) School of Earth and Space Exploration, Arizona State University, Box 871404, Tempe, AZ 85287-1404, USA;(4) Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC 20013, USA
Abstract:The Mercury Dual Imaging System (MDIS) on the MESSENGER spacecraft will provide critical measurements tracing Mercury’s origin and evolution. MDIS consists of a monochrome narrow-angle camera (NAC) and a multispectral wide-angle camera (WAC). The NAC is a 1.5° field-of-view (FOV) off-axis reflector, coaligned with the WAC, a four-element refractor with a 10.5° FOV and 12-color filter wheel. The focal plane electronics of each camera are identical and use a 1,024×1,024 Atmel (Thomson) TH7888A charge-coupled device detector. Only one camera operates at a time, allowing them to share a common set of control electronics. The NAC and the WAC are mounted on a pivoting platform that provides a 90° field-of-regard, extending 40° sunward and 50° anti-sunward from the spacecraft +Z-axis—the boresight direction of most of MESSENGER’s instruments. Onboard data compression provides capabilities for pixel binning, remapping of 12-bit data into 8 bits, and lossless or lossy compression. MDIS will acquire four main data sets at Mercury during three flybys and the two-Mercury-solar-day nominal mission: a monochrome global image mosaic at near-zero emission angles and moderate incidence angles, a stereo-complement map at off-nadir geometry and near-identical lighting, multicolor images at low incidence angles, and targeted high-resolution images of key surface features. These data will be used to construct a global image base map, a digital terrain model, global maps of color properties, and mosaics of high-resolution image strips. Analysis of these data will provide information on Mercury’s impact history, tectonic processes, the composition and emplacement history of volcanic materials, and the thickness distribution and compositional variations of crustal materials. This paper summarizes MDIS’s science objectives and technical design, including the common payload design of the MDIS data processing units, as well as detailed results from ground and early flight calibrations and plans for Mercury image products to be generated from MDIS data.
Keywords:MESSENGER  Mercury  Imaging  Camera  Imager  CCD  Heat pipe  Wax pack  Photometry  Stereo
本文献已被 SpringerLink 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号