Date of Award
Winter 2019
Project Type
Dissertation
Program or Major
Physics
Degree Name
Doctor of Philosophy
First Advisor
Harald Kucharek
Second Advisor
Karsten Pohl
Third Advisor
James Ryan
Abstract
Earth's magnetosphere contains plasma originating both from the solar wind and from
the ionosphere. While H+ is the dominant ion from both sources, the solar wind contains
high charge state ions such as He++, and O6+, while the ionosphere contributes singly ionized
heavy ions including He+, N+ and O+. Measuring the composition gives information on
the source and mass dependent entry, heating and acceleration mechanisms. However, most
ion composition instruments are not able to clearly distinguish between some of the heavy
ions involved in these processes, particularly N+ and O+. This thesis aims to test a new
design of a Time-of-Flight mass spectrometer that should improve the mass resolution by
reducing scattering. In this new design, the carbon foil that is normally used to generate
a "Start" signal is replaced by a single straight-channel Microchannel Plate (MCP). These
changes are implemented in the engineering copy of the Ion Composition and Distribution
Function analyzer (CODIF) instrument, allowing us to investigate the eects of the change
on spectra and flux for different MCP geometries as well as different thin film coatings. We
demonstrate that all tested MCP geometries with or without coatings significantly reduce
the energy lost from the ion when compared against the carbon foil, but only for ions heavier
than carbon; this improves separation of the heavier ion species close in mass, characterized
by the transit time of the Gaussian-distributed centroid in time and the Full Width Half
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Max of the spectra. Geometry effects are the most significant, with the narrower pores
having the largest reduction in energy transferred from the ion. However, MCP response
is heavily dependent on impinging angle and comes at the cost of severely decreased ion
flux for the narrower pore sizes. Thin film coatings of Al2O3 on the MCPs result in smooth
surfaces that increase the probabilities of specular reflection occurring and reduce the energy
required to emit an electron, resulting in slightly increased scattering while improving the
detection efficiency. Additionally, the instrument using MCPs can accurately determine mass
at energies far lower than where the carbon foil's energy losses cause the spectra to be too
broad to be distinguished. This demonstrates that an MCP-based instrument would not
require a Post Acceleration voltage (PAC). Results from this work culminate in a future
detector design, capitalizing on the advantages offered by the MCP and carbon foils.
Recommended Citation
Lubinsky, Nicholas Kenneth, "Microchannel Plates in Mass Spectrometer Instruments for Spacecraft" (2019). Doctoral Dissertations. 2491.
https://scholars.unh.edu/dissertation/2491