排序方式： 共有12条查询结果，搜索用时 0 毫秒
11.
《Space Science Reviews》2007,128(1-4):433-506
The Optical, Spectroscopic, and Infrared Remote Imaging System OSIRIS is the scientific camera system onboard the Rosetta
spacecraft (Figure 1). The advanced high performance imaging system will be pivotal for the success of the Rosetta mission.
OSIRIS will detect 67P/Churyumov-Gerasimenko from a distance of more than 106 km, characterise the comet shape and volume, its rotational state and find a suitable landing spot for Philae, the Rosetta
lander. OSIRIS will observe the nucleus, its activity and surroundings down to a scale of ~2 cm px−1. The observations will begin well before the onset of cometary activity and will extend over months until the comet reaches
perihelion. During the rendezvous episode of the Rosetta mission, OSIRIS will provide key information about the nature of
cometary nuclei and reveal the physics of cometary activity that leads to the gas and dust coma.
OSIRIS comprises a high resolution Narrow Angle Camera (NAC) unit and a Wide Angle Camera (WAC) unit accompanied by three
electronics boxes. The NAC is designed to obtain high resolution images of the surface of comet 67P/Churyumov-Gerasimenko
through 12 discrete filters over the wavelength range 250–1000 nm at an angular resolution of 18.6 μrad px−1. The WAC is optimised to provide images of the near-nucleus environment in 14 discrete filters at an angular resolution of
101 μrad px−1. The two units use identical shutter, filter wheel, front door, and detector systems. They are operated by a common Data
Processing Unit. The OSIRIS instrument has a total mass of 35 kg and is provided by institutes from six European countries. 相似文献
12.
在对各种交错网格离散格式的奇偶不耦合数值误差进行了详细的傅里叶分析和比较后,采用一种紧致的交错网格有限体积法将纳维-斯托克斯方程和k-ε湍流模型方程紧密的耦合在一起求解,发展了一套三维定常流程序.通过对NASA Rotor 67设计和非设计工况内部流场的数值模拟结果与实验的比较、分析,初步验证了程序的准确性和可靠性. 相似文献