Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/367
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dc.contributor.authorĆurić, M.en
dc.contributor.authorJanc, Dejanen
dc.date.accessioned2022-07-12T15:23:42Z-
dc.date.available2022-07-12T15:23:42Z-
dc.date.issued1996-01-01en
dc.identifier.issn0941-2948en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/367-
dc.description.abstractThe sensitivity of modeled hail accretion rates on the lower boundary of the hail size spectrum is investigated. Two different expressions for hail terminal velocity are considered: New hail accretion rates consider only hail size particles greater or equal than 0.5 cm (corresponding to the real spectrum); these rates are compared with those derived from an idealized hail spectrum with diameters from 0 to ∞. Sensitivity tests show clearly that the errors in the computation of accretion can be minimized by using the new accretion rates. New accretion rates can differ up to a factor of 77.6 from those based on the idealized spectrum. In addition, it is shown that the accretion rate is sensitive to the expression used for the hail terminal velocity. © by Gebrüder Borntraeger 1996.en
dc.relation.ispartofMeteorologische Zeitschriften
dc.titleSensitivity of modeled hail accretion rates on the lower boundary of the hail spectrumen
dc.typeArticleen
dc.identifier.doi10.1127/metz/5/1996/51en
dc.identifier.scopus2-s2.0-0042425934en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/0042425934en
dc.relation.issue2en
dc.relation.volume5en
dc.relation.firstpage51en
dc.relation.lastpage59en
item.openairetypeArticle-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
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