HR: 11:50h
AN: SH52B-07    [Abstracts]
TI: Solar Wind Charge State Composition Results from PLASTIC
AU: * Popecki, M
EM: mark.popecki@unh.edu
AF: University of New Hampshire, Morse Hall 39 College Rd, Durham, NH 03824, United States
AU: Galvin, A B
EM: toni.galvin@unh.edu
AF: University of New Hampshire, Morse Hall 39 College Rd, Durham, NH 03824, United States
AU: Kistler, L M
EM: lynn.kistler@unh.edu
AF: University of New Hampshire, Morse Hall 39 College Rd, Durham, NH 03824, United States
AU: Moebius, E
EM: eberhard.moebius@unh.edu
AF: University of New Hampshire, Morse Hall 39 College Rd, Durham, NH 03824, United States
AU: Klecker, B
EM: berndt.klecker@mpe.mpg.de
AF: Max-Planck Institut fuer extraterrestrische Physik, Giessenbachstrasse, Garching, 85748, Germany
AU: Kucharek, H
EM: harald.kucharek@unh.edu
AF: University of New Hampshire, Morse Hall 39 College Rd, Durham, NH 03824, United States
AU: Simunac, K
EM: kristin.simunac@cisunix.unh.edu
AF: University of New Hampshire, Morse Hall 39 College Rd, Durham, NH 03824, United States
AU: Bochsler, P
EM: peter.bochsler@phim.unibe.ch
AF: Physikalisches Institut, University of Bern Sidlerstrasse 5, Bern, 3012, Switzerland
AU: Blush, L
EM: lisa.blush@space.unibe.ch
AF: Physikalisches Institut, University of Bern Sidlerstrasse 5, Bern, 3012, Switzerland
AU: Karrer, R
EM: reto.karrer@space.unibe.ch
AF: Physikalisches Institut, University of Bern Sidlerstrasse 5, Bern, 3012, Switzerland
AU: Daoudi, H
EM: hagar.daoudi@space.unibe.ch
AF: Physikalisches Institut, University of Bern Sidlerstrasse 5, Bern, 3012, Switzerland
AU: Opitz, A
EM: andrea.opitz@space.unibe.ch
AF: Physikalisches Institut, University of Bern Sidlerstrasse 5, Bern, 3012, Switzerland
AU: Giammanco, C
EM: corrado.giammanco@space.unibe.ch
AF: Physikalisches Institut, University of Bern Sidlerstrasse 5, Bern, 3012, Switzerland
AU: Wimmer-Schweingruber, R
EM: wimmer@physik.uni-kiel.de
AF: Institute for Experimental and Applied Physics, University of Kiel, Kiel, 24098, Germany
AB: The PLASTIC instrument on the STEREO spacecraft provides solar wind proton moments and heavy ion composition. Using an electrostatic analyzer with a time of flight and residual energy measurement, it can supply mass and ionic charge state for solar wind heavy ions. Preliminary results for iron will be shown for selected events, including the possible flux rope passage on May 21-22, 2007, and a near-magnetotail passage in February, 2007.
DE: 2164 Solar wind plasma
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2007 Fall Meeting