HR: 1340h
AN: SH33A-1083    [Abstracts]
TI: Solar Wind and Suprathermal Ion Populations at the STEREO Spacecraft Approaching Solar Minimum
AU: * Galvin, A B
EM: toni.galvin@unh.edu
AF: University of New Hampshire, Space Science Center Morse Hall, Durham, NH 03824, United States
AU: Popecki, M
AF: University of New Hampshire, Space Science Center Morse Hall, Durham, NH 03824, United States
AU: Kistler, L
AF: University of New Hampshire, Space Science Center Morse Hall, Durham, NH 03824, United States
AU: Simunac, K
AF: University of New Hampshire, Space Science Center Morse Hall, Durham, NH 03824, United States
AU: Farrugia, C
AF: University of New Hampshire, Space Science Center Morse Hall, Durham, NH 03824, United States
AU: Gustafson, A
AF: University of New Hampshire, Space Science Center Morse Hall, Durham, NH 03824, United States
AU: Barry, J
AF: University of New Hampshire, Space Science Center Morse Hall, Durham, NH 03824, United States
AU: Ellis, L
AF: University of New Hampshire, Space Science Center Morse Hall, Durham, NH 03824, United States
AU: Moebius, E
AF: University of New Hampshire, Space Science Center Morse Hall, Durham, NH 03824, United States
AU: Blush, L
AF: University of Bern, Physikalisches Institute, Bern, 3012, Switzerland
AU: Klecker, B
AF: Max Planck Institute for extraterrestrial physics, Giessenbachstrasse, Garching, 85748, Germany
AU: Bochsler, P
AF: University of Bern, Physikalisches Institute, Bern, 3012, Switzerland
AU: Wurz, P
AF: University of Bern, Physikalisches Institute, Bern, 3012, Switzerland
AU: Wimmer-Schweingruber, R
AF: University of Kiel, institute for Experimental and Applied Physics, Kiel, 24098, Germany
AU: Thompson, B
AF: NASA, Goddard Spaceflight Center, Greenbelt, MD 20771, United States
AU: Luhmann, J
AF: University of California, Berkeley, Space Science Laboratory, Berkeley, CA 94720, United States
AU: Russell, C
AF: University of California, Los Angeles, Institute of Geophysics and Planetary Physics, Los Angeles, CA 90024, United States
AB: The two STEREO spacecraft, which were launched in October 2006, have been gradually separating in longitude at a rate of about 22 degrees per year. During this past year, the dominant heliospheric features have been a series of recurrent high and slow speed solar wind and their interaction regions, an occasional transient event (e.g., May 22), and "background" suprathermal populations such as interstellar pick up ions. In this poster we present an overview of the plasma and suprathermal signatures observed by the STEREO spacecraft using data from the Plasma and Suprathermal Ion Composition (PLASTIC) and Magnetometer (IMPACT/MAG) investigations. Complementary STEREO PLASTIC related presentations in this session are by Popecki et al., Klecker et al. (invited), and Simunac et al.
DE: 2111 Ejecta, driver gases, and magnetic clouds
DE: 2164 Solar wind plasma
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2007 Fall Meeting