To link to full-text access for this article, visit this link: http://dx.doi.org/10.1016/j.icarus.2005.09.018 Byline: E. Kallio (a), A. Fedorov (b), E. Budnik (b), T. Sales (a), P. Janhunen (a), W. Schmidt (a), H. Koskinen (a)(q), P. Riihela (a), S. Barabash (c), R. Lundin (c), M. Holmstrom (c), H. Gunell (c), K. Brinkfeldt (c), Y. Futaana (c), H. Andersson (c), M. Yamauchi (c), A. Grigoriev (c), J.-A. Sauvaud (b), J.-J. Thocaven (b), J.D. Winningham (d), R.A. Frahm (d), J.R. Sharber (d), J.R. Scherrer (d), A.J. Coates (e), D.R. Linder (e), D.O. Kataria (e), J. Kozyra (f), J.G. Luhmann (g), E. Roelof (h), D. Williams (h), S. Livi (h), C.C. Curtis (i), K.C. Hsieh (i), B.R. Sandel (i), M. Grande (j), M. Carter (j), S. McKenna-Lawler (k), S. Orsini (l), R. Cerulli-Irelli (l), M. Maggi (l), P. Wurz (m), P. Bochsler (m), N. Krupp (n), J. Woch (n), M. Franz (n), K. Asamura (o), C. Dierker (p) Keywords: Mars; atmosphere; Ionospheres Abstract: We have analysed ion escape at Mars by comparing ASPERA-3/Mars Express ion measurements and a 3-D quasi-neutral hybrid model. As Mars Express does not have a magnetometer onboard, the analysed IMA data are from an orbit when the IMF clock angle was possible to determine from the magnetic field measurements of Mars Global Surveyor. We found that fast escaping planetary ions were observed at the place which, according to the 3-D model, is anticipated to contain accelerated heavy ions originating from the martian ionosphere. The direction of the interplanetary magnetic field was found to affect noticeably which regions can be magnetically connected to Mars Express and to the overall 3-D Mars-solar wind interaction. Author Affiliation: (a) Space Research Unit, Finnish Meteorological Institute, Erik Palmenin aukio 1, P.O. Box 503, FIN-00101 Helsinki, Finland (b) Centre d'Etude Spatiale des Rayonnements, BP-4346, F-31028 Toulouse, France (c) Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden (d) Southwest Research Institute, San Antonio, TX 7228-0510, USA (e) Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK (f) Space Physics Research Laboratory, University of Michigan, Ann Arbor, MI 48109-2143, USA (g) Space Science Laboratory, University of California in Berkeley, Berkeley, CA 94720-7450, USA (h) Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723-6099, USA (i) University of Arizona, Tucson, AZ 85721, USA (j) Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, UK (k) Space Technology Ltd., National University of Ireland, Maynooth, Co. Kildare, Ireland (l) Istituto di Fisica dello Spazio Interplanetari, I-00133 Rome, Italy (m) Physikalisches Institut, University of Bern, CH-3012 Bern, Switzerland (n) Max-Planck-Institut fur Aeronomie, D-37191 Katlenburg-Lindau, German (o) Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamichara, Japan (p) Technical University of Braunschweig, Hans-Sommer-Strasse 66, D-38106 Braunschweig, Germany (q) Department of Physical Sciences, University of Helsinki, P.O. Box 64, FIN-00014 Helsinki, Finland Article History: Received 19 April 2005; Revised 12 September 2005