Cube Root Georgia Institute of Technology Matt Bigelow, Gregory Hansen, Sarah McNeese, Luke Walker
Mission Overview: The Cube Root mission will demonstrate various functionalities of components to be used in the R 3 satellite. The visible camera will capture images from the edge-of- space environment. The radiation dosimeter will detect the total ionizing dose of the SHOT II environment. The flight computer will interface with these two components for command and data handling. An image processing benchmark will demonstrate one of the major mission objectives of the R 3 satellite.
SHOT II / UNP-6 Connection: Cube Root shall support R 3 by evaluating component performance in the edge-of-space environment: Visible camera Radiation dosimeter (temperature anomalies?) Flight computer Cube Root provided fabrication experience: Soldering and board layout design Component configuration and wire harnessing Flight software development. Cube root provided I&T experience, including physical, thermal, electrical, and functional testing.
SHOT II Design and Test Details: Basic Components: Flight Computer (FCS20, DSP-FPGA) Radiation Dosimeter Visible Camera (Point Grey Grasshopper) Power Supply (18 VDC, 5 VDC) Compliance: Mass: 1.2 kg Dimensions: 16 x 18 x 24 cm Flight String: directly though center of structure, no corners Testing: Structural integrity: whip, drop, and stair pitch tests Dosimeter and visible camera functionality: tested in Micro-C++ with a laptop computer Image processing benchmark: tested on the flight computer with pre-loaded images.
Expected Results: The radiation dosimeter may return flipped bits as a result of the radiation environment during flight. The visible camera will return images from the flight. The flight computer will return coordinates of the center of brightness of preloaded images. These same algorithms will be applied to IR images on R 3 to detect thermal boundaries and anomalies
Demonstration: The image processing algorithm will be demonstrated on the Cube Root flight computer. Pre-loaded images will represent those to be taken during flight. The computer will process the images and find the coordinates of the center of brightness. The output will be the raw image and the desired coordinates, which, when onboard the R 3 satellite, will be used for rapid response.