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421.
提出了适用于跟踪在复杂背景下快速移动目标的实时跟踪系统.利用基于马尔可夫场模型的背景减除算法检测像素变化,以跟踪移动目标.分割掩膜的先验概率用马尔可夫场模型来表示,因此目标跟踪任务即被转化成最大后验问题.实验结果表明,本文算法在简单背景或复杂背景下的离线和在线移动目标跟踪方面均有较好的效果. 相似文献
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Segura A Krelove K Kasting JF Sommerlatt D Meadows V Crisp D Cohen M Mlawer E 《Astrobiology》2003,3(4):689-708
Coupled radiative-convective/photochemical modeling was performed for Earth-like planets orbiting different types of stars (the Sun as a G2V, an F2V, and a K2V star). O(2) concentrations between 1 and 10(-5) times the present atmospheric level (PAL) were simulated. The results were used to calculate visible/near-IR and thermal-IR spectra, along with surface UV fluxes and relative dose rates for erythema and DNA damage. For the spectral resolution and sensitivity currently planned for the first generation of terrestrial planet detection and characterization missions, we find that O(2) should be observable remotely in the visible for atmospheres containing at least 10(-2) PAL of O(2). O(3) should be visible in the thermal-IR for atmospheres containing at least 10(-3) PAL of O(2). CH(4) is not expected to be observable in 1 PAL O(2) atmospheres like that of modern Earth, but it might be observable at thermal-IR wavelengths in \"mid-Proterozoic-type\" atmospheres containing approximately 10(-1) PAL of O(2). Thus, the simultaneous detection of both O(3) and CH(4) - considered to be a reliable indication of life - is within the realm of possibility. High-O(2) planets orbiting K2V and F2V stars are both better protected from surface UV radiation than is modern Earth. For the F2V case the high intrinsic UV luminosity of the star is more than offset by the much thicker ozone layer. At O(2) levels below approximately 10(-2) PAL, planets around all three types of stars are subject to high surface UV fluxes, with the F2V planet exhibiting the most biologically dangerous radiation environment. Thus, while advanced life is theoretically possible on high-O(2) planets around F stars, it is not obvious that it would evolve as it did on Earth. 相似文献
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本文描述了中分辨率成像光谱仪(MERIS)的设计。该仪器已被选为计划于1997年发射的欧洲极轨平台上的一个核心仪器。其光谱覆盖范围为400nm到1050nm,覆盖区宽度为1500km,光谱分辨率为1.5nm,空间分辨率为260m。此仪器主要用于海洋、陆地和大气方面的研究。 相似文献
425.
四向织物增强碳一碳复合材料的研究工作正在进行中。这种复合材料是为制造在工作时承受很高的热应力的零、部件而专门设计的。本文概要地描述了四向织物并指出它与三向、七向、十一向相比较所具有的优点。四向织物是用单向碳纱按“抽拉工艺”制得的杆制造的,复合研究证明沥青在压力下浸渍-碳化工艺是优越的。 相似文献
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In the frame of the EXPOSE-E mission on the Columbus external payload facility EuTEF on board the International Space Station, passive thermoluminescence dosimeters were applied to measure the radiation exposure of biological samples. The detectors were located either as stacks next to biological specimens to determine the depth dose distribution or beneath the sample carriers to determine the dose levels for maximum shielding. The maximum mission dose measured in the upper layer of the depth dose part of the experiment amounted to 238±10 mGy, which relates to an average dose rate of 408±16 μGy/d. In these stacks of about 8?mm height, the dose decreased by 5-12% with depth. The maximum dose measured beneath the sample carriers was 215±16 mGy, which amounts to an average dose rate of 368±27 μGy/d. These values are close to those assessed for the interior of the Columbus module and demonstrate the high shielding of the biological experiments within the EXPOSE-E facility. Besides the shielding by the EXPOSE-E hardware itself, additional shielding was experienced by the external structures adjacent to EXPOSE-E, such as EuTEF and Columbus. This led to a dose gradient over the entire exposure area, from 215±16 mGy for the lowest to 121±6 mGy for maximum shielding. Hence, the doses perceived by the biological samples inside EXPOSE-E varied by 70% (from lowest to highest dose). As a consequence of the high shielding, the biological samples were predominantly exposed to galactic cosmic heavy ions, while electrons and a significant fraction of protons of the radiation belts and solar wind did not reach the samples. 相似文献
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爱丁堡皇家天文台的COSMOS自动测量仪是为现代化的大型施密特望远镜的天文数据测量而设计的测量系统。COSMOS的功能之一是自动地从拍摄到的大量星体图象中分离出星系图象。设在澳大利亚的英国施密特望远镜能拍到南天的23等星。COSMOS对施密特望远镜干板测量后,自动识别出星系图象,这样就能对大量可观测的宇宙天体中的星系分布情况进行研究。 相似文献