dc.contributor.author | Sánchez Lavega, Agustín María ![ORCID](/themes/Mirage2//images/orcid_16x16.png) | |
dc.contributor.author | Erkoreka Pérez, Aitor | |
dc.contributor.author | Hernández Bernal, Jorge | |
dc.contributor.author | Del Río Gaztelurrutia, María Teresa | |
dc.contributor.author | García Morales, Josu | |
dc.contributor.author | Ordoñez Etxeberria, Iñaki ![ORCID](/themes/Mirage2//images/orcid_16x16.png) | |
dc.contributor.author | Cardesín-Moinelo, Alejandro | |
dc.contributor.author | Titov, Dimitri | |
dc.contributor.author | Wood, Simon | |
dc.contributor.author | Tirsch, Daniela | |
dc.contributor.author | Hauber, E. | |
dc.contributor.author | Matz, Klaus-Dieter | |
dc.date.accessioned | 2024-05-24T15:05:34Z | |
dc.date.available | 2024-05-24T15:05:34Z | |
dc.date.issued | 2022-11 | |
dc.identifier.citation | Icarus 387 : (2022) // Article ID 115183 | es_ES |
dc.identifier.issn | 1090-2643 | |
dc.identifier.issn | 0019-1035 | |
dc.identifier.uri | http://hdl.handle.net/10810/68156 | |
dc.description.abstract | We present a study of textured local dust storms that develop at the northern polar cap boundary on Mars springtime. We have used images obtained with VMC and HRSC cameras onboard Mars Express and MARCI on MRO to analyze dust storms captured from March to July 2019 (Ls = 350° in MY 34–Ls = 54° in MY 35). The textured storms grow in the longitude sector 150°E-210°E centered at latitude ~60°N and exhibit spiral, filamentary and compact shapes that change and evolve rapidly in a daily basis. The storms translate by prevailing east and southeast winds with speeds 15–45 ms−1. In some areas of their interiors they show organized clusters of cells formed typically by 100 elements with sizes ~5–30 km with a length/width ratio ~ 1.2–3 in the wind direction. The cells have elongated downwind tails with lengths 4–8 times the cell size. The cells top altitudes are ~6–11 km above their surroundings. We propose that the spirals grow as baroclinic vortices within a vertically sheared eastward jet present at this epoch in Mars due to the intense meridional temperature gradient at the polar cap edge. We show using a simple one-dimensional model that the cells can be produced by shallow dry convection with dust acting as the heating source to generate the updrafts. These patterns resemble those seen in laboratory experiments and on clouds in Earth's atmosphere and can serve to comparatively elucidate and discern the different mechanisms at work in each case. | es_ES |
dc.description.sponsorship | This work has been supported by the Spanish project PID2019-109467GB-I00 (MINECO/FEDER, UE) and Grupos Gobierno Vasco IT- 1742-22. JHB was supported by ESA Contract No. 4000118461/16/ES/JD, Scientific Support for Mars Express Visual Monitoring Camera. The Aula EspaZio Gela is supported by a grant from the Diputación Foral de Bizkaia (BFA). We acknowledge support from the Faculty of the European Space Astronomy Center (ESAC). Special thanks are due to the Mars Express Science Ground Segment and Flight Control Team at ESAC and ESOC. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | Elsevier | es_ES |
dc.relation | info:eu-repo/grantAgreement/MICINN/PID2019-109467GB-I00 | es_ES |
dc.rights | info:eu-repo/semantics/openAccess | es_ES |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ | * |
dc.subject | Mars | es_ES |
dc.subject | atmospheric dynamics | es_ES |
dc.subject | dust storms | es_ES |
dc.subject | cellular convection | es_ES |
dc.title | Cellular patterns and dry convection in textured dust storms at the edge of Mars North Polar Cap | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.rights.holder | © 2022 The Authors. Published by Elsevier Inc. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-
nc-nd/4.0/). | es_ES |
dc.rights.holder | Atribución-NoComercial-SinDerivadas 3.0 España | * |
dc.relation.publisherversion | https://www.sciencedirect.com/science/article/pii/S0019103522002846 | es_ES |
dc.identifier.doi | 10.1016/j.icarus.2022.115183 | |
dc.departamentoes | Física | es_ES |
dc.departamentoes | Física aplicada I | es_ES |
dc.departamentoeu | Fisika | es_ES |
dc.departamentoeu | Fisika aplikatua I | es_ES |