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Marshall Space Flight Center's Solar Wind FacilityHistorically, NASA's Marshall Space Flight Center (MSFC) has operated a Solar Wind Facility (SWF) to provide long term particle and photon exposure to material samples. The requirements on the particle beam details were not stringent as the cumulative fluence level is the test goal. Motivated by development of the faraday cup instrument on the NASA Solar Probe Plus (SPP) mission, the MSFC SWF has been upgraded to included high fidelity particle beams providing broadbeam ions, broadbeam electrons, and narrow beam protons or ions, which cover a wide dynamic range of solar wind velocity and flux conditions. The large vacuum chamber with integrated cryo-shroud, combined with a 3-axis positioning system, provides an excellent platform for sensor development and qualification. This short paper provides some details of the SWF charged particle beams characteristics in the context of the Solar Probe Plus program requirements. Data will be presented on the flux and energy ranges as well as beam stability.
Document ID
20170005311
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Wright, K. H.
(Universities Space Research Association Huntsville, AL, United States)
Schneider, T. A.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Vaughn, J. A.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Whittlesey, P. L.
(California Univ. Berkeley, CA, United States)
Date Acquired
June 7, 2017
Publication Date
May 15, 2017
Subject Category
Solar Physics
Report/Patent Number
M17-6026
Meeting Information
Meeting: Applied Space Environments Conference (ASEC)
Location: Huntsville, AL
Country: United States
Start Date: May 15, 2017
End Date: May 19, 2017
Sponsors: Universities Space Research Association
Funding Number(s)
CONTRACT_GRANT: NNM13AA43C
CONTRACT_GRANT: NNM11AA01A
Distribution Limits
Public
Copyright
Public Use Permitted.
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