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AI-driven surface mapping and explainable AI for climate insights on Mars

Fanara, Lida und Su, Shu und Martynchuk, Oleksii und Hauber, Ernst und Gwinner, Klaus (2024) AI-driven surface mapping and explainable AI for climate insights on Mars. Europlanet Science Congress 2024, 2024-09-08 - 2024-09-13, Berlin, Germany. doi: 10.5194/epsc2024-948.

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Offizielle URL: https://meetingorganizer.copernicus.org/EPSC2024/EPSC2024-948.html

Kurzfassung

We are deriving insights about the climate evolution of Mars by automating surface mapping and monitoring with AI models. We are also analysing these models’ uncertainty and decision-making process with explainable AI and uncertainty estimation techniques. We focus on ice block fall detection at the north polar region and polygon detection globally. The north polar ice cap on Mars is comprised of ice layers relating to the climate cycles of Mars and this way it preserves a ∼ 4 million years climate change record of the planet. These layers are exposed at the marginal steep scarps of the cap, that are currently active with avalanches and block falls. We are monitoring the mass wasting activity at the north polar region by detecting ice blocks [1] and their sources [2]. We estimate the current erosion rates of all scarps resulting in a detailed map of how this extensive ice-layered dome is being shaped today. At the mid-latitude regions, where large volumes of excess ice exist, young patterned ground resembles glacial and periglacial patterns on Earth. Can freeze-thaw cycles have recently thawed the permafrost on Mars to produce these landforms? This would have implications for the recent hydrologic past of the planet. We detect young ice-wedge polygons to determine their distribution and relationship to the topography with the potential of elucidating the formation mechanism and the role of liquid water in the recent past of Mars. We use AI models to automate surface mapping and monitoring, because they outperform all other methods. However, they are treated as black box systems. We want to know why a model produces a specific response and how certain it is about the correctness of each result. To answer these questions, we put together an application-independent framework that deploys uncertainty estimation and explainable AI methods to provide insights into the decision-making process and assess the uncertainty of the results [3], in this project the uncertainty of the surface mapping.

elib-URL des Eintrags:https://elib.dlr.de/211452/
Dokumentart:Konferenzbeitrag (Vortrag)
Titel:AI-driven surface mapping and explainable AI for climate insights on Mars
Autoren:
AutorenInstitution oder E-Mail-AdresseAutoren-ORCID-iDORCID Put Code
Fanara, LidaLida.Fanara (at) dlr.dehttps://orcid.org/0000-0003-2677-2503NICHT SPEZIFIZIERT
Su, Shushu.su (at) campus.tu-berlin.dehttps://orcid.org/0000-0002-7122-9393NICHT SPEZIFIZIERT
Martynchuk, OleksiiOleksii.Martynchuk (at) dlr.deNICHT SPEZIFIZIERTNICHT SPEZIFIZIERT
Hauber, ErnstErnst.Hauber (at) dlr.dehttps://orcid.org/0000-0002-1375-304XNICHT SPEZIFIZIERT
Gwinner, KlausKlaus.Gwinner (at) dlr.deNICHT SPEZIFIZIERTNICHT SPEZIFIZIERT
Datum:2024
Referierte Publikation:Nein
Open Access:Ja
Gold Open Access:Nein
In SCOPUS:Nein
In ISI Web of Science:Nein
Band:17
DOI:10.5194/epsc2024-948
Seitenbereich:EPSC2024-948
Name der Reihe:EPSC Abstracts
Status:veröffentlicht
Stichwörter:Mars, climate, ice, polar regions, explainable AI, artificial intelligence, machine learning
Veranstaltungstitel:Europlanet Science Congress 2024
Veranstaltungsort:Berlin, Germany
Veranstaltungsart:internationale Konferenz
Veranstaltungsbeginn:8 September 2024
Veranstaltungsende:13 September 2024
Veranstalter :Europlanet Society
HGF - Forschungsbereich:Luftfahrt, Raumfahrt und Verkehr
HGF - Programm:Raumfahrt
HGF - Programmthema:Robotik
DLR - Schwerpunkt:Raumfahrt
DLR - Forschungsgebiet:R RO - Robotik
DLR - Teilgebiet (Projekt, Vorhaben):R - Planetare Exploration, R - Planetary Evolution and Life
Standort: Berlin-Adlershof
Institute & Einrichtungen:Institut für Planetenforschung > Planetengeodäsie
Institut für Planetenforschung > Planetengeologie
Hinterlegt von: Hauber, Ernst
Hinterlegt am:07 Jan 2025 10:25
Letzte Änderung:07 Jan 2025 10:25

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