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Resolving Space Plasma Species With Electrostatic Analyzers

Nicolaou, Georgios; Haythornthwaite, Richard P; Coates, Andrew J; (2022) Resolving Space Plasma Species With Electrostatic Analyzers. Frontiers in Astronomy and Space Sciences , 9 , Article 861433. 10.3389/fspas.2022.861433. Green open access

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Abstract

Electrostatic analyzers resolve the energy-per-charge distributions of charged plasma particles. Some space plasma instruments use electrostatic analyzers among other units, such as aperture deflectors and position sensitive detectors, in order to resolve the three-dimensional energy (velocity) distribution functions of plasma particles. When these instruments do not comprise a mass analyzer unit, different species can be resolved only if there are measurable differences in their energy-per-charge distributions. This study examines the ability of single electrostatic analyzer systems in resolving co-moving plasma species with different mass-per-charge ratios. We consider examples of static plasma consisting of two species of heavy negative ions measured by a typical electrostatic analyzer design, similar to the electron spectrometer on board Cassini spacecraft. We demonstrate an appropriate modeling technique to simulate the basic features of the instrument response in the specific plasma conditions and we quantify its ability to resolve the key species as a function of the spacecraft speed and the plasma temperature. We show that for the parameter range we examine, the mass resolution increases with increasing spacecraft speed and decreasing plasma temperature. We also demonstrate how our model can analyze real measurements and drive future instrument designs.

Type: Article
Title: Resolving Space Plasma Species With Electrostatic Analyzers
Open access status: An open access version is available from UCL Discovery
DOI: 10.3389/fspas.2022.861433
Publisher version: https://doi.org/10.3389/fspas.2022.861433
Language: English
Additional information: Copyright © 2022 Nicolaou, Haythornthwaite and Coates. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
Keywords: Science & Technology, Physical Sciences, Astronomy & Astrophysics, plasma physics, instrumentation, planetary physics, Methods, plasma modeling, SOLAR-WIND, IONS
UCL classification: UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL
URI: https://discovery.ucl.ac.uk/id/eprint/10152361
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