Invited article: Characterization of background sources in space-based time-of-flight mass spectrometers
J A Gilbert1, D J Gershman1, G Gloeckler1
1Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, 2455 Hayward St, Ann Arbor, Michigan 48109, USA.
The Review of Scientific Instruments
|October 3, 2014
Summary
Background signals in time-of-flight mass spectrometers complicate space plasma data analysis. This review details common sources, their data signatures, and mitigation strategies for improved instrument performance.
Area of Science:
- Space plasma physics
- Instrumental analysis
- Mass spectrometry
Background:
- Background signals in time-of-flight (TOF) instruments can compromise space plasma measurements.
- These signals increase data analysis complexity and reduce signal-to-noise ratios, impacting scientific value.
Purpose of the Study:
- To review common background signal sources in TOF mass spectrometers used for space plasma.
- To illustrate the effects of these sources using real data examples.
- To discuss mitigation strategies and design considerations for future instruments.
Main Methods:
- Review of established literature on TOF mass spectrometry background.
- Analysis of data from space plasma instruments ACE-SWICS and MESSENGER-FIPS.
- Identification and categorization of various background signal origins.
Main Results:
- Identified key background sources: penetrating particles, UV photons, energy/angular scattering, electron stimulated desorption, ion-induced electron emission, accidental coincidences, and electronic noise.
- Demonstrated data signatures for each source using instrument examples.
- Provided insights into the impact of each source on data quality.
Conclusions:
- Understanding and mitigating background signals are crucial for accurate space plasma measurements.
- Effective strategies and design considerations can enhance the performance of TOF instruments.
- This review serves as a guide for researchers and instrument designers in the field.
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