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91.
Gerstenmaier W 《Acta Astronautica》2004,54(11-12):777-778
This introductory address provides a brief overview and a timeline for construction of the International Space Station, beginning with the July 2000 launch of the Russian Service Module, Zvezda, and ending with the Mission STS-112. 相似文献
92.
Jill Tarter Robert Ackermann William Barott Peter Backus Michael Davis John Dreher Gerald Harp Jane Jordan Tom Kilsdonk Seth Shostak Ken Smolek 《Acta Astronautica》2011,68(3-4):340-346
The Search for ExtraTerrestrial Intelligence (SETI) finally has its own full-time telescope. The Allen telescope array (ATA) in Northern California was dedicated on October 11, 2007. This array, which will eventually be composed of 350 small radio antennas, each 6.1 m in diameter, is being built as a partnership between the SETI Institute and the University of California Radio Astronomy Laboratory. Last October, Paul G. Allen (who provided the funds for the technology development and the first phase of array construction) pushed a silver button and all 42 antennas of the current ATA-42 slewed to point in the direction of the distant galaxy M81. Specialized electronic backend detectors attached to the ATA began making a radio map of that galaxy and simultaneously began SETI observations of HIP48573, a G5V star near M81 on the sky and a distance of 264 light years from Earth. The Allen telescope array will greatly improve the speed of conducting SETI searches over the next few decades, and it will allow a suite of different search strategies to be undertaken. This paper summarizes some of the earliest SETI observations from the array, and describes the search strategies currently being planned. 相似文献
93.
英国温莎和上海完全是天壤之别的。温莎是一个传统的英式小镇,坐落在泰晤士河畔,离伦敦东部20英里,小卵石铺就的街道两旁坐落着小商店和餐馆,而上海是一个生机勃勃的现代化大都市,到处都是马路,商店和人。那么是什么使温莎变得特别呢?首先她是英国女王的主要住所温莎城堡的所在地,而且她有着被世界公认的最著名的学校——伊顿公学。 相似文献
94.
Over the next 2 decades, NASA and ESA are planning a series of space-based observatories to detect and characterize extrasolar planets. This first generation of observatories will not be able to spatially resolve the terrestrial planets detected. Instead, these planets will be characterized by disk-averaged spectroscopy. To assess the detectability of planetary characteristics in disk-averaged spectra, we have developed a spatially and spectrally resolved model of the Earth. This model uses atmospheric and surface properties from existing observations and modeling studies as input, and generates spatially resolved high-resolution synthetic spectra using the Spectral Mapping Atmospheric Radiative Transfer model. Synthetic spectra were generated for a variety of conditions, including cloud coverage, illumination fraction, and viewing angle geometry, over a wavelength range extending from the ultraviolet to the farinfrared. Here we describe the model and validate it against disk-averaged visible to infrared observations of the Earth taken by the Mars Global Surveyor Thermal Emission Spectrometer, the ESA Mars Express Omega instrument, and ground-based observations of earthshine reflected from the unilluminated portion of the Moon. The comparison between the data and model indicates that several atmospheric species can be identified in disk-averaged Earth spectra, and potentially detected depending on the wavelength range and resolving power of the instrument. At visible wavelengths (0.4-0.9 microm) O3, H2O, O2, and oxygen dimer [(O2)2] are clearly apparent. In the mid-infrared (5-20 microm) CO2, O3, and H2O are present. CH4, N2O, CO2, O3, and H2O are visible in the near-infrared (1-5 microm). A comprehensive three-dimensional model of the Earth is needed to produce a good fit with the observations. 相似文献
95.
英国伊顿公学被外界誉为制造精英的"流水线",风靡一时的哈利波特黑色礼服和神秘古堡,让人不得不相信"魔力"依存的伊顿,迄今已有19名英国首相从那座"古堡"中走了出来。伦敦以西20多英里的温莎小镇,浸润着英王室数百年的"恩泽"。567个年头的漫漫岁月,侵蚀了伊顿古旧的砖墙,让伊顿显得有些老气横秋,但是,伊顿依然坚守着传统的价值,锤炼着过去,现在和未来恒久的伊顿教育的"哲学"。伊顿的教育不只在于成功,而是在于孩子们一个完整的人生,为此,成绩和专业仅仅只是他们的一个基本点。 相似文献
96.
Raymond M. Wheeler Gary W. Stutte Cheryl L. Mackowiak Neil C. Yorio John C. Sager William M. Knott 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(5):798-806
Plants can provide a means for removing carbon dioxide (CO2) while generating oxygen (O2) and clean water for life support systems in space. To study this, 20 m2 stands of potato (Solanum tuberosum L.) plants were grown in a large (113 m3 vol.), atmospherically closed chamber. Photosynthetic uptake of CO2 by the stands was detected about 10 DAP (days after planting), after which photosynthetic rates rose rapidly as stand ground cover and total light interception increased. Photosynthetic rates peaked ca. 50 DAP near 45 μmol CO2 m−2 s−1 under 865 μmol m−2 s−1 PPF (average photosynthetic photon flux), and near 35 μmol CO2 m−2 s−1 under 655 μmol m−2 s−1 PPF. Short term changes in PPF caused a linear response in stand photosynthetic rates up to 1100 μmol m−2 s−1 PPF, with a light compensation point of 185 μmol m−2 s−1 PPF. Comparisons of stand photosynthetic rates at different CO2 concentrations showed a classic C3 response, with saturation occurring near 1200 μmol mol−1 CO2 and compensation near 100 μmol mol−1 CO2. In one study, the photoperiod was changed from 12 h light/12 h dark to continuous light at 58 DAP. This caused a decrease in net photosynthetic rates within 48 h and eventual damage (scorching) of upper canopy leaves, suggesting the abrupt change stressed the plants and/or caused feedback effects on photosynthesis. Dark period (night) respiration rates increased during early growth as standing biomass increased and peaked near 9 μmol CO2 m−2 s−1 ca. 50 DAP, after which rates declined gradually with age. Stand transpiration showed a rapid rise with canopy ground cover and peaked ca. 50 DAP near 8.9 L m−2 d−1 under 860 μmol m−2 s−1 PPF and near 6.3 L m−2 d−1 under 650 μmol m−2 s−1 PPF. Based on the best photosynthetic rates from these studies, approximately 25 m2 of potato plants under continuous cultivation would be required to support the CO2 removal and O2 requirements for one person. 相似文献
97.
Long-duration spacecraft in low earth orbit such as the International Space Station (ISS) are highly susceptible to high-speed impacts by pieces of debris from past earth-orbiting missions. Among the hazards that accompany the penetration of a pressurized manned spacecraft are critical crack propagation in the module wall, crew hypoxia, and uncontrolled thrust due to air rushing out of the module wall hole. A Monte Carlo simulation tool was used to determine the effect of spacecraft wall construction on the survivability of ISS modules and crew following an orbital debris penetration. The simulation results indicate that enhanced shield wall designs (i.e., multi-wall systems with heavier inner bumpers) always lead to higher overall survivability of the station and crew due to an overwhelming decrease in likelihood of module penetration. The results of the simulations also indicate that changes in crew operations, equipment locations, and operation procedures can significantly reduce the likelihood of crew or station loss following an orbital debris penetration. 相似文献
98.
99.
A two-port with both generator and load constitutes a closed system; it can be defined as a system with only interdependent variables or as a system containing no independent variables. The flowgraph describes the relationships between variables in a closed system as determined by the topology of its components. The corresponding closed flowgraph represents a zero-port network from which N-port networks can be generated as subsets by truncation of the closed system. A constraint governing any closed system expressing the properties of its cut-sets and tie-sets is referred to as the topology equation. The topology equation can be computed from the sum of loops in the closed flowgraph, and forms the key for the derivation of properties of closed systems and derived N-port subsets. Oscillators analyzed as zero-ports are discussed in detail to illustrate the rationale for the flowgraph approach to closed systems. To exploit the closed system model conceptually and computationally for N-ports, an approach is suggested and illustrated for N = 1 by an analysis of transfer functions and for N = 2 by a sensitivity analysis of stochastic networks. 相似文献
100.