{"id":297,"date":"2020-11-11T17:29:33","date_gmt":"2020-11-11T17:29:33","guid":{"rendered":"http:\/\/planetary-defense.eu\/?post_type=knowledgebase&#038;p=297"},"modified":"2021-01-08T16:40:34","modified_gmt":"2021-01-08T16:40:34","slug":"simulation-of-meteors-by-tc-libs-advantages-limits-and-challenges","status":"publish","type":"knowledgebase","link":"https:\/\/planetary-defense.eu\/?knowledgebase=simulation-of-meteors-by-tc-libs-advantages-limits-and-challenges","title":{"rendered":"Simulation of meteors by TC-LIBS: Advantages, limits and challenges"},"content":{"rendered":"\n<p><strong>Martin Ferus, Anna K\u0159ivkov\u00e1, Luk\u00e1\u0161 Petera, Vojt\u011bch Laitl, Libor Len\u017ea, Anton\u00edn Kn\u00ed\u017eek, Ji\u0159\u00ed Srba, Nikola Schmidt, Petr Boh\u00e1\u010dek, Svatopluk Civi\u0161, Miroslav Kr\u016fs, Jan Kub\u00e1t,<\/strong> <strong>Lucie Palou\u0161ov\u00e1, Elias Chatzitheodoridis, Petr Kubel\u00edk<\/strong><\/p>\n\n\n\n<p>Important features in meteor spectra are usually interpreted by synthetic convolution of lines extracted from databases. We developed new approach in this field: experimental techniques based on ablation of real meteorite samples using a wide range of laser sources. We performed experiments in order to provide spectra of several molecular, radical and molecular ion species that are likely to appear in meteor or cometary impact plasma. The spectra are recorded by high-resolution laboratory Echelle spectrograph and simultaneously using a high-resolution Meteor Spectral Camera for real meteor observation. In this manner, we show that instead of theoretical spectra simulation, laboratory experiments can be applied at least for qualitative evaluation of the observational data and assignment of important spectral features in meteor emission spectra. We also provide examination of ablation spots for future estimation of parameters of a high-power laser, which is used for remote LIBS applied in astronautics.<\/p>\n\n\n\n<div class=\"wp-block-uagb-buttons uagb-buttons__outer-wrap uagb-block-5e57e8dc\"><div class=\"uagb-buttons__wrap uagb-buttons-layout-wrap\">\n<div class=\"wp-block-uagb-buttons-child uagb-buttons__outer-wrap uagb-block-de0e4416\"><div class=\"uagb-button__wrapper\"><a class=\"uagb-buttons-repeater\" href=\"https:\/\/planetary-defense.eu\/wp-content\/uploads\/2020\/11\/23b-IMC2019-Ferus-et-al-1.0.pdf\" rel=\"noopener noreferrer\" target=\"_blank\"><div class=\"uagb-button__link\">DOWNLOAD<\/div><span class=\"uagb-button__icon uagb-button__icon-position-after\"><svg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 384 512\"><path d=\"M181.9 256.1c-5-16-4.9-46.9-2-46.9 8.4 0 7.6 36.9 2 46.9zm-1.7 47.2c-7.7 20.2-17.3 43.3-28.4 62.7 18.3-7 39-17.2 62.9-21.9-12.7-9.6-24.9-23.4-34.5-40.8zM86.1 428.1c0 .8 13.2-5.4 34.9-40.2-6.7 6.3-29.1 24.5-34.9 40.2zM248 160h136v328c0 13.3-10.7 24-24 24H24c-13.3 0-24-10.7-24-24V24C0 10.7 10.7 0 24 0h200v136c0 13.2 10.8 24 24 24zm-8 171.8c-20-12.2-33.3-29-42.7-53.8 4.5-18.5 11.6-46.6 6.2-64.2-4.7-29.4-42.4-26.5-47.8-6.8-5 18.3-.4 44.1 8.1 77-11.6 27.6-28.7 64.6-40.8 85.8-.1 0-.1.1-.2.1-27.1 13.9-73.6 44.5-54.5 68 5.6 6.9 16 10 21.5 10 17.9 0 35.7-18 61.1-61.8 25.8-8.5 54.1-19.1 79-23.2 21.7 11.8 47.1 19.5 64 19.5 29.2 0 31.2-32 19.7-43.4-13.9-13.6-54.3-9.7-73.6-7.2zM377 105L279 7c-4.5-4.5-10.6-7-17-7h-6v128h128v-6.1c0-6.3-2.5-12.4-7-16.9zm-74.1 255.3c4.1-2.7-2.5-11.9-42.8-9 37.1 15.8 42.8 9 42.8 9z\"><\/path><\/svg><\/span><\/a><\/div><\/div>\n<\/div><\/div>\n\n\n\n<div style=\"height:28px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<hr class=\"wp-block-separator is-style-wide\"\/>\n\n\n<div class=\"embed-pdf-viewer-wrapper aligncenter wp-block-embed-pdf-viewer-pdf\"><iframe loading=\"lazy\" class=\"embed-pdf-viewer\" src=\"https:\/\/planetary-defense.eu\/wp-content\/uploads\/2020\/11\/23b-IMC2019-Ferus-et-al-1.0.pdf\" height=\"1200\" width=\"1000\" title=\"\"><\/iframe><\/div>","protected":false},"excerpt":{"rendered":"<p>Martin Ferus, Anna K\u0159ivkov\u00e1, Luk\u00e1\u0161 Petera, Vojt\u011bch Laitl, Libor Len\u017ea, Anton\u00edn Kn\u00ed\u017eek, Ji\u0159\u00ed Srba, Nikola Schmidt, Petr Boh\u00e1\u010dek, Svatopluk Civi\u0161, Miroslav Kr\u016fs, Jan Kub\u00e1t, Lucie Palou\u0161ov\u00e1, Elias Chatzitheodoridis, Petr Kubel\u00edk Important features in meteor spectra are usually interpreted by synthetic convolution of lines extracted from databases. We developed new approach in this field: experimental techniques &hellip; <\/p>\n<p class=\"link-more\"><a href=\"https:\/\/planetary-defense.eu\/?knowledgebase=simulation-of-meteors-by-tc-libs-advantages-limits-and-challenges\" class=\"more-link\">Continue reading<span class=\"screen-reader-text\"> &#8220;Simulation of meteors by TC-LIBS: Advantages, limits and challenges&#8221;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","template":"","knowledgebase_cat":[9],"class_list":["post-297","knowledgebase","type-knowledgebase","status-publish","hentry","knowledgebase_cat-conference-papers"],"uagb_featured_image_src":{"full":false,"thumbnail":false,"medium":false,"medium_large":false,"large":false,"1536x1536":false,"2048x2048":false,"twentyseventeen-featured-image":false,"twentyseventeen-thumbnail-avatar":false},"uagb_author_info":{"display_name":"nicholas","author_link":"https:\/\/planetary-defense.eu\/?author=1"},"uagb_comment_info":0,"uagb_excerpt":"Martin Ferus, Anna K\u0159ivkov\u00e1, Luk\u00e1\u0161 Petera, Vojt\u011bch Laitl, Libor Len\u017ea, Anton\u00edn Kn\u00ed\u017eek, Ji\u0159\u00ed Srba, Nikola Schmidt, Petr Boh\u00e1\u010dek, Svatopluk Civi\u0161, Miroslav Kr\u016fs, Jan Kub\u00e1t, Lucie Palou\u0161ov\u00e1, Elias Chatzitheodoridis, Petr Kubel\u00edk Important features in meteor spectra are usually interpreted by synthetic convolution of lines extracted from databases. We developed new approach in this field: experimental techniques&hellip;","_links":{"self":[{"href":"https:\/\/planetary-defense.eu\/index.php?rest_route=\/wp\/v2\/knowledgebase\/297","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/planetary-defense.eu\/index.php?rest_route=\/wp\/v2\/knowledgebase"}],"about":[{"href":"https:\/\/planetary-defense.eu\/index.php?rest_route=\/wp\/v2\/types\/knowledgebase"}],"author":[{"embeddable":true,"href":"https:\/\/planetary-defense.eu\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/planetary-defense.eu\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=297"}],"version-history":[{"count":3,"href":"https:\/\/planetary-defense.eu\/index.php?rest_route=\/wp\/v2\/knowledgebase\/297\/revisions"}],"predecessor-version":[{"id":427,"href":"https:\/\/planetary-defense.eu\/index.php?rest_route=\/wp\/v2\/knowledgebase\/297\/revisions\/427"}],"wp:attachment":[{"href":"https:\/\/planetary-defense.eu\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=297"}],"wp:term":[{"taxonomy":"knowledgebase_cat","embeddable":true,"href":"https:\/\/planetary-defense.eu\/index.php?rest_route=%2Fwp%2Fv2%2Fknowledgebase_cat&post=297"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}