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Plug and Play Mission Operations 即插即用任务操作
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187394
T. Sorensen, E. Pilger, B. Yost, M. Nunes, J. Differding
Ongoing and planned smallsat programs within NASA, the DoD, and academia have indicated a need to be able to routinely and efficiently operate multiple small spacecraft in support of science and technology missions. However, as the number of these missions is expected to grow rapidly, the associated costs to develop and operate unique ground control stations, tools, and networks may become prohibitive to the sponsoring organizations or universities. In order to inform and raise the awareness of the smallsat space operations community, the University of Hawai'i, NASA Ames Research Center, San Jose State University (SJSU) and American Institure of Aeronautics and Astronautics (AIAA) held a workshop entitled Plug `n' Play Mission Operations (PPMO) which held May 16-17, 2011 at the SJSU campus in San Jose, California. The purpose of the workshop was to foster collaboration and leveraging of existing and developing capabilities that may be collectively utilized by the smallsat community for space operations. Although the emphasis of the workshop was on small satellites, many of the techniques discussed would be applicable to large spacecraft mission operations as well. The workshop explored the adoption of standards and existing capabilities as well as the creation of new technologies that will enable space mission developers to plan, design, and operate their spacecraft using a common architecture in order to reduce cost and overall mission risk. The PPMO workshop investigated the various needs of the smallsat communities (military, civil and educational space) and also touched on existing systems and capabilities (such as GSFC's GMSEC, JPL's AMMOS, and NRL's CGA used in the MC3 program) and those under development (such as HSFL's COSMOS and ESA's GENSO). The workshop also held facilitated discussions organized into categories along the lines of Approaches (programmatic and related issues), Implementation (technical solutions and architectures), and Applications (concept of operations, mission types and users). This paper presents the results of this workshop and the path forward.
美国宇航局、国防部和学术界正在进行和计划中的小卫星项目已经表明,需要能够常规和有效地操作多个小型航天器,以支持科学和技术任务。但是,由于这些特派团的数目预计将迅速增加,开发和操作独特地面控制站、工具和网络的相关费用可能会使赞助组织或大学望而却步。2011年5月16日至17日,夏威夷大学、美国宇航局艾姆斯研究中心、圣何塞州立大学(SJSU)和美国航空航天研究所(AIAA)在加州圣何塞的SJSU校园举办了一个名为“即插即播”任务操作(PPMO)的研讨会,以告知和提高小卫星空间操作社区的意识。讲习班的目的是促进协作和利用现有的和正在发展的能力,小卫星界可以将这些能力集体用于空间业务。虽然讲习班的重点是小型卫星,但所讨论的许多技术也将适用于大型航天器任务业务。讲习班探讨了标准和现有能力的采用以及新技术的创造,这些新技术将使空间任务开发人员能够使用通用架构规划、设计和操作其航天器,以降低成本和总体任务风险。PPMO研讨会调查了小卫星社区(军事、民用和教育空间)的各种需求,还涉及了现有系统和能力(如GSFC的GMSEC、JPL的AMMOS和NRL在MC3计划中使用的CGA)和正在开发的系统和能力(如HSFL的COSMOS和ESA的GENSO)。讲习班还进行了便利的讨论,按照方法(方案和有关问题)、执行(技术解决办法和结构)和应用(业务概念、任务类型和用户)等类别进行了讨论。本文介绍了本次研讨会的成果和未来的发展方向。
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引用次数: 4
A novel hyperspectral image clustering method based on spectral unmixing 一种基于光谱分解的高光谱图像聚类方法
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187196
Hamed Gholizadeh, Mohammad Javad Valdan Zoej, B. Mojaradi
In this paper, a novel hyperspectral image clustering procedure, which is based upon the Fully Constrained Least Squares (FCLS) spectral unmixing method, is proposed. The proposed clustering method consists of three major steps: endmember extraction, unmixing procedure and hardening process via the winner-takes-all approach. To estimate the optimal number of endmembers, instead of using the background signal subspace identification methods, the number of endmembers is varied in a predefined interval and the commonly accepted VCA (Vertex Component Analysis) algorithm is employed to extract the endmembers' spectra. At each iteration, the bandwise Root Mean Square Error (RMSE) between the reconstructed image, obtained from estimated fractions. and the original image is computed and the mean of all bandwise RMSEs is regarded as a measure to choose the optimum number of endmembers. Experiments conducted on the Indian Pines challenging dataset proved the superiority of proposed method over the K-Means and Fuzzy c-Means methods in terms of the widely used Adjusted Rand Index measure.
提出了一种基于全约束最小二乘(FCLS)光谱解混方法的高光谱图像聚类方法。本文提出的聚类方法包括三个主要步骤:端元提取、解混和硬化过程,采用赢者通吃的方法。为了估计最优端元数目,该方法不使用背景信号子空间识别方法,而是在预定义的区间内改变端元数目,并采用常用的VCA(顶点分量分析)算法提取端元光谱。在每次迭代中,从估计分数中获得重构图像之间的带向均方根误差(RMSE)。对原始图像进行计算,并将各带宽均方根值的平均值作为选择最优端元个数的度量。在Indian Pines具有挑战性的数据集上进行的实验证明,就广泛使用的调整后兰德指数度量而言,所提出的方法优于K-Means和模糊c-Means方法。
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引用次数: 1
LunarVader: Testing of a 1 meter lunar drill in a 3.5 meter vacuum chamber and in the Antarctic lunar analog site 月球维达者:在3.5米真空室和南极月球模拟地点测试1米月球钻
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187047
K. Zacny, G. Paulsen, B. Mellerowicz, J. Craft, Chris McKay, B. Glass, A. Davila, M. Marinova, W. Pollard
In this paper we report on the development of a rotary-percussive sampling drill, LunarVader. The purpose of the drill is to penetrate at least 1 meter in icy-regolith and acquire sub-surface sample for science analysis and for the In Situ Resource Utilization (ISRU). The drill was tested in a lunar analog site of the Ross Island, in the Antarctic and inside the 3.5 meter vacuum chamber in ice-bound JSC-1a lunar soil simulant. In both cases, the drill reached ~1 meter depth in approximately one hour. The average power was 100 Watts and Weight on Bit was less than 100 Newton. This corresponds to the drilling energy of 100 Whr. In each case approximately 500 grams of sample was recovered and autonomously deposited into a sterile bag.
在本文中,我们报告了一种旋转冲击取样钻机,月球维达的发展。钻探的目的是在冰层中穿透至少1米,获取地下样本,用于科学分析和就地资源利用(ISRU)。该钻头在罗斯岛的一个月球模拟地点、南极和3.5米的JSC-1a月球土壤模拟冰室中进行了测试。在这两种情况下,钻头在大约一个小时内达到了1米深。平均功率为100瓦,重量小于100牛顿。这相当于100瓦时的钻井能量。在每个案例中,大约500克样品被回收并自动存入无菌袋中。
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引用次数: 9
Compressive quantization versus compressive sampling in image digitization 图像数字化中的压缩量化与压缩采样
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187166
Y. Poberezhskiy
Digital image compression reduces the bandwidth, time, and energy needed for transmission of images and signals, as well as memory needed for their storage. However, it cannot solve the digitization problems. Recently proposed compressive sampling (or sensing) solves these problems by reducing the average number of projections required for representing images and signals through exploiting their sparsity. An alternative approach named compressive quantization solves identical problems by reducing the average number of bits required for the same purpose. It exploits statistical properties of images and signals, as well as specific features of quantizers. In this paper, the analysis and further development of compressive quantization used for digitization of images is combined with its comparison to compressive sampling. It is shown that compressive quantization simplifies the image digitization more significantly and provides more effective and less distorting compression than compressive sampling. Its practical realization is much easier than that of compressive sampling. The root causes of these advantages are revealed.
数字图像压缩减少了传输图像和信号所需的带宽、时间和能量,以及存储图像和信号所需的内存。然而,它并不能解决数字化问题。最近提出的压缩采样(或传感)通过利用图像和信号的稀疏性来减少表示图像和信号所需的投影的平均数量,从而解决了这些问题。另一种称为压缩量化的方法通过减少相同目的所需的平均比特数来解决相同的问题。它利用图像和信号的统计特性,以及量化器的特定特性。本文对用于图像数字化的压缩量化进行了分析和进一步发展,并与压缩采样进行了比较。结果表明,压缩量化比压缩采样更显著地简化了图像数字化,提供了更有效、更少失真的压缩。它的实际实现比压缩采样容易得多。揭示了这些优势的根本原因。
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引用次数: 1
Practical steps for patenting software post Bilski 专利软件后比尔斯基的实际步骤
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187446
G. R. Rapacki
The US Supreme Court's holding in Bilski v Kappos limits software developers attempting to patent inventions using method claims. The Bilski holding limited the scope of business method patents to those that claim a method hosted on a machine or those that effect a transformation of a particular article into a different state or thing. While today's scope of method claims is more limited than before Bilski, inventors can still effectively patent software inventions. This paper presents practical suggestions for patenting software inventions described by a method claim. The Supreme Court's holding is discussed, then using a scenario of an interest in patenting a method of finding the roots of a polynomial, several claim formats will be reviewed.
美国最高法院在Bilski诉Kappos案中的裁决限制了软件开发者试图利用方法权利要求为发明申请专利。Bilski案将商业方法专利的范围限制在那些声称在机器上托管的方法或那些将特定物品转化为不同状态或事物的方法。虽然今天的方法权利要求范围比Bilski之前更有限,但发明者仍然可以有效地为软件发明申请专利。本文提出了对方法权利要求所描述的软件发明实施专利的实用建议。讨论了最高法院的裁决,然后使用对寻找多项式根的方法申请专利感兴趣的场景,将审查几种权利要求格式。
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引用次数: 0
Cognitive bias in the verification and validation of space flight systems 航天飞行系统验证中的认知偏差
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187404
Steven. A. Larson, Steven. A. Larson
Cognitive bias is generally recognized as playing a significant role in virtually all domains of human decision making. Insight in to this role is informally built in to many of the system engineering practices employed in the aero space industry. The review process, for example, typically has features that help to counteract the effect of bias. This paper presents a discussion of how commonly recognized biases may affect the verification and validation process. Verifying and validating a system is arguably more challenging than development, both technically and cognitively. Whereas there may be a relatively limited number of options available for the design of a particular aspect of a system, there is a virtually unlimited number of potential verification scenarios that may be explored. The probability of any particular scenario occurring in operations is typically very difficult to estimate, which increases reliance on judgment that may be affected by bias. Implementing a verification activity often presents technical challenges that, if they can be overcome at all, often result in a departure from actual flight conditions (e.g., 1-g testing, simulation, time compression, artificial fault injection) that may raise additional questions about the meaningfulness of the results, and create opportunities for the introduction of additional biases. In addition to mitigating the biases it can introduce directly, the verification and validation process must also overcome the cumulative effect of biases introduced during all previous stages of development. A variety of cognitive biases will be described, with research results for illustration. A handful of case studies will be presented that show how cognitive bias may have affected the verification and validation process on recent JPL flight projects, identify areas of strength and weakness, and identify potential changes or additions to commonly used techniques that could provide a more robust verification and validation of future systems.
人们普遍认为,认知偏见在人类决策的几乎所有领域都发挥着重要作用。对这个角色的洞察是在航空航天工业中采用的许多系统工程实践中非正式地建立起来的。例如,审查过程通常具有有助于抵消偏见影响的特征。本文介绍了如何普遍认识的偏见可能会影响验证和确认过程的讨论。无论在技术上还是在认知上,验证和确认系统都可以说比开发更具挑战性。尽管对于系统的某个特定方面的设计,可用的选项可能相对有限,但实际上可以探索的潜在验证场景数量是无限的。在操作中发生任何特定情况的可能性通常很难估计,这增加了对可能受偏见影响的判断的依赖。实现验证活动通常会提出技术挑战,如果能够克服这些挑战,通常会导致偏离实际飞行条件(例如,1-g测试、模拟、时间压缩、人工故障注入),这可能会对结果的意义提出额外的问题,并为引入额外的偏差创造机会。除了减轻它可以直接引入的偏差之外,验证和确认过程还必须克服在所有先前开发阶段引入的偏差的累积效应。各种认知偏差将被描述,并以研究结果为例。将展示一些案例研究,展示认知偏差如何影响最近JPL飞行项目的验证和验证过程,确定优势和劣势领域,并确定对常用技术的潜在更改或补充,这些技术可以为未来系统提供更强大的验证和验证。
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引用次数: 1
Mars Ascent Vehicle system studies and baseline conceptual design 火星上升飞行器系统研究和基线概念设计
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187297
M. Trinidad, E. Zabrensky, A. Sengupta
The Mars Ascent Vehicle (MAV) is a critical mission element of the Mars Sample Return campaign that delivers the Martian sample from Mars surface to orbit for rendezvous with retrieving spacecraft and sample return to earth. The MAV design presents significant challenges in that it must fit in the Lander mission architecture, have a minimized total system mass (MAV and igloo/erector support system) with a mass goal of less than 360 kg, and deliver the 5 kg Martian sample payload to a 460 to 580km orbit. The MAV must also withstand the harsh Mars thermal environment for up to 9 months where power consumption for thermal conditioning and operation further impacts the mass allocation to the MAV. Northrop Grumman Aerospace Systems, in collaboration with NASA GRC and JPL, conducted a MAV system study and component definition under a National Research Announcement, NASA In-Space Propulsion program. The study investigated a two-stage liquid propulsion concept, an optimized MAV trajectory, guidance, navigation, and control, thermal requirements, MAV components, and MAV support systems. The results of the study and baseline MAV system design are presented in this report.
火星上升飞行器(MAV)是火星样本返回任务的关键任务,它将火星样本从火星表面运送到轨道上,与回收航天器交会,并将样本返回地球。MAV设计提出了重大挑战,因为它必须适应着陆器任务架构,具有最小的总系统质量(MAV和冰屋/直立支撑系统),质量目标小于360公斤,并将5公斤的火星样本有效载荷送到460至580公里的轨道上。MAV还必须承受火星恶劣的热环境长达9个月,热调节和操作的功耗进一步影响了MAV的质量分配。诺斯罗普·格鲁曼航天系统公司与NASA GRC和JPL合作,根据NASA太空推进计划的国家研究公告进行了MAV系统研究和组件定义。该研究研究了两级液体推进概念、优化的MAV轨迹、制导、导航和控制、热要求、MAV组件和MAV支持系统。本报告介绍了研究结果和基线MAV系统设计。
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引用次数: 9
Sub-arcsecond performance of the ST5000 star tracker on a balloon-borne platform ST5000星跟踪器在气球载平台上的亚弧秒性能
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187179
E. Young, R. Mellon, J. Percival, K. Jaehnig, J. Fox, T. Lachenmeier, B. Oglevie, M. Bingenheimer
The ST5000 is a star tracker developed at the University of Wisconsin and used in NASA's sounding rocket payloads. In order to demonstrate the ST5000's suitability for pointed balloon-borne telescopes, we flew an ST5000 on a stratospheric balloon on May 6, 2011. This flight addressed our four basic questions: will the ST5000 work from 120,000 ft (it does), what was the rms performance (about 0.6"), what angular rates of motion would cause the ST5000 to fail (greater than 0.5 degrees/sec) and could the ST5000 serve as a daytime star tracker (not without modifications). We will briefly present the results from the flight and describe the ST5000's quantitative performance. We will also describe the problems with background light as a function of wavelength, altitude and angle from the Sun. We will discuss approaches to improve the daytime performance using infrared detectors and longer focal lengths/reduced platescales. Solutions that have finer platescales have the potential to improve the star tracker's error signal to the 0.1" level, which is better than the diffraction limit of a one meter telescope at 5000 Å.
ST5000是威斯康星大学开发的一种恒星追踪器,用于美国宇航局的探空火箭有效载荷。为了证明ST5000对尖气球望远镜的适用性,我们在2011年5月6日将ST5000放在平流层气球上飞行。这次飞行解决了我们的四个基本问题:ST5000将从120,000英尺工作(它确实),什么是rms性能(约0.6“),运动的角速度会导致ST5000失败(大于0.5度/秒),ST5000可以作为白天的星跟踪器(不是没有修改)。我们将简要介绍飞行结果,并描述ST5000的定量性能。我们还将描述背景光作为波长、高度和与太阳的角度的函数的问题。我们将讨论使用红外探测器和更长的焦距/缩小的平板来提高白天性能的方法。具有更细刻度的解决方案有可能将星跟踪器的误差信号提高到0.1“水平,这比1米望远镜在5000 Å的衍射极限要好。
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引用次数: 10
Deep Space Climate Observatory: The DSCOVR mission 深空气候观测站:DSCOVR任务
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187025
J. Burt, Bob Smith
In 1998, then-Vice President Al Gore proposed a mission to the Earth-Sun first Lagrange point (L1) to observe the Earth as a planet. This mission was named Triana, after the lookout on Christopher Columbus's fleet who is reputedly the first of the European explorers to see the new world. Triana mission development proceeded for 21 months and cost an estimated $249M (in FY07$) before it was de-manifested from the Space Shuttle. The spacecraft has been in a state of “Stable Suspension” since November 2001. After the mission was placed into suspension, it was renamed the Deep Space Climate Observatory (DSCOVR). This paper will cover an overview of the original mission and highlights of refurbishing this mission to launch 16 years after it started, plus an update on its currently planned mission architecture.
1998年,当时的副总统戈尔提出了一项前往地球-太阳第一个拉格朗日点(L1)的任务,将地球作为一颗行星来观察。这次任务被命名为特里亚纳,以克里斯托弗·哥伦布舰队的了望者命名,据说他是第一个看到新世界的欧洲探险家。特里亚纳任务的开发进行了21个月,估计花费了2.49亿美元(2007财年美元),然后才从航天飞机上卸下。自2001年11月以来,该航天器一直处于“稳定悬浮”状态。任务中止后,它被重新命名为深空气候观测站(DSCOVR)。本文将概述最初的任务,重点介绍在启动16年后对该任务进行翻新,并对其目前计划的任务架构进行更新。
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引用次数: 59
A new fuzzy CFAR processor for radar MTD systems 雷达MTD系统中一种新型模糊CFAR处理器
Pub Date : 2012-03-03 DOI: 10.1109/AERO.2012.6187140
H. El-Henawy, E. Abdoul-Fattah, M. Gamal, M. Attala, A. Hafez
This paper proposes a new fuzzy constant false alarm processor (FCFAR) for radar MTD systems. The proposed amplitude processor decides the fixed threshold value for the CFAR using fuzzy logic controller according three input variables. First input is the fast threshold from fifty serially averaged range cells. The second is the slow threshold from concatenated 500 averaged range cells. The third input is the signal to noise ratio at the RF stage of the radar system. The proposed processor is simulated under Matlab program environment on 1 million range cells data in additive white Gaussian noise (AWGN) with non-homogeneous background clutter and from 5 to 30 dB signal to noise ratio (S/N). The results show the superiority of the proposed FCFAR than the traditional systems used during the last decade.
提出了一种新的用于雷达MTD系统的模糊恒值虚警处理器(FCFAR)。该幅值处理器利用模糊控制器根据三个输入变量确定CFAR的固定阈值。第一个输入是50个连续平均距离单元的快速阈值。第二种是从连接的500个平均范围单元中获得的慢阈值。第三个输入是雷达系统射频级的信噪比。在Matlab编程环境下,对100万个距离单元数据在非均匀背景杂波加性高斯白噪声(AWGN)和5 ~ 30 dB信噪比(S/N)条件下进行了仿真。结果表明,所提出的FCFAR比过去十年中使用的传统系统具有优越性。
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引用次数: 4
期刊
2012 IEEE Aerospace Conference
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