2013
DOI: 10.1063/1.4824352
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Response in electrostatic analyzers due to backscattered electrons: Case study analysis with the Juno Jovian Auroral Distribution Experiment-Electron instrument

Abstract: In this study, we introduce a model to characterize electron scattering in an electrostatic analyzer. We show that electrons between 0.5 and 30 keV scatter from internal surfaces to produce a response up to ~20% of the ideal, unscattered response. We compare our model results to laboratory data from the Jovian Auroral Distribution Experiment-Electron sensor onboard the NASA Juno mission. Our model reproduces the measured energy-angle response of the instrument well. Understanding and quantifying this scatterin… Show more

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Cited by 2 publications
(6 citation statements)
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“…A Maxwellian‐like distribution centered on ~300 keV is clearly evident in the upward moving electrons and not the other pitch angles, suggesting a coherent acceleration structure aligning the particles parallel to the local magnetic field. The very slight “bump” near 300 keV in f ( p ) trap at 1% level is likely due to scattering within the instrument [ Mauk et al ., ; Clark et al ., ]. The half width at half maximum (HWHM) of the field‐aligned portion of the pitch angle distribution is ~10°, which suggests a beam collimated along the field.…”
Section: Low‐altitude Observations Of Energetic Electrons and Ions Ovmentioning
confidence: 99%
“…A Maxwellian‐like distribution centered on ~300 keV is clearly evident in the upward moving electrons and not the other pitch angles, suggesting a coherent acceleration structure aligning the particles parallel to the local magnetic field. The very slight “bump” near 300 keV in f ( p ) trap at 1% level is likely due to scattering within the instrument [ Mauk et al ., ; Clark et al ., ]. The half width at half maximum (HWHM) of the field‐aligned portion of the pitch angle distribution is ~10°, which suggests a beam collimated along the field.…”
Section: Low‐altitude Observations Of Energetic Electrons and Ions Ovmentioning
confidence: 99%
“…For example, magnetic field strengths on the order of a few Gauss or less can have a considerable affect on the sensor's response function for electron energies below~5 keV. Electron scattering was found to be important for energies between~1 keV to greater than 50 keV [Clark et al, 2013]. Lastly, it was shown in McComas et al [2013] that electron relativistic effects are nonnegligible for energies above 20-30 keV.…”
Section: Modelmentioning
confidence: 99%
“…Journal of Geophysical Research: Space Physics 10.1002/2016JA022583 electron scattering [Clark et al, 2013] for the JADE-E sensor as well as other plasma sensors [e.g., Collinson et al, 2009;Randol et al, 2010].…”
Section: Modelmentioning
confidence: 99%
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