Plasma and Radiation Combined IN-situ Instrument (PRCINI): Difference between revisions
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(Created page with "{{Infobox Technology |pi=Ian Cohen |inst=John Hopkins University Applied Physics Laboratory (JHU/APL) |trl=3 |instrument type=Particle Spectrometer |status=Active |id=20-HTIDS-20-0009 }} ==Overview== PRCINI integrates the electrostatic analyzer (ESA) from the Cassini/Charge-Energy-Mass-Spectrometer (CHEMS) instrument into a modified version of the Parker Solar Probe/Energetic Particle Instrument (EPI)-Lo sensor, resulting in a combined suprathermal and energetic ion inst...") |
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Latest revision as of 15:33, 15 February 2023
| Plasma and Radiation Combined IN-situ Instrument (PRCINI) | |
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| Principal Investigator | Ian Cohen |
| Institution | John Hopkins University Applied Physics Laboratory (JHU/APL) |
| Technology Readiness Level | 3 |
| Instrument Type | Particle Spectrometer |
| Project Status | Active |
| Project ID | 20-HTIDS-20-0009 |
Overview
PRCINI integrates the electrostatic analyzer (ESA) from the Cassini/Charge-Energy-Mass-Spectrometer (CHEMS) instrument into a modified version of the Parker Solar Probe/Energetic Particle Instrument (EPI)-Lo sensor, resulting in a combined suprathermal and energetic ion instrument that measures energy, angular distribution, and compositional distributions from ~1 keV to ≳15 MeV, as well as ion charge-state composition from ~15 (protons) to ~220 keV/q, over co-planar fields-of-view.