ICARUS 129, 270±288 (1997) ARTICLE NO. IS975789 South±North and Radial Traverses through the Interplanetary Dust Cloud E. GruÈ n Max-Planck-Institut fuÈr Kernphysik, 69117 Heidelberg, Germany E-mail:
[email protected] P. Staubach ESA±ESOC, 64293 Darmstadt, Germany M. Baguhl Max-Planck-Institut fuÈr Kernphysik, 69117 Heidelberg, Germany D. P. Hamilton University of Maryland, College Park, Maryland 20742 H. A. Zook NASA Johnson Space Center, Houston, Texas 77058 S. Dermott and B. A. Gustafson University of Florida, Gainesville, Florida 32611 H. Fechtig, J. Kissel, D. Linkert, G. Linkert, and R. Srama Max-Planck-Institut fuÈr Kernphysik, 69117 Heidelberg, Germany M. S. Hanner and C. Polanskey Jet Propulsion Laboratory, Pasadena, California 91103 M. Horanyi Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Colorado B. A. Lindblad Lund Observatory, 221 Lund, Sweden I. Mann Max-Planck-Institut fuÈr Aeronomie, 37191 Katlenburg-Lindau, Germany J. A. M. McDonnell University of Kent, Canterbury CT2 7NR, United Kingdom G. E. Mor®ll Max-Planck-Institut fuÈr Extraterrestrische Physik, 85748 Garching, Germany and G. Schwehm ESA±ESTEC, 2200 AG Noordwijk, The Netherlands Received February 7, 1996; revised June 9, 1997 270 0019-1035/97 $25.00 Copyright 1997 by Academic Press All rights of reproduction in any form reserved. TRAVERSES THROUGH THE INTERPLANETARY DUST CLOUD 271 Identical in situ dust detectors are ¯own on board the Galileo and Ulysses spacecraft. They record impacts of micrometeor- oids in the ecliptic plane at heliocentric distances from 0.7 to 5.4 AU and in a plane almost perpendicular to the ecliptic from 2798 to 1798 ecliptic latitude.