least squares
Mission-integrated ⪅8nT magnetometer (MAG) data at Jupiter and Saturn, 100-minute averages. Data consist of the only available MAG measurements that spanned at least 6 months (180 Earth days), and include the Cassini–Huygens, Galileo, and Juno missions. Steven P. Joy and Joe Mafi (UCLA & NASA Planetary Data System/Planetary Plasma Interactions Node) provided concatenated and RTN-rotated Jupiter MAG 1-minute averages from Galileo and Juno, including random samples of field swelling.
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North/South-separated <10nT magnetometer data from the 1994-2008 Ulysses space mission's samplings of polar solar winds, hourly averaged, non-decimated. The set also includes data from the WIND space mission, the WSO terrestrial observatory (solar Mean Magnetic Field), and the WSO solar Polar magnetic Field, all used in the same research project. The NOAA Solar Indices data (not included) were used for verification, see paper for details.
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This data-set was used for the localization of an emitter based on Time Difference of Arrival (TDoA).
The classical least-squares (LS) algorithm, with a limited number of TDoA measurements, has been utilized for obtaining a closed-form solution to the source localization problem.
An extension of the classical LS algorithm has been employed in an attempt to improve the precision of the localization technique by using a larger set of TDoA estimates.
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