{"has_accepted_license":"1","status":"public","volume":608,"ddc":["530"],"user_id":"158","publisher":"EDP Sciences","_id":"3523","urn":"35230","page":"A20","citation":{"mla":"Dogra, Shraddha, et al. “Radar Backscattering from a Large-Grain Cometary Coma: Numerical Simulation.” <i>Astronomy &#38; Astrophysics</i>, vol. 608, EDP Sciences, 2017, p. A20, doi:<a href=\"https://doi.org/10.1051/0004-6361/201730801\">10.1051/0004-6361/201730801</a>.","ama":"Dogra S, Grynko Y, Zubko E, Förstner J. Radar backscattering from a large-grain cometary coma: numerical simulation. <i>Astronomy &#38; Astrophysics</i>. 2017;608:A20. doi:<a href=\"https://doi.org/10.1051/0004-6361/201730801\">10.1051/0004-6361/201730801</a>","bibtex":"@article{Dogra_Grynko_Zubko_Förstner_2017, title={Radar backscattering from a large-grain cometary coma: numerical simulation}, volume={608}, DOI={<a href=\"https://doi.org/10.1051/0004-6361/201730801\">10.1051/0004-6361/201730801</a>}, journal={Astronomy &#38; Astrophysics}, publisher={EDP Sciences}, author={Dogra, Shraddha and Grynko, Yevgen and Zubko, Evgenij and Förstner, Jens}, year={2017}, pages={A20} }","apa":"Dogra, S., Grynko, Y., Zubko, E., &#38; Förstner, J. (2017). Radar backscattering from a large-grain cometary coma: numerical simulation. <i>Astronomy &#38; Astrophysics</i>, <i>608</i>, A20. <a href=\"https://doi.org/10.1051/0004-6361/201730801\">https://doi.org/10.1051/0004-6361/201730801</a>","ieee":"S. Dogra, Y. Grynko, E. Zubko, and J. Förstner, “Radar backscattering from a large-grain cometary coma: numerical simulation,” <i>Astronomy &#38; Astrophysics</i>, vol. 608, p. A20, 2017.","short":"S. Dogra, Y. Grynko, E. Zubko, J. Förstner, Astronomy &#38; Astrophysics 608 (2017) A20.","chicago":"Dogra, Shraddha, Yevgen Grynko, Evgenij Zubko, and Jens Förstner. “Radar Backscattering from a Large-Grain Cometary Coma: Numerical Simulation.” <i>Astronomy &#38; Astrophysics</i> 608 (2017): A20. <a href=\"https://doi.org/10.1051/0004-6361/201730801\">https://doi.org/10.1051/0004-6361/201730801</a>."},"file_date_updated":"2018-09-03T14:05:33Z","oa":"1","intvolume":"       608","article_type":"original","date_updated":"2022-01-06T06:59:21Z","publication_status":"published","publication_identifier":{"issn":["0004-6361","1432-0746"]},"author":[{"last_name":"Dogra","first_name":"Shraddha","full_name":"Dogra, Shraddha"},{"id":"26059","full_name":"Grynko, Yevgen","last_name":"Grynko","first_name":"Yevgen"},{"last_name":"Zubko","first_name":"Evgenij","full_name":"Zubko, Evgenij"},{"full_name":"Förstner, Jens","first_name":"Jens","orcid":"0000-0001-7059-9862","last_name":"Förstner","id":"158"}],"title":"Radar backscattering from a large-grain cometary coma: numerical simulation","year":"2017","doi":"10.1051/0004-6361/201730801","language":[{"iso":"eng"}],"abstract":[{"lang":"eng","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."}],"publication":"Astronomy & Astrophysics","department":[{"_id":"61"}],"type":"journal_article","keyword":["tet_topic_scattering"],"date_created":"2018-07-10T10:19:01Z","file":[{"date_created":"2018-08-14T10:17:27Z","creator":"hclaudia","file_id":"3903","content_type":"application/pdf","file_name":"2017-10 Dogra,Grynko,Zubko,Förstner_Radar backscattering from large scale cometary coma-Numerical simulation_Astronomy and Astrophysics.pdf","file_size":1206283,"access_level":"open_access","relation":"main_file","date_updated":"2018-09-03T14:05:33Z"}]}