D. Möhlmann

TL;DR: The Cassini-Huygens Cosmic Dust Analyzer (CDA) is intended to provide direct observations of dust grains with masses between 10-19 and 10-9 kg in interplanetary space and in the jovian and satumian systems, to investigate their physical, chemical and dynamical properties as functions of the distances to the Sun, to Jupiter and to Saturn and its satellites and rings as mentioned in this paper.

TL;DR: The Cometary and Interstellar Dust Analyzer (CIDA) as mentioned in this paper analyzes the composition of individual grains in the cometary coma using a fast time-of-flight mass spectrometer.

TL;DR: In this paper, the authors focus on the analysis of impact rates, which were strongly variable primarily due to changes of the spacecraft pointing and the Cosmic Dust Analyser (CDA) data within Titan's orbit.

TL;DR: The German cosmic dust analyser (CDA) was developed under the leadership of the Max Planck Institute for Nuclear Physics in Heidelberg under the support of the DLR e.V..

TL;DR: The Cosmic Dust Analyzer (CDA) as mentioned in this paper measured the interplanetary, interstellar and planetary dust in our solar system since 1999 and provided unique discoveries, including the discovery of large reservoirs of liquid water (oceans) below the icy crust of Enceladus.