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Title: Onboard Science Data Analysis: Implications for Future Missions
Primary Author: David R. Thompson
Secondary Author(s): David R. Thompson, Robert C. Anderson, Benjamin Bornstein, Nathalie A. Cabrol, Steve Chien, Tara Estlin, Terry Fong, Robert Hogan, Ralph Lorenz, Daniel Gaines, Martha S. Gilmore, Mario Parente, Liam Pedersen, Ted L. Roush, Giuseppe Marzo, David Wettergreen
Institution: Jet Propulsion Laboratory
Date: September 15, 2009
Summary: Onboard science data analysis enables new spacecraft operational modes that improve science yield. It can relieve constraints on time, bandwidth and power, and respond automatically to events on short time scales. We examine applications to rover, aerobot, and orbital platforms.
Panel Selection: Inner Planets: Mercury, Venus, and the Moon.
Mars: Not Phobos and Deimos.
Giant Planets: Jupiter, Saturn, Uranus, Neptune, and exoplanets, including rings and magnetic fields, but not their satellites.
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets.
Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust.
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These documents have been prepared in coordination with the National Academies of Science in support of the National Academies Planetary Science Decadal Survey. These documents are being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology.