2001 Mars Odyssey Mission Summary

The 2001 Mars Odyssey spacecraft, now in orbit at Mars, will observe the Martian surface at infrared and visible wavelengths to determine surface mineralogy and morphology, acquire global gamma ray and neutron observations for a full Martian year, and study the Mars radiation environment from orbit. The science objectives of this mission are to: (1) globally map the elemental composition of the surface, (2) determine the abundance of hydrogen in the shallow subsurface, (3) acquire high spatial and spectral resolution images of the surface mineralogy, (4) provide information on the morphology of the surface, and (5) characterize the Martian near-space radiation environment as related to radiation-induced risk to human explorers. To accomplish these objectives, the 2001 Mars Odyssey science payload includes a Gamma Ray Spectrometer (GRS), a multi-spectral Thermal Emission Imaging System (THEMIS), and a radiation detector, the Martian Radiation Environment Experiment (MARIE). THEMIS and MARIE are mounted on the spacecraft with THEMIS pointed at nadir. GRS is a suite of three instruments: a Gamma Subsystem (GSS), a Neutron Spectrometer (NS) and a High-Energy Neutron Detector (HEND). The HEND and NS instruments are mounted on the spacecraft body while the GSS is on a 6-m boom. Some science data were collected during the cruise and aerobraking phases of the mission before the prime mission started. THEMIS acquired infrared and visible images of the Earth-Moon system and of the southern hemisphere of Mars. MARIE monitored the radiation environment during cruise. The GRS collected calibration data during cruise and aerobraking. Early GRS observations in Mars orbit indicated a hydrogen-rich layer in the upper meter of the subsurface in the Southern Hemisphere. Also, atmospheric densities, scale heights, temperatures, and pressures were observed by spacecraft accelerometers during aerobraking as the spacecraft skimmed the upper portions of the Martian atmosphere. This provided the first in-situ evidence of winter polar warming in the Mars upper atmosphere. The prime mission for 2001 Mars Odyssey began in February 2002 and will continue until August 2004. During this prime mission, the 2001 Mars Odyssey spacecraft will also provide radio relays for the National Aeronautics and Space Administration (NASA) and European landers in early 2004. Science data from 2001 Mars Odyssey instruments will be provided to the science community via NASA’s Planetary Data System (PDS). The first PDS release of Odyssey data was in October 2002; subsequent releases occur every 3 months.     

The global positioning system: policy issues for an information technology

This article, based on the executive summary of a RAND Corporation study, analyses the policy issues facing the USA in the use of its Global Positioning System (GPS), in terms of both national security and commercial applications. Foreign policy issues, including how to react to the emergence of non-US (Russian, European and Inmarsat-sponsored) alternatives to the GPS are also examined. The article concludes with a series of recommendations for policy makers. Reprinted by permission.     

Disaster monitoring and mitigation using aerospace technologies and integrated telecommunication networks

How space technologies and new integrated telecommunication networks can mitigate the impact of natural and man-made disasters. The objective is to design new, potentially attractive telecommunication architectures to better manage a disaster scenario. The strengths and the weaknesses of the proposed space-based telecommunication architectures for the emergency and recovery will be outlined also, to individuate the needs for an optimal provision of information and accessibility of space-related services in case of disaster.     

Challenges to US space sustainability

With space now crucial to such a wide range of activities on Earth, the USA must ensure the sustainability of its efforts, a task that involves technological feasibility and political will. Near-term challenges include US human access to space and the Shuttle transition, funding NASA sufficiently in a time of recession, and rebuilding the country's space industrial base. Longer-term challenges will be better protecting the space environment (including the electromagnetic spectrum) from overcrowding and the effects of space weather and NEOs, and defining responsibilities for distributing climate change data and recognition of property rights for the commercial development of in-space resources. As an aid to dealing with these challenges the USA must ask itself whether there is a human future in space and seek to answer the question in the course of human and robotic exploration beyond Earth.     

Photochemical synthesis of citric acid cycle intermediates based on titanium dioxide

The emergence of the citric acid cycle is one of the most remarkable occurrences with regard to understanding the origin and evolution of metabolic pathways. Although the chemical steps of the cycle are preserved intact throughout nature, diverse organisms make wide use of its chemistry, and in some cases organisms use only a selected portion of the cycle. However, the origins of this cycle would have arisen in the more primitive anaerobic organism or even back in the proto-metabolism, which likely arose spontaneously under favorable prebiotic chemical conditions. In this context, we report that UV irradiation of formamide in the presence of titanium dioxide afforded 6 of the 11 carboxylic acid intermediates of the reductive version of the citric acid cycle. Since this cycle is the central metabolic pathway of contemporary biology, this report highlights the role of photochemical processes in the origin of the metabolic apparatus.     

Relative targeting architectures for captive-carry HIL missilesimulator experiments

Captive-carry electronic warfare (EW) tests evaluate the response of hardware-in-the-loop (HIL) missile seekers to an actual environment (test-range) including the presence of electronic attack. This paper describes a relative targeting architecture that displays the test-range results in geodetic coordinates using only the sensors available on board the captive-carry platform (GPS, INS, seekers). To derive the target position in geodetic coordinates, a lever-arm correction process is described that determines the position of each seeker and the corresponding pitch and yaw of the simulator. Combining the positional parameters of the seeker with its targeting variables, the seeker track point is displayed in geodetic coordinates, A track tagging algorithm is presented to identify the true target from the EW disruption using the drift angle from the inertial navigation system (INS), To eliminate the scintillation noise present in the track image, a Kalman filter in sensor coordinates is applied to the targeting variables allowing optimization of the track tagging. Experimental results from a recent EW field test using antiship cruise missile simulators are shown to demonstrate the feasibility of the approach for determining EW effectiveness in near real-time. Targeting accuracy is also quantified by comparing the derived target position with the true Global Positioning System (GPS) test-range position of the ship in the absence of electronic attack     

False alarm analysis of the envelope detection GO-CFAR processor

The greatest of constant false alarm rate processor (GO CFAR) is a useful architecture for adaptively setting a radar detection threshold in the presence of clutter edges. The GO CFAR input is often the envelope detected in-phase (I) and quadrature (Q) channels of the baseband signal (x_e=√(I²+Q²)). This envelope detection can also be approximated using x=a max{|I|,|Q|}+b min{|I|,|Q|} which requires less complex hardware (a and b are simple multiplying coefficients). The envelope GO CFAR processor and several envelope approximation GO CFAR processors are compared in terms of the probability of false alarm (PFA) performance. Closed-form expressions which describe the PFA performance are given and their accuracy evaluated. It is shown that for all cases, the PFA is proportional to the number of reference cells n for small threshold multiplier T and inversely proportional to n for large T. A region of intersection occurs where the PFA is the same for two different values of n. For example, at T'=1.68 in the |I|+|Q| GO CFAR (a=1, b=1) the PFA for n=1 is equal to the optimal n=∞ fixed-threshold PFA (PFA=0.112)     

低截获概率雷达的特征和机载系统

1 低截获概率雷达的特征 许多组合特性有助于防止低截获概率（LPI）雷达被现代截获接收机探测到。这些特性集中在天线（天线方向图和扫描图形）和发射机（辐射波形）中。     

Combination methods of tropospheric time series

In this article we present two methods for combination of different Global Navigation Satellite Systems (GNSS) Zenith Total Delay (ZTD) time-series for the same GNSS site, but from different producers or different processing setups. One method has been setup at ASI/CGS, the other at KNMI. Using Near Real-Time (NRT) ZTD data covering 1 year from the E-GVAP project, the performance of the two methods is inter-compared and validation is made against a combined ZTD solution from EUREF, based on post-processed ZTDs. Further, validation of the ASI combined solutions is made against independent ZTDs derived from radiosonde, Numerical Weather Prediction (NWP) model and Very Long Baseline Interferometry (VLBI) ZTD.