Sky polarization and sun sensor system and method
First Claim
1. A method of determining orientation of an object, the method comprising:
- recording raw image data of the sky using a sky polarimeter;
calculating Stokes parameters (S0, S1, S2), degree of linear polarization (DoLP) and angle of polarization (AoP) from the image data;
detecting obscurants and filtering the obscurants from the image data to produce a filtered image;
obtaining position/orientation data of the object;
finding the Sun azimuth and elevation in the filtered image by performing a coordinate transform on a measured polarization pattern to generate a scanning AoP image;
determining one or more of the roll, pitch, yaw, latitude and longitude of the object using the filtered image;
when yaw is determined using the filtered image, calculating platform yaw based on the angle between the line intersecting the Sun and the zenith and expected Sun/azimuth position for a given date and time;
performing minimum detection and extracting a region of the image containing the Sun and zenith;
applying morphological erosion on a binary image to reduce the detected minimum region to a single line; and
extracting a sun-zenith line.
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Abstract
A system for determining a new orientation and/or position of an object comprises a sky polarimeter configured to record image data of the sky, a signal processing unit, and logic configured to receive and store in memory the image data received from the sky polarimeter. The logic calculates the Stokes parameters (S0, S1, S2,), DoLP, and AoP from the image data, detects obscurants and filters the obscurants (such as clouds and trees) from the image data to produce a filtered image. The logic is further configured to find the Sun and zenith in the filtered image, and to determine the roll, pitch, yaw, latitude and longitude of the object using the filtered image. A method for determining a new position/orientation of an object comprises recording raw image data using a sky polarimeter, calculating S0, S1, S2, DoLP, and AoP from the image data, detecting obscurants and filtering the obscurants from the image data to produce a filtered image, obtaining last known position/orientation data of the object, finding the Sun and zenith in the filtered image, and determining the roll, pitch, yaw, latitude and longitude of the object using the filtered image.
32 Citations
9 Claims
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1. A method of determining orientation of an object, the method comprising:
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recording raw image data of the sky using a sky polarimeter; calculating Stokes parameters (S0, S1, S2), degree of linear polarization (DoLP) and angle of polarization (AoP) from the image data; detecting obscurants and filtering the obscurants from the image data to produce a filtered image; obtaining position/orientation data of the object; finding the Sun azimuth and elevation in the filtered image by performing a coordinate transform on a measured polarization pattern to generate a scanning AoP image; determining one or more of the roll, pitch, yaw, latitude and longitude of the object using the filtered image; when yaw is determined using the filtered image, calculating platform yaw based on the angle between the line intersecting the Sun and the zenith and expected Sun/azimuth position for a given date and time; performing minimum detection and extracting a region of the image containing the Sun and zenith; applying morphological erosion on a binary image to reduce the detected minimum region to a single line; and extracting a sun-zenith line. - View Dependent Claims (2, 3, 4, 5, 6, 7, 8, 9)
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Specification