{"id":20652,"date":"2019-11-04T17:42:56","date_gmt":"2019-11-04T16:42:56","guid":{"rendered":"http:\/\/karmaka.de\/?p=20652"},"modified":"2019-11-04T17:43:08","modified_gmt":"2019-11-04T16:43:08","slug":"a-statistical-analysis-of-the-h-l-ratio-of-ordinary-chondrite-finds-and-falls-a-comparison-of-oman-finds-with-other-populations","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=20652","title":{"rendered":"A statistical analysis of the H\/L ratio of ordinary chondrite finds and falls: A comparison of Oman finds with other populations"},"content":{"rendered":"\n<p>Ioannis Kouvatsis, Beda A. Hofmann <\/p>\n\n\n\n<p>Meteoritics &amp; Planetary Science <\/p>\n\n\n\n<p><a href=\"https:\/\/onlinelibrary.wiley.com\/doi\/full\/10.1111\/maps.13410\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>LINK<\/strong><\/a><\/p>\n\n\n\n<p class=\"justify-text\">&#8220;Hot and cold deserts have been thoroughly searched for meteorites in the past decades, which has led to a large inventory of classified meteorites. H\u2010 and L\u2010chondrites are the most abundant meteorites in all collections, and many authors used the H\/L ratio as a characteristic parameter in comparing meteorite populations. H\/L ratios (after pairing) vary from 0.90 in observed falls up to 1.74 in El M\u00e9dano (Atacama Desert). In this study, we investigate the H\/L ratio of 965 unpaired H\u2010 and L\u2010chondrites collected in Oman and compare this population with observed falls and other hot desert collections. We find a mass dependence of the H\/L ratio among hot desert finds and identify mechanisms such as fragmentation during weathering and fall that have an impact on the H\/L ratio. We employ the Kolmogorov\u2013Smirnov and Mann\u2013Whitney U statistical tests to compare the mass distributions of H\u2010 and L\u2010chondrites and to test the relationship between the similarity of mass distributions and the H\/L ratio. We conclude that the variations of the H\/L ratios observed in various populations are a sampling artifact resulting from secondary effects and observational bias, expressed in differences of the H and L mass distributions which are not observed in falls, and not due to variations in H\/L of the meteorite flux. The H\/L ratio of 0.90 observed among recent falls is considered as most representative for the overall meteorite flux, at least since the Late Pleistocene.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Ioannis Kouvatsis, Beda A. Hofmann Meteoritics &amp; Planetary Science LINK &#8220;Hot and cold deserts have been thoroughly searched for meteorites in the past decades, which has led to a large inventory of classified meteorites. H\u2010&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,23,176,7],"tags":[2522,4852,5250,2898,3188,3548,5249,610,1807],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/20652"}],"collection":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=20652"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/20652\/revisions"}],"predecessor-version":[{"id":20653,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/20652\/revisions\/20653"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=20652"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=20652"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=20652"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}