All Physics Faculty Publications

Document Type

Article

Journal/Book Title/Conference

IEEE Transactions on Plasma Science

Volume

40

Issue

2

Publication Date

2-2012

First Page

298

Last Page

304

DOI

10.1109/TPS.2011.2178251

Abstract

Spacecraft charging codes require accurate models of electron yields as a function of accumulated charge to correctly predict the charge build up on spacecraft. The accumulated charge creates equilibrium surface potentials on spacecraft resulting from interactions with the space plasma environment. There is, however, a complex relation between these emission properties and the charge built up in spacecraft insulators.

This paper focuses on different methods appropriate to determine the fundamental electronic material property of total electron yield as the materials accumulate charge. Three methods for determining the uncharged total yield are presented:

(i) The DC Continuous Beam Method is a relatively easy and accurate method appropriate for conductors and semi- conductors with maximum total electron yield σmaxρ<1017 >Ω-cm.

(ii) The Pulse-Yield Method seeks to minimize the effects of charging and is applicable to materials with σmaxρ up to >1024 Ω-cm. (iii) The Yield Decay Method is a very difficult and time consuming technique that uses a combination of measurement and modeling to investigate the most difficult materials with σmax>4 and ρ up to >1024 Ω-cm.

Data for high purity polycrystalline Au, KaptonTM HN and CP1TM polyimides, and polycrystalline aluminum oxide ceramic are presented. These data demonstrate the relative strengths and weaknesses of each method, but more importantly show that the methods described herein are capable of reliably measuring the total electron yield of almost any spacecraft material.

Comments

Published by IEEE in IEEE Transactions on Plasma Science. Author post print available for download through link above.

This study was partially funded by the NASA Solar Probe Mission through the Johns Hopkins University Applied Physics Laboratory and by the NASA Space Environments and Effects program.

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