Search Publications
Clouds and Aerosols on the Terrestrial Planets
Kahre, M. A.; Esposito, L. W.; Colaprete, A. +2 more
Distribution of magnetic fields in the quiet Sun
Faurobert, M.; Ricort, G.
Context. The distribution of magnetic fields in the atmosphere of the quiet Sun has been extensively studied with various methods, but it is still a matter of debate. Previous analyses mostly rely on the inversion of spectro-polarimetric data and different methods lead to somewhat different results.
Aims: Here we do not intend to determine th…
Observability of YSOs with the WISE and AKARI infrared space observatories
Tamura, M.; Marton, G.; Ueno, M. +4 more
Large area surveys allow us to identify young stellar objects and classify them based on their colours. The near-, mid- and far-infrared filters' sensitivities are different, therefore different proportions of young stars are observable. Evolutionary times for the different classes can be concluded from the popularity of the classes. Our aim was t…
Cassini High Rate Detector V12.0
Economou, T.; DiDonna, P.
The High Rate Detector (HRD) from the University of Chicago is an independent part of the CDA instrument on the Cassini Orbiter that measures the dust flux and particle mass distribution of dust particles hitting the HRD detectors. This data set includes all data from the HRD through December 31, 2012. Please refer to Srama et al. (2004) for a det…
Sunyaev-Zel'dovich effect or not ? detecting the main foreground effect of most galaxy clusters.
Zhang, B.; Wu, Y.; Xiao, W. +2 more
Galaxy clusters are the most massive objects in the Universe and comprise a high-temperature intracluster medium of about 107 K, believed to offer a main foreground effect for cosmic microwave background (CMB) data in the form of the thermal Sunyaev-Zel'dovich (SZ) effect. This assumption has been confirmed by SZ signal detection in hun…
Gaskell Tethys Shape Model V1.0
Gaskell, R. W.
The shape model of Tethys derived by Robert Gaskell from Cassini Imaging Science Subsystem narrow and wide angle camera (ISSNA and ISSWA) images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 25, 2012. Vertex-facet versions of the models are also provided.