TY  - JOUR
A1  - Meier, Patrick
A1  - Kriegel, Hendrik
A1  - Motschmann, Uwe
A1  - Schmidt, Jürgen
A1  - Spahn, Frank
A1  - Hill, Thomas W.
A1  - Dong, Yaxue
A1  - Jones, Geraint H.
T1  - A model of the spatial and size distribution of Enceladus' dust plume
JF  - Planetary and space science
KW  - Enceladus
KW  - Plume
KW  - Nanograins
KW  - Cassini
KW  - Tail
Y1  - 2014
U6  - https://doi.org/10.1016/j.pss.2014.09.016
SN  - 0032-0633
VL  - 104
SP  - 216
EP  - 233
PB  - Elsevier
CY  - Oxford
ER  - 
TY  - JOUR
A1  - Srama, Ralf
A1  - Kempf, S.
A1  - Moragas-Klostermeyer, Georg
A1  - Helfert, S.
A1  - Ahrens, T. J.
A1  - Altobelli, N.
A1  - Auer, S.
A1  - Beckmann, U.
A1  - Bradley, J. G.
A1  - Burton, M.
A1  - Dikarev, V. V.
A1  - Economou, T.
A1  - Fechtig, H.
A1  - Green, S. F.
A1  - Grande, M.
A1  - Havnes, O.
A1  - Hillierf, J.K.
A1  - Horanyii, M.
A1  - Igenbergsj, E.
A1  - Jessberger, E. K.
A1  - Johnson, T. V.
A1  - Krüger, H.
A1  - Matt, G.
A1  - McBride, N.
A1  - Mocker, A.
A1  - Lamy, P.
A1  - Linkert, D.
A1  - Linkert, G.
A1  - Lura, F.
A1  - McDonnell, J.A.M.
A1  - Möhlmann, D.
A1  - Morfill, G. E.
A1  - Postberg, F.
A1  - Roy, M.
A1  - Schwehm, G.H.
A1  - Spahn, Frank
A1  - Svestka, J.
A1  - Tschernjawski, V.
A1  - Tuzzolino, A. J.
A1  - Wäsch, R.
A1  - Grün, E.
T1  - In situ dust measurements in the inner Saturnian system
JF  - Planetary and space science
N2  - In July 2004 the Cassini–Huygens mission reached the Saturnian system and started its orbital tour. A total of 75 orbits will be carried out during the primary mission until August 2008. In these four years Cassini crosses the ring plane 150 times and spends approx. 400 h within Titan's orbit. The Cosmic Dust Analyser (CDA) onboard Cassini characterises the dust environment with its extended E ring and embedded moons. Here, we focus on the CDA results of the first year and we present the Dust Analyser (DA) data within Titan's orbit. This paper does investigate High Rate Detector data and dust composition measurements. The authors focus on the analysis of impact rates, which were strongly variable primarily due to changes of the spacecraft pointing. An overview is given about the ring plane crossings and the DA counter measurements. The DA dust impact rates are compared with the DA boresight configuration around all ring plane crossings between June 2004 and July 2005. Dust impacts were registered at altitudes as high as 100 000 km above the ring plane at distances from Saturn between 4 and 10 Saturn radii. In those regions the dust density of particles bigger than 0.5 can reach values of 0.001m-3.
KW  - Cassini
KW  - dust
KW  - CDA
KW  - E-ring
KW  - water ice
Y1  - 2006
U6  - https://doi.org/10.1016/j.pss.2006.05.021
SN  - 0032-0633
VL  - 54
IS  - 9-10
SP  - 967
EP  - 987
PB  - Elsevier
CY  - Oxford
ER  -