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41.
42.
This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination
of the Huygens atmospheric probe into Titan's atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing
observations of Titan. This not only provides a rich harvest of data about Saturn's famous satellite but will permit a useful
calibration of the remote-sensing instruments which will also be used on Saturn itself. Composition, thermal structure, dynamics,
aeronomy, magnetosphere interactions and origins will all be investigated for the two atmospheres, and the spacecraft will
also deliver information on the interiors of both Titan and Saturn. As the surface of Titan is intimately linked with the
atmosphere, we also discuss some of the surface studies that will be carried out by both probe and orbiter.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
43.
Daniel Cadet 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(4):113-120
The GARP Monsoon Experiment (MONEX) provided a unique set of observations during the months May, June, July and August 1979, to study the Indian summer monsoon. Data sets from different platforms were collected during this period. In this paper, these platforms are reviewed and their data are presented with a special emphasis on the non-conventional ones : geostationary satellite (GOES), constant-level balloons (BALSAMINE Experiment) and instrumented aircrafts. Some results on the low-level circulation over the Arabian Sea as deduced from these observations are given. In 1979, the onset of the monsoon was very late and took place around mid-June. It was characterized by the formation of a vortex off the western coast of India and its later westward displacement over the Arabian Sea. 相似文献
44.
Roger C. Wiens Daniel B. Reisenfeld Chad Olinger Peter Wurz Veronika S. Heber Donald S. Burnett 《Space Science Reviews》2013,175(1-4):93-124
The Genesis mission Solar Wind Concentrator was built to enhance fluences of solar wind by an average of 20x over the 2.3 years that the mission exposed substrates to the solar wind. The Concentrator targets survived the hard landing upon return to Earth and were used to determine the isotopic composition of solar-wind—and hence solar—oxygen and nitrogen. Here we report on the flight operation of the instrument and on simulations of its performance. Concentration and fractionation patterns obtained from simulations are given for He, Li, N, O, Ne, Mg, Si, S, and Ar in SiC targets, and are compared with measured concentrations and isotope ratios for the noble gases. Carbon is also modeled for a Si target. Predicted differences in instrumental fractionation between elements are discussed. Additionally, as the Concentrator was designed only for ions ≤22 AMU, implications of analyzing elements as heavy as argon are discussed. Post-flight simulations of instrumental fractionation as a function of radial position on the targets incorporate solar-wind velocity and angular distributions measured in flight, and predict fractionation patterns for various elements and isotopes of interest. A tighter angular distribution, mostly due to better spacecraft spin stability than assumed in pre-flight modeling, results in a steeper isotopic fractionation gradient between the center and the perimeter of the targets. Using the distribution of solar-wind velocities encountered during flight, which are higher than those used in pre-flight modeling, results in elemental abundance patterns slightly less peaked at the center. Mean fractionations trend with atomic mass, with differences relative to the measured isotopes of neon of +4.1±0.9 ‰/amu for Li, between ?0.4 and +2.8 ‰/amu for C, +1.9±0.7‰/amu for N, +1.3±0.4 ‰/amu for O, ?7.5±0.4 ‰/amu for Mg, ?8.9±0.6 ‰/amu for Si, and ?22.0±0.7 ‰/amu for S (uncertainties reflect Monte Carlo statistics). The slopes of the fractionation trends depend to first order only on the relative differential mass ratio, Δm/m. This article and a companion paper (Reisenfeld et al. 2012, this issue) provide post-flight information necessary for the analysis of the Genesis solar wind samples, and thus serve to complement the Space Science Review volume, The Genesis Mission (v. 105, 2003). 相似文献
45.
Daniel Okoh Lee-Anne McKinnell Pierre Cilliers Pius Okeke 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
This paper presents the development of a Total Electron Content (TEC) map for the Nigerian ionosphere. In this work, TEC measurements obtained from the AFRL-SCINDA GPS (Air Force Research Laboratory-Scintillation Network Decision Aid, Global Positioning System) equipment installed at Nsukka (6.87°N, 7.38°E) are used to adapt the International Reference Ionosphere (IRI) model for the Nigerian Ionosphere. The map is being developed as a computer program (implemented in the MATLAB programming language) that shows spatial and temporal representations of TEC for the Nigerian ionosphere. The method is aimed at showing how the IRI model can be used to estimate VTEC over wide areas by incorporating GPS measurements. This method is validated by using GPS VTEC data collected from a station in Ilorin (8.50°N, 4.55°E). 相似文献
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48.
Nikos Mastrodemos Daniel G. Kubitschek Stephen P. Synnott 《Space Science Reviews》2005,117(1-2):95-121
The engineering goal of the Deep Impact mission is to impact comet Tempel 1 on July 4, 2005, with a 370 kg active Impactor
spacecraft (s/c). The impact velocity will be just over 10 km/s and is expected to excavate a crater approximately 20 m deep
and 100 m wide. The Impactor s/c will be delivered to the vicinity of Tempel 1 by the Flyby s/c, which is also the key observing
platform for the event. Following Impactor release, the Flyby will change course to pass the nucleus at an altitude of 500
km and at the same time slow down in order to allow approximately 800 s of observation of the impact event, ejecta plume expansion,
and crater formation. Deep Impact will use the autonomous optical navigation (AutoNav) software system to guide the Impactor
s/c to intercept the nucleus of Tempel 1 at a location that is illuminated and viewable from the Flyby. The Flyby s/c uses
identical software to determine its comet-relative trajectory and provide the attitude determination and control system (ADCS)
with the relative position information necessary to point the High Resolution Imager (HRI) and Medium Resolution Imager (MRI)
instruments at the impact site during the encounter. This paper describes the Impactor s/c autonomous targeting design and
the Flyby s/c autonomous tracking design, including image processing and navigation (trajectory estimation and maneuver computation).
We also discuss the analysis that led to the current design, the expected system performance as compared to the key mission
requirements and the sensitivity to various s/c subsystems and Tempel 1 environmental factors. 相似文献
49.
The present study aimed to document the psychometric properties of a recently declassified map reading test used in World War II, known as the Spatial Orientation Test (SOT), which measures mostly the ability to match map and aerial images. We also examined the influence of timing conditions and sex of the participants as correlates of performance. A total of 101 participants (41 males, 60 females) completed the SOT, along with other spatial tests and spatial affect scales (tapping spatial anxiety and confidence). Results showed a significant male advantage on this rediscovered map reading test. Additionally, timing affected overall performance but not the magnitude of sex differences. Finally, significant correlations were found between the SOT and other spatial tests and scales. The processes underlying this test and its potential for future use are discussed. 相似文献
50.
Paul Jaffe Jason HodkinForest Harrington Clark PersonMichael Nurnberger Bang NguyenSusie LaCava Dave ScheimanGrant Stewart Andrew HanEthan Hettwer Daniel Rhoades 《Acta Astronautica》2014
Space solar power (SSP) has been broadly defined as the collection of solar energy in space and its wireless transmission for use on earth. This approach potentially gives the benefit of provision of baseload power while avoiding the losses due to the day/night cycle and tropospheric effects that are associated with terrestrial solar power. Proponents have contended that the implementation of such systems could offer energy security, environmental, and technological advantages to those who would undertake their development. Among recent implementations commonly proposed for SSP, the modular symmetrical concentrator (MSC) and other modular concepts have received considerable attention. Each employs an array of modules for performing conversion of concentrated sunlight into microwaves or laser beams for transmission to earth. While prototypes of such modules have been designed and developed previously by several groups, none have been subjected to the challenging conditions inherent to the space environment and the possible solar concentration levels in which an array of modules might be required to operate. The research described herein details our team's efforts in the development of photovoltaic arrays, power electronics, microwave conversion electronics, and antennas for microwave-based “sandwich” module prototypes. The implementation status and testing results of the prototypes are reviewed. 相似文献