SkyWatch: A Passive Multistatic Radar Network for the Measurement of Object Position and Velocity

Author:

Randall Mitch12,Delacroix Alex2,Ezell Carson23,Kelderman Ezra2,Little Sarah24,Loeb Abraham25,Masson Eric2,Watters Wesley Andrés26,Cloete Richard2ORCID,White Abigail23

Affiliation:

1. Ascendant AI, Boulder, CO 80304, USA

2. Galileo Project, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02139, USA

3. Harvard University, 60 Garden Street, Cambridge, MA, 02138, USA

4. Scientific Coalition for UAP Studies, Fort Myers, FL 33913, USA

5. Astronomy Department, Harvard University, 60 Garden Street, Cambridge, MA 02138, USA

6. Whitin Observatory, Wellesley College, 106 Central Street, Wellesley, MA 02481, USA

Abstract

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’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 80[Formula: see text]km, horizontal distances up to 150[Formula: see text]km, and at velocities to [Formula: see text][Formula: see text]km/s ([Formula: see text][Formula: see text]Mach). 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–Smithsonian Center for Astrophysics (CfA), to validate full 3D position and velocity recovery. The experimental multistatic system intermittently records raw data for later processing to aid development. The results of the multistatic experiment will inform the design of a compact, economical receiver intended for deployment in a large-scale, mass-deployed mesh network. Such a network would greatly increase the probability of detecting and recording the movements of aerial objects with anomalous kinematics suggestive of Unidentified Aerial Phenomena (UAP).

Publisher

World Scientific Pub Co Pte Ltd

Subject

Astronomy and Astrophysics,Instrumentation

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