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Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus

Authors :
Massachusetts Institute of Technology. Department of Physics
MIT Kavli Institute for Astrophysics and Space Research
Belcher, John Winston
Lazarus, Alan J
Richardson, John D
Kasper, Justin C
Abiad, Robert
Austin, Gerry
Balat-Pichelin, Marianne
Bale, Stuart D
Berg, Peter
Bergner, Henry
Berthomier, Matthieu
Bookbinder, Jay
Brodu, Etienne
Caldwell, David
Case, Anthony W
Chandran, Benjamin D G
Cheimets, Peter
Cirtain, Jonathan W
Cranmer, Steven R
Curtis, David W
Daigneau, Peter
Dalton, Greg
Dasgupta, Brahmananda
DeTomaso, David
Diaz-Aguado, Millan
Djordjevic, Blagoje
Donaskowski, Bill
Effinger, Michael
Florinski, Vladimir
Fox, Nichola
Freeman, Mark
Gallagher, Dennis
Gary, S. P
Gauron, Tom
Gates, Richard
Goldstein, Melvin
Golub, Leon
Gordon, Dorothy A
Gurnee, Reid
Guth, Giora
Halekas, Jasper
Hatch, Ken
Heerikuisen, Jacob
Ho, George
Hu, Qiang
Johnson, Greg
Jordan, Steven P
Korreck, Kelly E
Larson, Davin
Li, Gang
Livi, Roberto
Ludlam, Michael
Maksimovic, Milan
McFadden, James P
Marchant, William
Maruca, Bennet A
McComas, David J
Messina, Luciana
Mercer, Tony
Park, Sang
Peddie, Andrew M
Pogorelov, Nikolai
Reinhart, Matthew J
Robinson, Miles
Rosen, Irene
Skoug, Ruth M
Slagle, Amanda
Steinberg, John T
Stevens, Michael L
Taylor, Ellen R
Tiu, Chris
Turin, Paul
Velli, Marco
Webb, Gary
Whittlesey, Phyllis
Wright, Ken
Wu, S. T
Zank, Gary
Szabo, Adam, 1965
Richardson, John D.
Massachusetts Institute of Technology. Department of Physics
MIT Kavli Institute for Astrophysics and Space Research
Belcher, John Winston
Lazarus, Alan J
Richardson, John D
Kasper, Justin C
Abiad, Robert
Austin, Gerry
Balat-Pichelin, Marianne
Bale, Stuart D
Berg, Peter
Bergner, Henry
Berthomier, Matthieu
Bookbinder, Jay
Brodu, Etienne
Caldwell, David
Case, Anthony W
Chandran, Benjamin D G
Cheimets, Peter
Cirtain, Jonathan W
Cranmer, Steven R
Curtis, David W
Daigneau, Peter
Dalton, Greg
Dasgupta, Brahmananda
DeTomaso, David
Diaz-Aguado, Millan
Djordjevic, Blagoje
Donaskowski, Bill
Effinger, Michael
Florinski, Vladimir
Fox, Nichola
Freeman, Mark
Gallagher, Dennis
Gary, S. P
Gauron, Tom
Gates, Richard
Goldstein, Melvin
Golub, Leon
Gordon, Dorothy A
Gurnee, Reid
Guth, Giora
Halekas, Jasper
Hatch, Ken
Heerikuisen, Jacob
Ho, George
Hu, Qiang
Johnson, Greg
Jordan, Steven P
Korreck, Kelly E
Larson, Davin
Li, Gang
Livi, Roberto
Ludlam, Michael
Maksimovic, Milan
McFadden, James P
Marchant, William
Maruca, Bennet A
McComas, David J
Messina, Luciana
Mercer, Tony
Park, Sang
Peddie, Andrew M
Pogorelov, Nikolai
Reinhart, Matthew J
Robinson, Miles
Rosen, Irene
Skoug, Ruth M
Slagle, Amanda
Steinberg, John T
Stevens, Michael L
Taylor, Ellen R
Tiu, Chris
Turin, Paul
Velli, Marco
Webb, Gary
Whittlesey, Phyllis
Wright, Ken
Wu, S. T
Zank, Gary
Szabo, Adam, 1965
Richardson, John D.
Source :
Springer Netherlands
Publication Year :
2017

Abstract

The Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Solar Probe Plus is a four sensor instrument suite that provides complete measurements of the electrons and ionized helium and hydrogen that constitute the bulk of solar wind and coronal plasma. SWEAP consists of the Solar Probe Cup (SPC) and the Solar Probe Analyzers (SPAN). SPC is a Faraday Cup that looks directly at the Sun and measures ion and electron fluxes and flow angles as a function of energy. SPAN consists of an ion and electron electrostatic analyzer (ESA) on the ram side of SPP (SPAN-A) and an electron ESA on the anti-ram side (SPAN-B). The SPAN-A ion ESA has a time of flight section that enables it to sort particles by their mass/charge ratio, permitting differentiation of ion species. SPAN-A and -B are rotated relative to one another so their broad fields of view combine like the seams on a baseball to view the entire sky except for the region obscured by the heat shield and covered by SPC. Observations by SPC and SPAN produce the combined field of view and measurement capabilities required to fulfill the science objectives of SWEAP and Solar Probe Plus. SWEAP measurements, in concert with magnetic and electric fields, energetic particles, and white light contextual imaging will enable discovery and understanding of solar wind acceleration and formation, coronal and solar wind heating, and particle acceleration in the inner heliosphere of the solar system. SPC and SPAN are managed by the SWEAP Electronics Module (SWEM), which distributes power, formats onboard data products, and serves as a single electrical interface to the spacecraft. SWEAP data products include ion and electron velocity distribution functions with high energy and angular resolution. Full resolution data are stored within the SWEM, enabling high resolution observations of structures such as shocks, reconnection events, and other transient structures to be selected for download after the fact. This paper describes t<br />United States. National Aeronautics and Space Administration (contract NNN06AA01C (Task NNN10AA08T))

Details

Database :
OAIster
Journal :
Springer Netherlands
Notes :
application/pdf, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1141889468
Document Type :
Electronic Resource