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dc.contributor.authorLohmeyer, Whitney
dc.contributor.authorCarlton, Ashley
dc.contributor.authorWong, Frankie
dc.contributor.authorBodeau, Michael
dc.contributor.authorKennedy, Andrew
dc.contributor.authorCahoy, Kerri
dc.date.accessioned2017-06-28T13:12:07Z
dc.date.available2017-06-28T13:12:07Z
dc.date.issued2015-05-25
dc.identifier.urihttp://hdl.handle.net/1721.1/110345
dc.description.abstractThe key components in communications satellite payloads are the high-power amplifiers that amplify the received signal so that it can be accurately transmitted to the intended end user. In this study, we examine 26 amplifier anomalies and quantify the high-energy electron environment for periods of time prior to the anomalies. Building on the work of Lohmeyer and Cahoy (2013), we find that anomalies occur at a rate higher than just by chance when the >2 MeV electron fluence accumulated over 14 and 21 days is elevated. To try to understand “why,” we model the amplifier subsystem to assess whether the dielectric material in the radio frequency (RF) coaxial cables, which are the most exposed part of the system, is liable to experience electrical breakdown due to internal charging. We find that the accumulated electric field over the 14 and 21 days leading up to the anomalies is high enough to cause the dielectric material in the coax to breakdown. We also find that the accumulated voltages reached are high enough to compromise components in the amplifier system, for example, the direct current (DC) blocking capacitor. An electron beam test using a representative coaxial cable terminated in a blocking capacitor showed that discharges could occur with peak voltages and energies sufficient to damage active RF semiconductor devices.en_US
dc.description.sponsorshipAir Force Office of Sponsored Research (AFOSR) grant FA9550-13-1-0099 and the National Science Foundation (NSF)en_US
dc.language.isoen_USen_US
dc.publisherAGU Space Weatheren_US
dc.titleResponse of geostationary communications satellite solid-state power amplifiers to high-energy electron fluenceen_US
dc.typeArticleen_US
dc.identifier.citationLohmeyer, W., A. Carlton, F. Wong, M. Bodeau, A. Kennedy, and K. Cahoy (2015), Response of geostationary communications satellite solid-state power amplifiers to high-energy electron fluence, Space Weather, 13, 298–315, doi:10.1002/2014SW001147.en_US


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