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ARIES ST Radar: The first Central Himalayan wind profiler ARIES ST雷达:第一个喜马拉雅中部风廓线仪
IF 1.3 Q2 Physics and Astronomy Pub Date : 2023-02-16 DOI: 10.1142/s2251171722400050
S. Bhattacharjee, M. Naja, A. Jaiswal, K. Rawat, R. Sagar, S. Ananthakrishnan
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引用次数: 0
Detection of Moving Objects in Earth Observation Satellite Images 对地观测卫星图像中运动物体的检测
IF 1.3 Q2 Physics and Astronomy Pub Date : 2023-01-17 DOI: 10.1142/s225117172340007x
E. Keto, W. Watters
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引用次数: 0
L Band Phased Array Feed Noise Figure and Radiation Efficiency Measurement with the Antenna Y Factor Method 天线Y因子法测量L波段相控阵馈电噪声图及辐射效率
IF 1.3 Q2 Physics and Astronomy Pub Date : 2023-01-17 DOI: 10.1142/s2251171723500022
M. Burnett, David Buck, Nathaniel Ashcraft, Spencer M. Ammermon, B. Jeffs, K. Warnick
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引用次数: 1
An Image Auto-Guider System for Kodaikanal Tower Tunnel Telescope Kodaikanal塔式隧道望远镜图像自动导引系统
IF 1.3 Q2 Physics and Astronomy Pub Date : 2023-01-17 DOI: 10.1142/s2251171723500034
H. Mathur, K. C. Thulasidharen, H. Pruthvi, K. Nagaraju, M. Rajalingam
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引用次数: 0
The Scientific Investigation of Unidentified Aerial Phenomena (UAP) Using Multimodal Ground-based Observatories 利用多模式地面观测站对不明空中现象(UAP)进行科学调查
IF 1.3 Q2 Physics and Astronomy Pub Date : 2023-01-12 DOI: 10.1142/S2251171723400068
W. Watters, A. Loeb, F. Laukien, Richard Cloete, A. Delacroix, Sergei Dobroshinsky, Benjamin Horvath, Ezra Kelderman, Sarah Little, Eric Masson, Andy Mead, M. Randall, Forrest Schultz, Matthew Szenher, F. Vervelidou, Abigail White, A. Ahlstrom, Carol Cleland, S. Dockal, N. Donahue, Mark Elowitz, Carson Ezell, Alex Gersznowicz, Nicholas Gold, Michael G. Hercz, E. Keto, K. Knuth, A. Lux, G. Melnick, A. Moro-Martin, J. Martín‐Torres, Daniel Llusa Ribes, P. Sail, M. Teodorani, J. Tedesco, Gerald Thomas Tedesco, M. Tu, M. Zorzano
(Abridged) Unidentified Aerial Phenomena (UAP) have resisted explanation and have received little formal scientific attention for 75 years. A primary objective of the Galileo Project is to build an integrated software and instrumentation system designed to conduct a multimodal census of aerial phenomena and to recognize anomalies. Here we present key motivations for the study of UAP and address historical objections to this research. We describe an approach for highlighting outlier events in the high-dimensional parameter space of our census measurements. We provide a detailed roadmap for deciding measurement requirements, as well as a science traceability matrix (STM) for connecting sought-after physical parameters to observables and instrument requirements. We also discuss potential strategies for deciding where to locate instruments for development, testing, and final deployment. Our instrument package is multimodal and multispectral, consisting of (1) wide-field cameras in multiple bands for targeting and tracking of aerial objects and deriving their positions and kinematics using triangulation; (2) narrow-field instruments including cameras for characterizing morphology, spectra, polarimetry, and photometry; (3) passive multistatic arrays of antennas and receivers for radar-derived range and kinematics; (4) radio spectrum analyzers to measure radio and microwave emissions; (5) microphones for sampling acoustic emissions in the infrasonic through ultrasonic frequency bands; and (6) environmental sensors for characterizing ambient conditions (temperature, pressure, humidity, and wind velocity), as well as quasistatic electric and magnetic fields, and energetic particles. The use of multispectral instruments and multiple sensor modalities will help to ensure that artifacts are recognized and that true detections are corroborated and verifiable.
(节录)75年来,不明空中现象(UAP)一直难以得到解释,也很少得到正式的科学关注。伽利略项目的一个主要目标是建立一个集成的软件和仪器系统,用于对空中现象进行多模态普查并识别异常。在这里,我们提出了UAP研究的主要动机,并解决了历史上对这项研究的反对意见。我们描述了一种在我们的普查测量的高维参数空间中突出异常事件的方法。我们提供详细的路线图来决定测量需求,以及科学可追溯性矩阵(STM),用于将受欢迎的物理参数与可观测值和仪器要求联系起来。我们还讨论了决定在哪里定位用于开发、测试和最终部署的仪器的潜在策略。我们的仪器包是多模态和多光谱的,包括:(1)多波段的宽视场相机,用于瞄准和跟踪空中物体,并使用三角测量法获得它们的位置和运动学;(2)窄视场仪器,包括用于表征形貌、光谱、偏振法和光度法的照相机;(3)用于雷达衍生距离和运动学的无源多静态天线和接收机阵列;(四)无线电频谱分析仪,用于测量无线电和微波发射;(5)通过超声波频段对次声发射进行采样的传声器;(6)用于表征环境条件(温度、压力、湿度和风速)、准静态电场和磁场以及高能粒子的环境传感器。多光谱仪器和多种传感器模式的使用将有助于确保识别人工制品,并证实和核实真实的检测结果。
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引用次数: 1
SkyWatch: A Passive Multistatic Radar Network for the Measurement of Object Position and Velocity SkyWatch:用于测量物体位置和速度的无源多基地雷达网络
IF 1.3 Q2 Physics and Astronomy Pub Date : 2022-12-08 DOI: 10.1142/S2251171723400044
M. Randall, A. Delacroix, Carson Ezell, Ezra Kelderman, Sarah Little, A. Loeb, Eric Masson, W. Watters, Richard Cloete, A. White
(Abridged) Quantitative three-dimensional (3D) position and velocity estimates obtained by passive radar will assist the Galileo Project in the detection and classification of aerial objects by providing critical measurements of range, location, and kinematics. These parameters will be combined with those derived from the Project{textquoteright}s suite of electromagnetic sensors and used to separate known aerial objects from those exhibiting anomalous kinematics. SkyWatch, a passive multistatic radar system based on commercial broadcast FM radio transmitters of opportunity, is a network of receivers spaced at geographical scales that enables estimation of the 3D position and velocity time series of objects at altitudes up to 80km, horizontal distances up to 150km, and at velocities to {textpm}2{textpm}2km/s ({textpm}6{textpm}6Mach). The receivers are designed to collect useful data in a variety of environments varying by terrain, transmitter power, relative transmitter distance, adjacent channel strength, etc. In some cases, the direct signal from the transmitter may be large enough to be used as the reference with which the echoes are correlated. In other cases, the direct signal may be weak or absent, in which case a reference is communicated to the receiver from another network node via the internet for echo correlation. Various techniques are discussed specific to the two modes of operation and a hybrid mode. Delay and Doppler data are sent via internet to a central server where triangulation is used to deduce time series of 3D positions and velocities. A multiple receiver (multistatic) radar experiment is undergoing Phase 1 testing, with several receivers placed at various distances around the Harvard{textendash}Smithsonian Center for Astrophysics (CfA), to validate full 3D position and velocity recovery.
(摘要)被动雷达获得的定量三维位置和速度估计将通过提供距离、位置和运动学的关键测量,帮助伽利略项目探测和分类空中物体。这些参数将与项目电磁传感器套件中得出的参数相结合,用于将已知的航空物体与表现出异常运动学的物体分离。SkyWatch是一种基于商业广播调频无线电发射机的无源多基地雷达系统,是一个在地理尺度上间隔开的接收器网络,能够估计高度高达80公里、水平距离高达150公里、速度高达2公里/秒(6马赫)的物体的3D位置和速度时间序列。接收器被设计为在因地形、发射器功率、相对发射器距离、相邻信道强度等而变化的各种环境中收集有用的数据。在一些情况下,来自发射器的直接信号可能足够大,可以用作回波相关的参考。在其他情况下,直接信号可能较弱或不存在,在这种情况下,参考通过互联网从另一个网络节点传送到接收器,用于回声相关性。针对两种操作模式和混合模式讨论了各种技术。延迟和多普勒数据通过互联网发送到中央服务器,在那里三角测量用于推断3D位置和速度的时间序列。一个多接收器(多基地)雷达实验正在进行第一阶段测试,在哈佛史密森天体物理中心(CfA)周围的不同距离放置了几个接收器,以验证完整的3D位置和速度恢复。
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引用次数: 2
Cumulative Author Index — Volume 11 (2022) 累积作者指数——第11卷(2022)
IF 1.3 Q2 Physics and Astronomy Pub Date : 2022-12-01 DOI: 10.1142/s225117172299001x
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引用次数: 0
ARIES 130-cm Devasthal Fast Optical Telescope - Operation and Outcome 白羊座130厘米毁灭性快速光学望远镜-操作和结果
IF 1.3 Q2 Physics and Astronomy Pub Date : 2022-11-24 DOI: 10.1142/s2251171722400049
Y. Joshi, T. Bangia, M. Jaiswar, J. Pant, K. Reddy, S. Yadav
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引用次数: 4
First Light Preparations of the 4m ILMT 4m ILMT的首光准备
IF 1.3 Q2 Physics and Astronomy Pub Date : 2022-11-16 DOI: 10.1142/s2251171722400037
B. Kumar, H. Kumar, Khushal Singh Dangwal, Himanshu Rawat, K. Misra, Vibhore Negi, M. Jaiswar, Naveen Dukiya, B. Ailawadhi, P. Hickson, J. Surdej
The 4[Formula: see text]m International Liquid Mirror Telescope (ILMT) is a zenith-pointing optical observing facility at ARIES Devasthal observatory (Uttarakhand, India). The first light preparatory activities of the ILMT were accomplished in April 2022 followed by on-sky tests that were carried out at the beginning of May 2022. This telescope will perform a multi-band optical (SDSS [Formula: see text], [Formula: see text] and [Formula: see text]) imaging of a narrow strip ([Formula: see text]) of sky utilizing the time-delayed integration technique. Single-scan ILMT images have an integration time of 102[Formula: see text]s and consecutive-night images can be co-added to further improve the signal-to-noise ratio. An image subtraction technique will also be applied to the nightly recorded observations in order to detect transients, objects exhibiting variations in flux or position. Presently, the facility is in the commissioning phase and regular operation will commence in March 2023. This paper presents a discussion of the main preparation activities before first light, along with preliminary results obtained.
4[公式:见正文]m国际液镜望远镜(ILMT)是ARIES Devasthal天文台(印度北阿坎德邦)的一个指向天顶的光学观测设施。ILMT的第一次灯光准备活动于2022年4月完成,随后于2022年5月初进行了天空测试。该望远镜将利用时间延迟积分技术对天空的窄带([公式:见正文])进行多波段光学成像(SDSS[公式:参见正文]、[公式:请见正文]和[公式:详见正文])。单次扫描ILMT图像的积分时间为102[公式:见正文],可以共同添加连续的夜间图像,以进一步提高信噪比。图像相减技术也将应用于夜间记录的观测,以检测瞬态,即通量或位置变化的物体。目前,该设施正处于调试阶段,将于2023年3月开始正常运行。本文讨论了初亮前的主要准备活动,以及获得的初步结果。
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引用次数: 8
Parameters of a short dipole antenna placed over a two-layer lunar soil 放置在两层月球土壤上的短偶极天线的参数
IF 1.3 Q2 Physics and Astronomy Pub Date : 2022-11-14 DOI: 10.1142/s2251171723500010
P. Tokarsky
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引用次数: 1
期刊
Journal of Astronomical Instrumentation
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