No CrossRef data available.
Published online by Cambridge University Press: 14 August 2015
Observations of the scattered sunlight and thermal emission from cometary dust provide information on the composition and dominant size of the dust. The observations will be summarized here and compared to theoretical models for dielectric and absorbing materials, with emphasis on the thermal emission. The compatibility of the optical data with the size distribution derived from dynamical studies is discussed.
Full text views reflects PDF downloads, PDFs sent to Google Drive, Dropbox and Kindle and HTML full text views.
* Views captured on Cambridge Core between September 2016 - 19th January 2021. This data will be updated every 24 hours.