Bussoletti, E. and Colangeli, L. and Moreno, J.J.L. and Epifani, E. and Mennella, V. and Palomba, E. and Palumbo, P. and Rotundi, A. and Vergara, S. and Girela, F. and Herranz, M. and Jeronimo, J.M. and Lopez-Jimenez, A.C. and Molina, A. and Moreno, F. and Olivares, I. and Rodrigo, R. and Rodriguez-Gomez, J.F. and Sanchez, J. and Mc Donnell, J.A.M. and Leese, M.R. and Lamy, P. and Perruchot, S. and Crifo, J.F. and Fulle, M. and Perrin, J.M. and Angrilli, F. and Benini, E. and Casini, L. and Cherubini, G. and Coradini, A. and Giovane, F. and Grun, E. and Gustafson, B.A. and Maag, C. and Weissmann, P.R. (1998) The GIADA experiment for ROSETTA mission to comet 46P/Wirtanen: Design and performances. In: Lamy, P. and Thomas, N., eds. EXPLORATION OF SMALL BODIES IN THE SOLAR SYSTEM: I. INITIAL RESULTS AND FUTURE PROSPECTS. ADVANCES IN SPACE RESEARCH, 24. Pergamon Press Ltd, Japan pp. 1139-1148.
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Rosetta is one of the most ambitious missions planned by ESA for the beginning of the next millennium. It will explore from very close a comet nucleus along its trajectory up to perihelion. In the instrument complex forming the scientific payload, the GIADA (Grain Impact Analyser and Dust Accumulator) experiment is devoted to study the cometary dust flux evolution and grain dynamic properties. To achieve the required performances and the expected scientific return, GIADA has been designed as a multi-sensor instrument. It is able to detect grain passage by laser light scattering measurement, particle momentum through piezoelectric transducers and mass flux by means of quartz crystal microbalances. In this paper we describe the technical solutions and performances which have been reached on the development models of GIADA. (C) 1999 COSPAR. Published by Elsevier Science Ltd.
|Item Type:||Conference or workshop item (Paper)|
|Subjects:||Q Science > QC Physics|
|Divisions:||Faculties > Science Technology and Medical Studies > School of Physical Sciences|
|Depositing User:||M. Nasiriavanaki|
|Date Deposited:||03 Jul 2009 06:38|
|Last Modified:||12 Jun 2012 15:27|
|Resource URI:||http://kar.kent.ac.uk/id/eprint/17158 (The current URI for this page, for reference purposes)|
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