Underwater Celestial Navigation Using the Polarization of Light Fields

Global-scale underwater navigation presents challenges that modern technology has not solved. Current technologies drift and accumulate errors over time (inertial measurement), are accurate but short-distance (acoustic), or do not sufficiently penetrate the air-water interface (radio and GPS). To address these issues, I have developed a new mode of underwater navigation based on the passive observation of patterns in the polarization of in-water light. These patterns can be used to infer the sun__s relative position, which enables the use of celestial navigation in the underwater environment. I have developed an underwater polarization video camera based on a bio-inspired polarization image sensor and the image processing and inference algorithms for estimating the sun__s position. My system estimates heading with RMS error of 6.02_ and global position with RMS error of 442 km. Averaging experimental results from a single site yielded a 0.38_ heading error and a 61 km error in global position. The instrument can detect changes in polarization due to a 0.31_ movement of the sun, which corresponds to 35.2 km of ground movement, with 99% confidence. This technique could be used by underwater vehicles for long-distance navigation and suggests additional ways that marine animals with polarization-sensitive vision could perform both local and long-distance navigation

Biologically Inspired Navigational Strategies Using Atmospheric Scattering Patterns

A source of accurate and reliable heading is vital for the navigation of autonomous systems such as micro-air vehicles (MAVs). It is desirous that a passive computationally efficient measure of heading is available even when magnetic heading is not. To confront this scenario, a biologically inspired methodology to determine heading based on atmospheric scattering patterns is proposed. A simplified model of the atmosphere is presented, and a hardware analog to the insect Dorsal Rim Area (DRA) photodetection is introduced. Several algorithms are developed to map the patterns of polarized and unpolarized celestial light to heading relative to the sun. Temporal information is used to determine current solar position, and then merged with solar relative heading resulting in absolute heading. Simulation and outdoor experimentation are used to validate the proposed heading determination methodology. Celestial heading measurements are shown to provide closed loop heading control of a ground based robot

Instrumentations to investigate magnetoreception in homing pigeons (Columba livia)

Seasonal migration of birds from one place to another is a very complex phenomenon investigated by researchers for many years. Birds move from one area to other often covering thousands of kilometres, and some species even fly only at night. In order to find the proper direction and their way to specific areas, birds use many cues, which can vary, for example objects that can be seen, smell or the perception of other environmental features. The type of cue depends upon whether the birds have to travel a short distance or if they have to travel to distant locations. The cues for birds, which migrate at day time, are rather different from those who travel at night. The first chapter of this thesis covers details of the strategies that pigeons use when homing and the interplay of the various navigation cues used. Various experiments have been carried out on pigeons but the results are quite complex. However, previous experiments have demonstrated that pigeons have the ability to use geomagnetism as a reference in order to find their way. The inclination and intensity of the field vector are both used as references. In this PhD research, I mainly focused on getting an answer whether homing pigeons are able to sense the Earth's magnetic field, which could then be used as a navigational cue in order to navigate and migrate. I have designed a 3D Helmholtz coil setup to a create variety of artificial magnetic fields and tried to evaluate the bird’s horizontal head movements recorded by a camera located above the coils. The effect of different fields has been examined, such as sweeping, null, steady and flipping fields. Evidence was found that homing pigeons are able to distinguish a flipping field from a steady field, and this can be observed by changes in their head movement. Homing pigeons have also been shown to distinguish different frequencies of flipping inclination field conditions. Data analysis has revealed that the pigeons respond more obviously to a field rotating in both directions, clockwise and counter clockwise. This response has been seen whether compared to a natural baseline or artificial baseline. However, the pigeons' response to the other magnetic field conditions varied significantly depending on the baseline type. III Noor Aldoumani Content Also, I focused on developing a head tracking system in order to extract pigeon's head saccades more accurately while the pigeons are experiencing the various field conditions. The main aim of the new tracking system is to investigate a pigeon's response to the Earth's magnetic field, which requires 3D monitoring of its motor responses to various stimuli. Conventional video analysis (VTA) involves tracking a 2D image, and the resulting data can be noisy and limited to a single field of view (one rotational angle)

Mechanisms of place recognition and path integration based on the insect visual system

Animals are often able to solve complex navigational tasks in very challenging terrain, despite using low resolution sensors and minimal computational power, providing inspiration for robots. In particular, many species of insect are known to solve complex navigation problems, often combining an array of different behaviours (Wehner et al., 1996; Collett, 1996). Their nervous system is also comparatively simple, relative to that of mammals and other vertebrates. In the first part of this thesis, the visual input of a navigating desert ant, Cataglyphis velox, was mimicked by capturing images in ultraviolet (UV) at similar wavelengths to the ant’s compound eye. The natural segmentation of ground and sky lead to the hypothesis that skyline contours could be used by ants as features for navigation. As proof of concept, sky-segmented binary images were used as input for an established localisation algorithm SeqSLAM (Milford and Wyeth, 2012), validating the plausibility of this claim (Stone et al., 2014). A follow-up investigation sought to determine whether using the sky as a feature would help overcome image matching problems that the ant often faced, such as variance in tilt and yaw rotation. A robotic localisation study showed that using spherical harmonics (SH), a representation in the frequency domain, combined with extracted sky can greatly help robots localise on uneven terrain. Results showed improved performance to state of the art point feature localisation methods on fast bumpy tracks (Stone et al., 2016a). In the second part, an approach to understand how insects perform a navigational task called path integration was attempted by modelling part of the brain of the sweat bee Megalopta genalis. A recent discovery that two populations of cells act as a celestial compass and visual odometer, respectively, led to the hypothesis that circuitry at their point of convergence in the central complex (CX) could give rise to path integration. A firing rate-based model was developed with connectivity derived from the overlap of observed neural arborisations of individual cells and successfully used to build up a home vector and steer an agent back to the nest (Stone et al., 2016b). This approach has the appeal that neural circuitry is highly conserved across insects, so findings here could have wide implications for insect navigation in general. The developed model is the first functioning path integrator that is based on individual cellular connections

The applications of satellites to communications, navigation and surveillance for aircraft operating over the contiguous United States. Volume 1 - Technical report

Satellite applications to aircraft communications, navigation, and surveillance over US including synthesized satellite network and aircraft equipment for air traffic contro

Abstracts on Radio Direction Finding (1899 - 1995)

The files on this record represent the various databases that originally composed the CD-ROM issue of "Abstracts on Radio Direction Finding" database, which is now part of the Dudley Knox Library's Abstracts and Selected Full Text Documents on Radio Direction Finding (1899 - 1995) Collection. (See Calhoun record https://calhoun.nps.edu/handle/10945/57364 for further information on this collection and the bibliography). Due to issues of technological obsolescence preventing current and future audiences from accessing the bibliography, DKL exported and converted into the three files on this record the various databases contained in the CD-ROM. The contents of these files are: 1) RDFA_CompleteBibliography_xls.zip [RDFA_CompleteBibliography.xls: Metadata for the complete bibliography, in Excel 97-2003 Workbook format; RDFA_Glossary.xls: Glossary of terms, in Excel 97-2003 Workbookformat; RDFA_Biographies.xls: Biographies of leading figures, in Excel 97-2003 Workbook format]; 2) RDFA_CompleteBibliography_csv.zip [RDFA_CompleteBibliography.TXT: Metadata for the complete bibliography, in CSV format; RDFA_Glossary.TXT: Glossary of terms, in CSV format; RDFA_Biographies.TXT: Biographies of leading figures, in CSV format]; 3) RDFA_CompleteBibliography.pdf: A human readable display of the bibliographic data, as a means of double-checking any possible deviations due to conversion

From skylight input to behavioural output : a computational model of the insect polarised light compass

Many insects navigate by integrating the distances and directions travelled on an outward path, allowing direct return to the starting point. Fundamental to the reliability of this process is the use of a neural compass based on external celestial cues. Here we examine how such compass information could be reliably computed by the insect brain, given realistic constraints on the sky polarisation pattern and the insect eye sensor array. By processing the degree of polarisation in different directions for different parts of the sky, our model can directly estimate the solar azimuth and also infer the confidence of the estimate. We introduce a method to correct for tilting of the sensor array, as might be caused by travel over uneven terrain. We also show that the confidence can be used to approximate the change in sun position over time, allowing the compass to remain fixed with respect to ‘true north’ during long excursions. We demonstrate that the compass is robust to disturbances and can be effectively used as input to an existing neural model of insect path integration. We discuss the plausibility of our model to be mapped to known neural circuits, and to be implemented for robot navigation