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81.
M. Gelman F. Finger A. Miller K. Johnson R. Nagatani 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,4(4):29-32
The National Meteorological Center of the National Oceanic and Atmospheric Administration (NOAA) has archived global, daily synoptic analyses and computer gridded fields of geopotential height and temperature for 8 stratospheric pressure levels (70, 50, 30, 10, 5, 2, 1 and 0.4 mb) since the Autumn of 1978. More restricted analyses are available since 1964. The fields are discussed, with special emphasis on improvement of the data bases and analysis procedures. Included in the discussions are screening procedures for the climatological data base. Examples are given with regard to monthly mean energy, wind and hemispheric temperature patterns calculated as the initial development of a stratospheric dynamic climatology. 相似文献
82.
The problem of high-frequency radio direction finding (HFDF) has perennially been compounded by the interference effects of multicomponent wavefields. The wavefields are generally produced by ionospheric multipath or cochannel interference from other transmitted signals. Because HFDF sytems must operate on short duration signals and are usually restricted to limited antenna array apertures, modern techniques of superresolution spectral analysis are applied to resolve the constituency of multicomponent wavefields. This paper presents a performance comparison of five superresolution spectral algorithms in solving the HFDF wave interference problem. 相似文献
83.
New, innovative joint safety policies and requirements were developed in support of the Shuttle/Mir program, which is the first phase of the International Space Station program. This work has resulted in a joint multinational analysis culminating in joint certification for mission readiness. For these planning and development efforts, each nation's risk programs and individual safety practices had to be integrated into a comprehensive and compatible system that reflects the joint nature of the endeavor. This paper highlights the major incremental steps involved in planning and program integration during development of the Shuttle/Mir program. It traces the transition from early development to operational status and highlights the valuable lessons learned that apply to the International Space Station program (Phase 2). Also examined are external and extraneous factors that affected mission operations and the corresponding solutions to ensure safe and effective Shuttle/Mir missions. 相似文献
84.
M. R. Torr D. G. Torr M. Zukic R. B. Johnson J. Ajello P. Banks K. Clark K. Cole C. Keffer G. Parks B. Tsurutani J. Spann 《Space Science Reviews》1995,71(1-4):329-383
The aurorae are the result of collisions with the atmosphere of energetic particles that have their origin in the solar wind, and reach the atmosphere after having undergone varying degrees of acceleration and redistribution within the Earth's magnetosphere. The global scale phenomenon represented by the aurorae therefore contains considerable information concerning the solar-terrestrial connection. For example, by correctly measuring specific auroral emissions, and with the aid of comprehensive models of the region, we can infer the total energy flux entering the atmosphere and the average energy of the particles causing these emissions. Furthermore, from these auroral emissions we can determine the ionospheric conductances that are part of the closing of the magnetospheric currents through the ionosphere, and from these we can in turn obtain the electric potentials and convective patterns that are an essential element to our understanding of the global magnetosphere-ionosphere-thermosphere-mesosphere. Simultaneously acquired images of the auroral oval and polar cap not only yield the temporal and spatial morphology from which we can infer activity indices, but in conjunction with simultaneous measurements made on spacecraft at other locations within the magnetosphere, allow us to map the various parts of the oval back to their source regions in the magnetosphere. This paper describes the Ultraviolet Imager for the Global Geospace Sciences portion of the International Solar-Terrestrial Physics program. The instrument operates in the far ultraviolet (FUV) and is capable of imaging the auroral oval regardless of whether it is sunlit or in darkness. The instrument has an 8° circular field of view and is located on a despun platform which permits simultaneous imaging of the entire oval for at least 9 hours of every 18 hour orbit. The three mirror, unobscured aperture, optical system (f/2.9) provides excellent imaging over this full field of view, yielding a per pixel angular resolution of 0.6 milliradians. Its FUV filters have been designed to allow accurate spectral separation of the features of interest, thus allowing quantitative interpretation of the images to provide the parameters mentioned above. The system has been designed to provide ten orders of magnitude blocking against longer wavelength (primarily visible) scattered sunlight, thus allowing the first imaging of key, spectrally resolved, FUV diagnostic features in the fully sunlit midday aurorae. The intensified-CCD detector has a nominal frame rate of 37 s, and the fast optical system has a noise equivalent signal within one frame of 10R. The instantaneous dynamic range is >1000 and can be positioned within an overall gain range of 104, allowing measurement of both the very weak polar cap emissions and the very bright aurora. The optical surfaces have been designed to be sufficiently smooth to permit this dynamic range to be utilized without the scattering of light from bright features into the weaker features. Finally, the data product can only be as good as the degree to which the instrument performance is characterized and calibrated. In the VUV, calibration of an an imager intended for quantitative studies is a task requiring some pioneering methods, but it is now possible to calibrate such an instrument over its focal plane to an accuracy of ±10%. In summary, very recent advances in optical, filter and detector technology have been exploited to produce an auroral imager to meet the ISTP objectives. 相似文献
85.
Pfiffner SM Onstott TC Ruskeeniemi T Talikka M Bakermans C McGown D Chan E Johnson A Phelps TJ Le Puil M Difurio SA Pratt LM Stotler R Frape S Telling J Lollar BS Neill I Zerbin B 《Astrobiology》2008,8(3):623-638
A scientific drilling expedition to the High Lake region of Nunavut, Canada, was recently completed with the goals of collecting samples and delineating gradients in salinity, gas composition, pH, pe, and microbial abundance in a 400 m thick permafrost zone and accessing the underlying pristine subpermafrost brine. With a triple-barrel wireline tool and the use of stringent quality assurance and quality control (QA/QC) protocols, 200 m of frozen, Archean, mafic volcanic rock was collected from the lower boundary that separates the permafrost layer and subpermafrost saline water. Hot water was used to remove cuttings and prevent the drill rods from freezing in place. No cryopegs were detected during penetration through the permafrost. Coring stopped at the 535 m depth, and the drill water was bailed from the hole while saline water replaced it. Within 24 hours, the borehole iced closed at 125 m depth due to vapor condensation from atmospheric moisture and, initially, warm water leaking through the casing, which blocked further access. Preliminary data suggest that the recovered cores contain viable anaerobic microorganisms that are not contaminants even though isotopic analyses of the saline borehole water suggests that it is a residue of the drilling brine used to remove the ice from the upper, older portion of the borehole. Any proposed coring mission to Mars that seeks to access subpermafrost brine will not only require borehole stability but also a means by which to generate substantial heating along the borehole string to prevent closure of the borehole from condensation of water vapor generated by drilling. 相似文献
86.
87.
88.
Pamela G. Conrad Jennifer L. Eigenbrode Max O. Von?der Heydt Claus T. Mogensen John Canham Dan N. Harpold Joel Johnson Therese Errigo Daniel P. Glavin Paul R. Mahaffy 《Space Science Reviews》2012,170(1-4):479-501
Mars Science Laboratory’s Curiosity rover carries a set of five external verification standards in hermetically sealed containers that can be sampled as would be a Martian rock, by drilling and then portioning into the solid sample inlet of the Sample Analysis at Mars (SAM) suite. Each organic check material (OCM) canister contains a porous ceramic solid, which has been doped with a fluorinated hydrocarbon marker that can be detected by SAM. The purpose of the OCM is to serve as a verification tool for the organic cleanliness of those parts of the sample chain that cannot be cleaned other than by dilution, i.e., repeated sampling of Martian rock. SAM possesses internal calibrants for verification of both its performance and its internal cleanliness, and the OCM is not used for that purpose. Each OCM unit is designed for one use only, and the choice to do so will be made by the project science group (PSG). 相似文献
89.
J. B. Blake J. F. Fennell L. M. Friesen B. M. Johnson W. A. Kolasinski D. J. Mabry J. V. Osborn S. H. Penzin E. R. Schnauss H. E. Spence D. N. Baker R. Belian T. A. Fritz W. Ford B. Laubscher R. Stiglich R. A. Baraze M. F. Hilsenrath W. L. Imhof J. R. Kilner J. Mobilia D. H. Voss A. Korth M. Güll K. Fisher M. Grande D. Hall 《Space Science Reviews》1995,71(1-4):531-562
90.
I R Johnson 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1996,18(1-2):163-166
Physiological models in the plant and crop sciences provide a means of integrating different aspects of the system, in particular the interaction between plant processes and environmental factors. This paper focuses on the response of canopy photosynthesis, including adaptation, to environmental conditions. Adaptation is likely to be important when considering controlled ecological life support systems since physiological characteristics are affected by past as well as current environmental conditions. In particular, the level of photosynthetic enzymes in a plant is generally greater for plants grown in high irradiance levels than for similar plants grown in low irradiance. The models have been developed to apply to 'normal' growing conditions, although the principles will apply to closed bioregenerative systems. 相似文献