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New Horizons Solar Wind Around Pluto (SWAP) - Pluto Encounter Raw Data, Version 1.0

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DataCite Commons2025-07-03 更新2026-05-05 收录
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https://pdssbn.astro.umd.edu/holdings/pds4-nh_swap:pluto_raw-v1.0/SUPPORT/dataset.shtml
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This data set contains Raw data taken by the New Horizons Solar Wind Around Pluto (SWAP) instrument during the PLUTO ENCOUNTER mission phase. These data were migrated from the PDS3 dataset: NH-P-SWAP-2-PLUTO-V3.0. SWAP comprises electro-optics and detectors to obtain count rate measurements of the solar wind; measuring the solar wind before, during and after the Pluto encounter will allow characterization of the atmospheric escape rate of Pluto. The SWAP electro-optic elements select the angles and energies of the solar wind and pickup ions to be measured; ions thus selected are registered with a coincidence detector system. SWAP measures the energy spectrum of ions in its environment by varying (also called scanning or sweeping) voltages of the electro-optics over many steps during a short time period. SWAP can also immediately follow a sweep of coarse voltage steps with a sweep of finer steps, centered on the peak measurement of the coarse sweep, to obtain a higher resolution of that portion of the energy spectrum. There are three types of SWAP science data: real-time; summary; histogram. Real-time data, at rates up to 1Hz, provide the most detailed science measurements since they contain the full count rate distribution as a function of energy (speed). For science summary and science histogram modes, the full distribution is not recorded. Instead, parameters are derived from the count rate distribution stored by SWAP. These derived parameters require less memory than storing the whole distribution. The science summary and science histogram modes are primarily used during the cruise phase of the mission. For science data, the common data product is usually a binary table; for calibrated real-time data, spectrograms as images are also provided. Typically the tables have instrument parameters and measurements in the columns and measurement times in the rows, but the actual format depends on the type of data and the processing level (raw vs. calibrated). Other tables containing housekeeping and other parameters are also provided. Labels were redesigned during migration using the .FIT header and PDS3 .LBL files, but the data files are unchanged from their PDS3 version.
提供机构:
NASA Planetary Data System
创建时间:
2025-03-13
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