HR: 09:10h
AN: P41A-03    [Abstracts]
TI: Emission Maps of Charge-transfer Induced Heliospheric X-rays
AU: * ROSINE, L
EM: rosine.lallement@aerov.jussieu.fr
AF: SERVICE D'AERONOMIE, BP 3, VERRIERES-LE-BUISSON, 91371 France
AU: DALGARNO, A
EM: dalgarno@cfa.harvard.edu
AF: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 United States
AU: KHARCHENKO, V
EM: kharchen@cfa.harvard.edu
AF: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 United States
AU: PEPPINO, R
EM: peppino@cfa.harvard.edu
AF: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 United States
AU: KOUTROUMPA, D
EM: dimitra.koutroupa@aerov.jussieu.fr
AF: SERVICE D'AERONOMIE, BP 3, VERRIERES-LE-BUISSON, 91371 France
AU: IZMODENOV, V
EM: izmod@ipmnet.ru
AF: INSTITUTE FOR PROBLEMS IN MECHANICS, Prospect Vernadskogo 101, Moscow, 117526 Russian Federation
AB: Model distributions of interstellar neutral hydrogen and helium in the heliosphere are combined with minimum and maximum activity 3D solar wind fluxes and compositions. Using updated charge-transfer cross-sections we derive maps and spectral properties of the soft X-ray emission as seen from different vantage points and at different solar cycle phases.
DE: 2144 Interstellar gas
DE: 2169 Sources of the solar wind
SC: Planetary Sciences [P]
MN: 2005 Joint Assembly