{"year":"2017","publication":"Astronomy & Astrophysics","doi":"10.1051/0004-6361/201730801","has_accepted_license":"1","volume":608,"title":"Radar backscattering from a large-grain cometary coma: numerical simulation","department":[{"_id":"61"}],"publication_status":"published","citation":{"ama":"Dogra S, Grynko Y, Zubko E, Förstner J. Radar backscattering from a large-grain cometary coma: numerical simulation. Astronomy & Astrophysics. 2017;608:A20. doi:10.1051/0004-6361/201730801","ieee":"S. Dogra, Y. Grynko, E. Zubko, and J. Förstner, “Radar backscattering from a large-grain cometary coma: numerical simulation,” Astronomy & Astrophysics, vol. 608, p. A20, 2017.","mla":"Dogra, Shraddha, et al. “Radar Backscattering from a Large-Grain Cometary Coma: Numerical Simulation.” Astronomy & Astrophysics, vol. 608, EDP Sciences, 2017, p. A20, doi:10.1051/0004-6361/201730801.","apa":"Dogra, S., Grynko, Y., Zubko, E., & Förstner, J. (2017). Radar backscattering from a large-grain cometary coma: numerical simulation. Astronomy & Astrophysics, 608, A20. https://doi.org/10.1051/0004-6361/201730801","chicago":"Dogra, Shraddha, Yevgen Grynko, Evgenij Zubko, and Jens Förstner. “Radar Backscattering from a Large-Grain Cometary Coma: Numerical Simulation.” Astronomy & Astrophysics 608 (2017): A20. https://doi.org/10.1051/0004-6361/201730801.","short":"S. Dogra, Y. Grynko, E. Zubko, J. Förstner, Astronomy & Astrophysics 608 (2017) A20.","bibtex":"@article{Dogra_Grynko_Zubko_Förstner_2017, title={Radar backscattering from a large-grain cometary coma: numerical simulation}, volume={608}, DOI={10.1051/0004-6361/201730801}, journal={Astronomy & Astrophysics}, publisher={EDP Sciences}, author={Dogra, Shraddha and Grynko, Yevgen and Zubko, Evgenij and Förstner, Jens}, year={2017}, pages={A20} }"},"user_id":"158","language":[{"iso":"eng"}],"_id":"3523","oa":"1","date_updated":"2022-01-06T06:59:21Z","type":"journal_article","file":[{"file_id":"3903","content_type":"application/pdf","date_updated":"2018-09-03T14:05:33Z","access_level":"open_access","date_created":"2018-08-14T10:17:27Z","file_size":1206283,"file_name":"2017-10 Dogra,Grynko,Zubko,Förstner_Radar backscattering from large scale cometary coma-Numerical simulation_Astronomy and Astrophysics.pdf","creator":"hclaudia","relation":"main_file"}],"urn":"35230","author":[{"full_name":"Dogra, Shraddha","last_name":"Dogra","first_name":"Shraddha"},{"id":"26059","full_name":"Grynko, Yevgen","last_name":"Grynko","first_name":"Yevgen"},{"first_name":"Evgenij","last_name":"Zubko","full_name":"Zubko, Evgenij"},{"full_name":"Förstner, Jens","id":"158","orcid":"0000-0001-7059-9862","first_name":"Jens","last_name":"Förstner"}],"date_created":"2018-07-10T10:19:01Z","page":"A20","status":"public","ddc":["530"],"intvolume":" 608","keyword":["tet_topic_scattering"],"article_type":"original","publisher":"EDP Sciences","file_date_updated":"2018-09-03T14:05:33Z","abstract":[{"text":"We numerically simulate the circular polarization ratio of the radar signal backscattered from a large-grain cometary coma and compare the simulation results with the radar measurements for seven comets. We apply the discrete dipole approximation method and a model of random irregular particles. Our results confirm water ice composition of the cm-sized chunks detected by the NASA Deep Impact space probe in the vicinity of the nucleus of Comet 103P/Hartley 2. The index of the power-law size distribution in this case can be constrained to the range n ≈ 3.3–4.3. For the other considered comets the circular polarization ratio can be reproduced with variations of the power index between 2 and 5.","lang":"eng"}],"publication_identifier":{"issn":["0004-6361","1432-0746"]}}