ExoMars – WISDOM Field-Test Data Processed with Automatic Pipeline

International audience The ExoMars Rover instrument WISDOM (“Water Ice and Subsurface Deposit Observations on Mars”) is a ground penetrating radar (GPR) designed to investigate the shallow subsurface of Oxia Planum, the ExoMars mission’s designated landing site. Using a frequency range from 0.5 GHz...

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Main Authors: Plettemeier, Dirk, Benedix, Wolf-Stefan, Hegler, Sebastian, Hahnel, Ronny, Statz, Christoph, Lu, Yun, Ciarletti, Valérie, Brighi, Emile, Le Gall, Alice, Sall, Issa, Mas, Esther, Shestov, Aleksey
Other Authors: Technische Universität Dresden = Dresden University of Technology (TU Dresden), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich), The University Centre in Svalbard (UNIS)
Format: Conference Object
Language:English
Published: HAL CCSD 2023
Subjects:
Online Access:https://insu.hal.science/insu-04015250
https://doi.org/10.5194/egusphere-egu23-16376
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spelling ftuniversailles:oai:HAL:insu-04015250v1 2023-12-31T10:23:32+01:00 ExoMars – WISDOM Field-Test Data Processed with Automatic Pipeline Plettemeier, Dirk Benedix, Wolf-Stefan Hegler, Sebastian Hahnel, Ronny Statz, Christoph Lu, Yun Ciarletti, Valérie Brighi, Emile Le Gall, Alice Sall, Issa Mas, Esther Shestov, Aleksey Technische Universität Dresden = Dresden University of Technology (TU Dresden) PLANETO - LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich) The University Centre in Svalbard (UNIS) Vienna (Austria), Austria 2023-09 https://insu.hal.science/insu-04015250 https://doi.org/10.5194/egusphere-egu23-16376 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/doi/10.5194/egusphere-egu23-16376 insu-04015250 https://insu.hal.science/insu-04015250 doi:10.5194/egusphere-egu23-16376 EGU General Assembly 2023 https://insu.hal.science/insu-04015250 EGU General Assembly 2023, Sep 2023, Vienna (Austria), Austria. pp.EGU23-16376, ⟨10.5194/egusphere-egu23-16376⟩ [SDU]Sciences of the Universe [physics] info:eu-repo/semantics/conferenceObject Conference papers 2023 ftuniversailles https://doi.org/10.5194/egusphere-egu23-16376 2023-12-05T23:40:29Z International audience The ExoMars Rover instrument WISDOM (“Water Ice and Subsurface Deposit Observations on Mars”) is a ground penetrating radar (GPR) designed to investigate the shallow subsurface of Oxia Planum, the ExoMars mission’s designated landing site. Using a frequency range from 0.5 GHz to 3.0 GHz the electromagnetic waves penetrate the subsurface via a wideband antenna assembly. The achieved penetration depth is at least three meters, with a depth resolution of a few centimeters. The dual-polarimetric design of the antenna allows to measure four different channels during probing the Mars soil.The WISDOM radar will give access to the geological structure, electromagnetic nature, and possibly hydrological state of the shallow subsurface by retrieving the layering and properties of the buried reflectors. A short-term subsurface analysis will support the tight schedules of the rover operations both for science and drill operations in finding places of high scientific interest and low risk.In order to achieve these short times for decision making the incoming data at the remote operation control center (ROCC) will be automatically processed through a predefined pipeline. The processing is written in Python, which uses a self-developed framework. The basic process consists of a chain of filters that produces several radargrams at different states of processing. Further, it prepares the data for storage in PDS4 format for long-term archiving.In this work, automatic processing is introduced and results of processed measurement data acquired during a WISDOM field test in Svalbard are presented. Conference Object Svalbard Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQ
institution Open Polar
collection Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQ
op_collection_id ftuniversailles
language English
topic [SDU]Sciences of the Universe [physics]
spellingShingle [SDU]Sciences of the Universe [physics]
Plettemeier, Dirk
Benedix, Wolf-Stefan
Hegler, Sebastian
Hahnel, Ronny
Statz, Christoph
Lu, Yun
Ciarletti, Valérie
Brighi, Emile
Le Gall, Alice
Sall, Issa
Mas, Esther
Shestov, Aleksey
ExoMars – WISDOM Field-Test Data Processed with Automatic Pipeline
topic_facet [SDU]Sciences of the Universe [physics]
description International audience The ExoMars Rover instrument WISDOM (“Water Ice and Subsurface Deposit Observations on Mars”) is a ground penetrating radar (GPR) designed to investigate the shallow subsurface of Oxia Planum, the ExoMars mission’s designated landing site. Using a frequency range from 0.5 GHz to 3.0 GHz the electromagnetic waves penetrate the subsurface via a wideband antenna assembly. The achieved penetration depth is at least three meters, with a depth resolution of a few centimeters. The dual-polarimetric design of the antenna allows to measure four different channels during probing the Mars soil.The WISDOM radar will give access to the geological structure, electromagnetic nature, and possibly hydrological state of the shallow subsurface by retrieving the layering and properties of the buried reflectors. A short-term subsurface analysis will support the tight schedules of the rover operations both for science and drill operations in finding places of high scientific interest and low risk.In order to achieve these short times for decision making the incoming data at the remote operation control center (ROCC) will be automatically processed through a predefined pipeline. The processing is written in Python, which uses a self-developed framework. The basic process consists of a chain of filters that produces several radargrams at different states of processing. Further, it prepares the data for storage in PDS4 format for long-term archiving.In this work, automatic processing is introduced and results of processed measurement data acquired during a WISDOM field test in Svalbard are presented.
author2 Technische Universität Dresden = Dresden University of Technology (TU Dresden)
PLANETO - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich)
The University Centre in Svalbard (UNIS)
format Conference Object
author Plettemeier, Dirk
Benedix, Wolf-Stefan
Hegler, Sebastian
Hahnel, Ronny
Statz, Christoph
Lu, Yun
Ciarletti, Valérie
Brighi, Emile
Le Gall, Alice
Sall, Issa
Mas, Esther
Shestov, Aleksey
author_facet Plettemeier, Dirk
Benedix, Wolf-Stefan
Hegler, Sebastian
Hahnel, Ronny
Statz, Christoph
Lu, Yun
Ciarletti, Valérie
Brighi, Emile
Le Gall, Alice
Sall, Issa
Mas, Esther
Shestov, Aleksey
author_sort Plettemeier, Dirk
title ExoMars – WISDOM Field-Test Data Processed with Automatic Pipeline
title_short ExoMars – WISDOM Field-Test Data Processed with Automatic Pipeline
title_full ExoMars – WISDOM Field-Test Data Processed with Automatic Pipeline
title_fullStr ExoMars – WISDOM Field-Test Data Processed with Automatic Pipeline
title_full_unstemmed ExoMars – WISDOM Field-Test Data Processed with Automatic Pipeline
title_sort exomars – wisdom field-test data processed with automatic pipeline
publisher HAL CCSD
publishDate 2023
url https://insu.hal.science/insu-04015250
https://doi.org/10.5194/egusphere-egu23-16376
op_coverage Vienna (Austria), Austria
genre Svalbard
genre_facet Svalbard
op_source EGU General Assembly 2023
https://insu.hal.science/insu-04015250
EGU General Assembly 2023, Sep 2023, Vienna (Austria), Austria. pp.EGU23-16376, ⟨10.5194/egusphere-egu23-16376⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.5194/egusphere-egu23-16376
insu-04015250
https://insu.hal.science/insu-04015250
doi:10.5194/egusphere-egu23-16376
op_doi https://doi.org/10.5194/egusphere-egu23-16376
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