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71.
One of the main limitations to the sensitivity of observations carried out withthe ISOCAM infrared camera comes from the responsivity variations and glitchescaused by impacts of charged particles. After more than 28 months of successfuloperations, the predicted glitch rate has been re-evaluated and compared toin-flight measurements. Glitch properties have been studied in orderto improve the removal algorithms, and thus the ultimate sensitivity of ISOCAM.All informations about the glitch phenomenon are very useful in order toprepare next space experiments. 相似文献
72.
A. Abergel M. A. Miville-Deschênes F. X. Désert M. Pérault H. Aussel M. Sauvage 《Experimental Astronomy》2000,10(2-3):353-368
The detector of the long wavelength channel of the ISOCAMcamera on-board the Infrared Space Observatory is a Galliumdoped Silicon photo-conductor hybridized by Indium bump. Itpresents systematic memory effects of the response which canbias the photometry by a factor of typically 40%. The main features of the response after flux variations are discussed. A simple empirical model actually used to correct systematically the data with a photometric accuracy of 5–10% is detailed. 相似文献
73.
GPS/INS直接定向精度分析 总被引:1,自引:0,他引:1
近年来,GPS/INS融合技术在国内逐渐被应用于航空摄影测量中,利用其直接获得外方位元素,从而减少外业控制点。通过试验,在DMC数码相机同高精度的GPS/INS系统联结下,直接获取了试验区的外方位元素,并对GPS/INS数据直接定向的精度进行分析和总结,得出了一些有益的结论。 相似文献
74.
热带大气季节内振荡的一个数值模拟研究 总被引:9,自引:2,他引:9
文中分析了中国科学院大气物理研究所全球气候谱模式ALGCM (R4 2L9) 12a(1978~ 1989年 )积分的逐日输出结果 ,并与 1978~ 1989年的逐日NCEP资料对照 ,以此对热带季节内振荡 (30~ 6 0d振荡 )进行数值模拟研究。分析表明 ,该模式在热带地区可以模拟出明显的季节内振荡 (ISO)的准周期信号 ,并抓住了热带ISO的基本传播特征 ,能较好地再现东、西半球传播速度的差异 ,同时模式模拟存在东传要好于西传 ,冬、春季的模拟要好于夏、秋季的现象。该模式模拟的热带ISO的强度较许多大气模式明显提高 ,尤其是对 2 0 0hPa上ISO动能强度的模拟。模式基本模拟出了ISO低层辐合、高层辐散的水平风场特征。模式较好地再现了热带ISO纬向风的垂直结构。此外 ,观测资料表明热带ISO在冬、春强 ,而夏、秋弱的季节性倾向与ISO的年际变化相联系 ,模拟的ISO在季节性倾向偏差上表现为冬、夏相对强 ,而春、秋相对弱。垂直速度、散度、水汽等物理量的配置同NCEP资料的结构特征仍有明显差异 ,模拟的ISO空间分布也不太理想 ,表明要很好模拟ISO结构和空间分布特征 ,还须做不少工作。 相似文献
75.
76.
Developments at ISO/REMCO and its Impact on the Production and Use of Geological Reference Materials
Angelique Botha 《Geostandards and Geoanalytical Research》2010,34(3):237-244
During the past decade the work of ISO/REMCO, the International Organization for Standardization’s Technical Committee on Reference Materials, was dedicated to achieving global harmonisation, and true involvement of the member countries. The first major accomplishment was the clarification of the terminology in the definitions for reference material and certified reference material, which were published as an amendment to ISO Guide 30 in 2008. The next milestone was the recognition that ISO Guide 34 (‘General requirements for the competence of reference material producers’) be used in conjunction with ISO/IEC 17025 for the accreditation of reference material producers. The third edition of ISO Guide 34 published in November 2009, clarifies the acceptable procedures for the certification of reference materials. This paper will discuss the role of ISO/REMCO in formalising the procedures for the accreditation of reference material producers and the evolution of the terms reference material and certified reference material. The paper will conclude with a case study, where a primary method in a single laboratory – one of the recognised acceptable metrologically valid procedures according to ISO Guide 34 – was used for the certification of reference materials. The reference materials are South African Reference Material SARM 2 (Syenite), SARM 3 (Lujavrite) and SARM 4 (Norite) from the suite of six NIMROCs that were originally certified by the Council for Mineral Technology (MINTEK) in South Africa in the 1970s. 相似文献
77.
Temporal and Spatial Characteristics of Intraseasonal Oscillations in the Meridional Wind Field over the Subtropical Northern Pacific 总被引:1,自引:0,他引:1
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Based on the NCEP/NCAR reanalysis I daily data from 1958 to 2002, climatic characteristics of the 30-60-day intraseasonal oscillations (ISOs) of the zonal wind (u), meridional wind (v), and geopotential height (h) over global areas and especially the ISO of v over the subtropical northern Pacific are analyzed using the space-time spectrum analysis and wavelet transform methods. The results show that the ISO of v is very different from those of u and h, with the former representing the meridional low-frequency disturbances, which are the most active in the subtropics and mid-high latitudes, but very weak in the tropics. In the subtropical Northern Hemisphere, the energies of the ISOs of u and h are both concentrated on the waves with wave number of 1 and periods of 30-60 days, while the main energy of the ISO of v is concentrated on the waves with wave numbers of 4-6 and periods of 30-60 and 70-90 days. The westward propagating energies for the 30-60-day oscillations of u, v, and h are all stronger than the eastward propagating energies in the subtropics. In addition, the ISO of v is the strongest (weakest) in summer (winter) over the subtropics of East Asia and northwestern Pacific, while the situation is reversed over the subtropical northeastern Pacific, revealing a "seesaw" of the ISO intensity with seasons over the subtropics from the northwestern to northeastern Pacific. In the subtropical northwestern Pacific, the interannual and interdecadal changes of the ISO for v at 850 hPa indicate that its activities are significantly strong during 1958 1975, while obviously weak during 1976-1990, and are the strongest during 1991-2000, and its spectral energy is obviously abnormal but ruleless during the ENSO periods. However, in the 2 7-yr bandpass filtering series, the interannual changes of the v ISO over the subtropical northwestern Pacific contain distinct ENSO signals. And in the 9-yr low-pass filtering series, the v ISO changes over the subtropical northwestern Pacific are significantly out of phase with the changes of the Ni(n)o -3.4 SST, whereas the v ISO changes in the subtropical northeastern Pacific are significantly in phase with the changes of the Ni(n)o-3.4 SST. 相似文献
78.
IMU/DGPS辅助航空摄影测量中检校场布设方案研究 总被引:6,自引:0,他引:6
在IMU/DGPS辅助航空摄影测量生产中,布设检校场的作用、检校场如何布设、飞行的频率以及飞行中的注意事项等一直是国内外众多学者专家积极讨论的内容.文中对检校场所起的作用进行了系统分析,提出了检校场的布设方案,并进行了大量的实测数据实验,探讨了上述问题. 相似文献
79.
Leech K. Crovisier J. Bockelée-Morvan D. Brooke T. Y. Hanner M. S. Altieri B. Keller H. U. Lellouch E. Lim T. 《Earth, Moon, and Planets》1997,78(1-3):81-83
Spectra of comet C/1995 O1 (Hale-Bopp) were obtained with the Infrared Space Observatory (ISO) at medium resolution with the
grating spectrometer in the photometer (PHT-S) and/or at high resolution with the short wavelength spectrometer (SWS) and
long wavelength spectrometer (LWS) in April 1996 (Crovisier et al., 1996), September–October 1996 (Crovisier et al., 1997a,
b) and December 1997, at distances from the Sun of 4.6, 2.9 and 3.9 AU, respectively. For the first time, high-resolution
spectra of a comet covering the entire 2.4 to 200 μm spectral range were obtained.
The vibrational bands of H2O, CO2 and CO are detected in emission with PHT-S. Relative production rates of 100:22:70 are derived for H2O:CO2:CO at 3 AU pre-perihelion. H2O is observed at high spectral resolution in the ν3 group of bands around 2.7 μm and the ν2 group around 6 μm with SWS, and in several rotational lines in the 100–180 μm region with LWS. The high signal-to-noise ratio
of the ν3 band observed on September–October 1996 allows accurate determinations of the water rotational temperature (28 K) and of
its ortho-to-para ratio(2.45 ± 0.10, which significantly differs from the high temperature limit and corresponds to a spin
temperature of 25 K).
Longward of 6 μm the spectrum is dominated by dust thermal continuum emission, upon which broad emission features are superimposed.
The wavelengths of the emission peaks correspond to those of Mg-rich crystalline olivine (forsterite). In the September–October
1996 spectra, emission features at 45 and 65 μm and possible absorption at 2.9–3.2 μm suggest that grains of water ice were
present at 3 AU from the Sun.
The observations made post-perihelion in late December 1997 led to the detections of H2O, CO2 and CO at 3.9 AU from the Sun (Figures 1 and 2). The production rates were ≈3.0 × 1028,3.5 × 1028 and ≈1.5 × 1029 s-1, respectively. This corresponds to H2O:CO2:CO = 100:110:500 and confirms that at such distances from the Sun, cometary activity is dominated by sublimation of CO and
CO2 rather than by H2O.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
80.
ISO19100地理信息系列标准特点及其本土化 总被引:9,自引:3,他引:6
采用国际标准和国外先进标准是国民经济发展的重要技术基础工作。文章简略介绍国际标准化组织地理信息技术委员会(ISO/TC211)研制ISO19100地理信息系列标准的概况,着重分析其结构体系、研制特点,讨论将这些标准转化为国家标准,即本土化工作应当遵循的原则、方法、国家标准与国际标准一致性程度划分等问题,并提出ISO19100地理信息系列标准本土化工作的建议。 相似文献