Germany / Netherlands / Norway / France / Russia / United States / United Kingdom / / /
Facility
University of Mannheim / Open University / Prague Observatory / University of Potsdam / Astronomy Institute of St. Petersburg State University / University of Chicago / University of Tromso / Rutherford Appleton Laboratory / Seismological Laboratory / Enrico Fermi Institute / University of Hawaii / Walton Hall / /
IndustryTerm
planetary ring systems / in-situ chemical analysis / µm thick stainless steel meteoroid penetration sensor / jovian and saturnian systems / remote chemical analyses / dust chemical composition / Chemical composition / chemical and molecular composition / neutral gas / energy distribution / chemical and dynamical properties / /
OperatingSystem
Fermi / /
Organization
University of Potsdam / Astronomy Institute / Open University / Laboratory for Atmospheric and Space Physics / University of Chicago / Chicago / STARDUST mission / University of Mannheim / Seismological Laboratory / Space Science Research Institut / Planetary and Space Science Division / University of Tromso / Rutherford Appleton Laboratory / Max-Planck-Institut f¨ur Kernphysik / Enrico Fermi Institute / African Union / ESA / St. Petersburg State University / University of Hawaii / National Aeronautics and Space Administration / Cassini-Huygens mission / Max-Planck-Institut / Post Office / /
Person
Milton Keynes / Galileo / Ulysses / /
Position
Author / model / /
Product
Voyager / /
ProvinceOrState
Texas / Virginia / Alabama / Illinois / Hawaii / California / Colorado / /
THE CASSINI COSMIC DUST ANALYZER R. SRAMA1,∗ , T. J. AHRENS3 , N. ALTOBELLI1 , S. AUER4 , J. G. BRADLEY2 , 11 ¨ M. BURTON2 , V. V. DIKAREV1,21 , T. ECONOMOU5 , H. FECHTIG1 , M. GORLICH ,