Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3174
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dc.contributor.authorRadeta, Markoen_US
dc.contributor.authorBehboodi, Zahraen_US
dc.contributor.authorZeković, Vladimiren_US
dc.contributor.authorAlves, Décioen_US
dc.contributor.authorPestana, Daviden_US
dc.contributor.authorNunes, Danielen_US
dc.contributor.authorFreitas, Margaridaen_US
dc.contributor.authorGupta, Ankiten_US
dc.contributor.authorPestana, Joãoen_US
dc.contributor.authorVieira, Dinarteen_US
dc.contributor.authorAlmeida, Sílviaen_US
dc.contributor.authorDias, Morgadoen_US
dc.contributor.authorClode, João Canningen_US
dc.contributor.authorCaldeira, Ruien_US
dc.contributor.authorRelvas, Pauloen_US
dc.contributor.authorVasiljevic, Antonioen_US
dc.date.accessioned2026-02-10T16:57:40Z-
dc.date.available2026-02-10T16:57:40Z-
dc.date.issued2026-04-01-
dc.identifier.issn09670637-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3174-
dc.description.abstractSubsurface observations are crucial for understanding the ocean's role in Earth's climate and for refining climate models. However, existing aquatic monitoring systems that allow such insights remain complex and costly due to their high demands for deployment, sampling, and recapture. Since low-cost, easy-to-deploy deep-sea landers are scarce, and with the aim of facilitating more subsurface observations, this study provides a simple method for georeferencing small-sized untethered landers. Their underwater trajectories are modelled with fundamental physics, dead reckoning, lander geometry, and numerical simulations. Using free fall, upthrust, and ocean current dynamics, the proposed approach estimates their underwater trajectories, including landing (at the seabed) and pop (at the sea surface) points. The method relies on the lander's physical characteristics, including its vertical and horizontal cross-sectional areas, to calculate the drag force coefficients used to determine its trajectories during descent and ascent through the water column. Ocean currents' magnitudes are modelled using Ekman's exponential decay down to 90 m of the water column, while the depths until 900 m are modelled from prior ADCP surveys by varying ocean current headings with depth between −20 and 20°. Surface ocean and wind current headings are modelled with open datasets from satellite telemetry. Lander's velocity, displacement, and dive time to the landing and pop points, including the total radial excursion and uncertainty in heading, are analytically derived, numerically calculated, and empirically assessed a-posteriori until 90 m, yielding a ∼38 m radial excursion (40% error) against the obtained GNSS coordinates in field deployment, and 33° in heading uncertainty during a 138-s excursion. Additional random walk simulations are shown for full ocean depth obtaining radial excursion of 1038 m with 278 min total dive time. This approach is generalizable to any subsurface aquatic monitoring systems targeting deployments with diverse payloads from smaller sea vessels, not requiring cranes, radio, GNSS, or acoustic telemetry. Since it accounts for key nature factors, our method provides special benefits in planning and optimizing deployments. Additional discussion focuses on the method's practicality for full ocean depth deployments.en_US
dc.language.isoenen_US
dc.publisherElsevieren_US
dc.relation.ispartofDeep Sea Research Part I Oceanographic Research Papersen_US
dc.subjectDead reckoningen_US
dc.subjectHydrodynamicsen_US
dc.subjectLander geometryen_US
dc.subjectLow-cost landersen_US
dc.subjectNumerical simulationsen_US
dc.subjectOcean physicsen_US
dc.subjectRadial excursion predictionen_US
dc.subjectUnderwater trajectoriesen_US
dc.subjectUpper ocean dynamicsen_US
dc.subjectWater column monitoringen_US
dc.titleMARS lander: Georeferencing landing and pop points of untethered ocean monitoring systems using fundamental physicsen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.dsr.2026.104650-
dc.identifier.scopus2-s2.0-105029022164-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/105029022164-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0967-0637en_US
dc.description.rankM22en_US
dc.relation.firstpageArticle no. 104650en_US
dc.relation.volume228en_US
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.languageiso639-1en-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-4985-3253-
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