Anisotropic MagnetoResistance (AMR) Instrument to Study the Martian Magnetic Environment from the Surface: Expected Scientific Return

The ExoMars programme has the objective to answer to the question of whether life ever existed on Mars. The second mission comprising the Rosalind Franklin rover and Kazachok Surface Platform was designed to focus specifically on the characterization of the environmental parameters which can play an...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Solar system research 2023-08, Vol.57 (4), p.307-323
Hauptverfasser: Díaz Michelena, Marina, Rivero, Miguel Ángel, Romero, Sergio Fernández, Adeli, Solmaz, Oliveira, Joana S., Henrich, Clara, Aspás, Alberto, Parrondo, María
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 323
container_issue 4
container_start_page 307
container_title Solar system research
container_volume 57
creator Díaz Michelena, Marina
Rivero, Miguel Ángel
Romero, Sergio Fernández
Adeli, Solmaz
Oliveira, Joana S.
Henrich, Clara
Aspás, Alberto
Parrondo, María
description The ExoMars programme has the objective to answer to the question of whether life ever existed on Mars. The second mission comprising the Rosalind Franklin rover and Kazachok Surface Platform was designed to focus specifically on the characterization of the environmental parameters which can play an important role for the existence of life on the surface of the planet. One of these parameters is the magnetic field because of its ability of shielding the solar and cosmic radiation. For such characterization, the scientific suite of the Surface Platform counts with two instruments: the Anisotropic MagnetoResistance (AMR) and the MArtIan Ground ElectromagneTic (MAIGRET) instruments. The AMR goal is to characterize both the surface and subsurface and the time-varying magnetic fields, related to the crustal and the external fields respectively, at the ExoMars landing site in Oxia Planum. The operation to achieve these goals includes two phases, the first phase corresponding to the lander descent and the second phase in which the instrument is deployed on the surface. In this work, we simulate the first operations phase using synthetic magnetic field models, assuming that the different crustal units at the landing site might be magnetized. We also perform measurements in our laboratory to simulate the second phase operation of the instrument on the Martian surface. We discuss the capability of interpretation of the instrument, based on the available information of the landing site and the results from our models.
doi_str_mv 10.1134/S003809462304010X
format Article
fullrecord <record><control><sourceid>crossref_sprin</sourceid><recordid>TN_cdi_crossref_primary_10_1134_S003809462304010X</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>10_1134_S003809462304010X</sourcerecordid><originalsourceid>FETCH-LOGICAL-c288t-24b47cfc668cc4e4834fc38fd99986c6d9ea749bd5c426acee81d4789fc870293</originalsourceid><addsrcrecordid>eNp9kM1KAzEURoMoWKsP4C5LXYwmk5hJ3BWpWmgRWgV3w_ROUlNsUpKM2AfwvU1_doKru_jOuffjInRJyQ2ljN_OCGGSKC5KRjih5P0I9aggsmC8ZMeot42LbX6KzmJckoyQSvTQz8DZ6FPwawt40iycTn6qo42pcaDx1WAyvcYjF1PoVtolnDyepa7d4PShMx-SbdzBywuG7ssG73akCX61o2ZdMA3oezz8XmtIusUzsJmwJhtTnbrgztGJaT6jvjjMPnp7HL4-PBfjl6fRw2BcQCllKko-5xUYEEICcM0l4waYNK1SSgoQrdJNxdW8vQNeinxTS9rySioDsiKlYn1E93sh-BiDNvU62FUTNjUl9faP9Z8_ZqfcOzGzbqFDvfS5cq75j_QLf6h3Yg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Anisotropic MagnetoResistance (AMR) Instrument to Study the Martian Magnetic Environment from the Surface: Expected Scientific Return</title><source>SpringerLink Journals - AutoHoldings</source><creator>Díaz Michelena, Marina ; Rivero, Miguel Ángel ; Romero, Sergio Fernández ; Adeli, Solmaz ; Oliveira, Joana S. ; Henrich, Clara ; Aspás, Alberto ; Parrondo, María</creator><creatorcontrib>Díaz Michelena, Marina ; Rivero, Miguel Ángel ; Romero, Sergio Fernández ; Adeli, Solmaz ; Oliveira, Joana S. ; Henrich, Clara ; Aspás, Alberto ; Parrondo, María</creatorcontrib><description>The ExoMars programme has the objective to answer to the question of whether life ever existed on Mars. The second mission comprising the Rosalind Franklin rover and Kazachok Surface Platform was designed to focus specifically on the characterization of the environmental parameters which can play an important role for the existence of life on the surface of the planet. One of these parameters is the magnetic field because of its ability of shielding the solar and cosmic radiation. For such characterization, the scientific suite of the Surface Platform counts with two instruments: the Anisotropic MagnetoResistance (AMR) and the MArtIan Ground ElectromagneTic (MAIGRET) instruments. The AMR goal is to characterize both the surface and subsurface and the time-varying magnetic fields, related to the crustal and the external fields respectively, at the ExoMars landing site in Oxia Planum. The operation to achieve these goals includes two phases, the first phase corresponding to the lander descent and the second phase in which the instrument is deployed on the surface. In this work, we simulate the first operations phase using synthetic magnetic field models, assuming that the different crustal units at the landing site might be magnetized. We also perform measurements in our laboratory to simulate the second phase operation of the instrument on the Martian surface. We discuss the capability of interpretation of the instrument, based on the available information of the landing site and the results from our models.</description><identifier>ISSN: 0038-0946</identifier><identifier>EISSN: 1608-3423</identifier><identifier>DOI: 10.1134/S003809462304010X</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Astronomy ; Astrophysics and Astroparticles ; Astrophysics and Cosmology ; Observations and Techniques ; Physics ; Physics and Astronomy ; Planetology</subject><ispartof>Solar system research, 2023-08, Vol.57 (4), p.307-323</ispartof><rights>Pleiades Publishing, Inc. 2023. ISSN 0038-0946, Solar System Research, 2023, Vol. 57, No. 4, pp. 307–323. © Pleiades Publishing, Inc., 2023.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c288t-24b47cfc668cc4e4834fc38fd99986c6d9ea749bd5c426acee81d4789fc870293</citedby><cites>FETCH-LOGICAL-c288t-24b47cfc668cc4e4834fc38fd99986c6d9ea749bd5c426acee81d4789fc870293</cites><orcidid>0000-0002-3414-7727</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S003809462304010X$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S003809462304010X$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Díaz Michelena, Marina</creatorcontrib><creatorcontrib>Rivero, Miguel Ángel</creatorcontrib><creatorcontrib>Romero, Sergio Fernández</creatorcontrib><creatorcontrib>Adeli, Solmaz</creatorcontrib><creatorcontrib>Oliveira, Joana S.</creatorcontrib><creatorcontrib>Henrich, Clara</creatorcontrib><creatorcontrib>Aspás, Alberto</creatorcontrib><creatorcontrib>Parrondo, María</creatorcontrib><title>Anisotropic MagnetoResistance (AMR) Instrument to Study the Martian Magnetic Environment from the Surface: Expected Scientific Return</title><title>Solar system research</title><addtitle>Sol Syst Res</addtitle><description>The ExoMars programme has the objective to answer to the question of whether life ever existed on Mars. The second mission comprising the Rosalind Franklin rover and Kazachok Surface Platform was designed to focus specifically on the characterization of the environmental parameters which can play an important role for the existence of life on the surface of the planet. One of these parameters is the magnetic field because of its ability of shielding the solar and cosmic radiation. For such characterization, the scientific suite of the Surface Platform counts with two instruments: the Anisotropic MagnetoResistance (AMR) and the MArtIan Ground ElectromagneTic (MAIGRET) instruments. The AMR goal is to characterize both the surface and subsurface and the time-varying magnetic fields, related to the crustal and the external fields respectively, at the ExoMars landing site in Oxia Planum. The operation to achieve these goals includes two phases, the first phase corresponding to the lander descent and the second phase in which the instrument is deployed on the surface. In this work, we simulate the first operations phase using synthetic magnetic field models, assuming that the different crustal units at the landing site might be magnetized. We also perform measurements in our laboratory to simulate the second phase operation of the instrument on the Martian surface. We discuss the capability of interpretation of the instrument, based on the available information of the landing site and the results from our models.</description><subject>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>Astrophysics and Cosmology</subject><subject>Observations and Techniques</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetology</subject><issn>0038-0946</issn><issn>1608-3423</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><recordid>eNp9kM1KAzEURoMoWKsP4C5LXYwmk5hJ3BWpWmgRWgV3w_ROUlNsUpKM2AfwvU1_doKru_jOuffjInRJyQ2ljN_OCGGSKC5KRjih5P0I9aggsmC8ZMeot42LbX6KzmJckoyQSvTQz8DZ6FPwawt40iycTn6qo42pcaDx1WAyvcYjF1PoVtolnDyepa7d4PShMx-SbdzBywuG7ssG73akCX61o2ZdMA3oezz8XmtIusUzsJmwJhtTnbrgztGJaT6jvjjMPnp7HL4-PBfjl6fRw2BcQCllKko-5xUYEEICcM0l4waYNK1SSgoQrdJNxdW8vQNeinxTS9rySioDsiKlYn1E93sh-BiDNvU62FUTNjUl9faP9Z8_ZqfcOzGzbqFDvfS5cq75j_QLf6h3Yg</recordid><startdate>20230801</startdate><enddate>20230801</enddate><creator>Díaz Michelena, Marina</creator><creator>Rivero, Miguel Ángel</creator><creator>Romero, Sergio Fernández</creator><creator>Adeli, Solmaz</creator><creator>Oliveira, Joana S.</creator><creator>Henrich, Clara</creator><creator>Aspás, Alberto</creator><creator>Parrondo, María</creator><general>Pleiades Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-3414-7727</orcidid></search><sort><creationdate>20230801</creationdate><title>Anisotropic MagnetoResistance (AMR) Instrument to Study the Martian Magnetic Environment from the Surface: Expected Scientific Return</title><author>Díaz Michelena, Marina ; Rivero, Miguel Ángel ; Romero, Sergio Fernández ; Adeli, Solmaz ; Oliveira, Joana S. ; Henrich, Clara ; Aspás, Alberto ; Parrondo, María</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c288t-24b47cfc668cc4e4834fc38fd99986c6d9ea749bd5c426acee81d4789fc870293</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Astrophysics and Cosmology</topic><topic>Observations and Techniques</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Planetology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Díaz Michelena, Marina</creatorcontrib><creatorcontrib>Rivero, Miguel Ángel</creatorcontrib><creatorcontrib>Romero, Sergio Fernández</creatorcontrib><creatorcontrib>Adeli, Solmaz</creatorcontrib><creatorcontrib>Oliveira, Joana S.</creatorcontrib><creatorcontrib>Henrich, Clara</creatorcontrib><creatorcontrib>Aspás, Alberto</creatorcontrib><creatorcontrib>Parrondo, María</creatorcontrib><collection>CrossRef</collection><jtitle>Solar system research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Díaz Michelena, Marina</au><au>Rivero, Miguel Ángel</au><au>Romero, Sergio Fernández</au><au>Adeli, Solmaz</au><au>Oliveira, Joana S.</au><au>Henrich, Clara</au><au>Aspás, Alberto</au><au>Parrondo, María</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Anisotropic MagnetoResistance (AMR) Instrument to Study the Martian Magnetic Environment from the Surface: Expected Scientific Return</atitle><jtitle>Solar system research</jtitle><stitle>Sol Syst Res</stitle><date>2023-08-01</date><risdate>2023</risdate><volume>57</volume><issue>4</issue><spage>307</spage><epage>323</epage><pages>307-323</pages><issn>0038-0946</issn><eissn>1608-3423</eissn><abstract>The ExoMars programme has the objective to answer to the question of whether life ever existed on Mars. The second mission comprising the Rosalind Franklin rover and Kazachok Surface Platform was designed to focus specifically on the characterization of the environmental parameters which can play an important role for the existence of life on the surface of the planet. One of these parameters is the magnetic field because of its ability of shielding the solar and cosmic radiation. For such characterization, the scientific suite of the Surface Platform counts with two instruments: the Anisotropic MagnetoResistance (AMR) and the MArtIan Ground ElectromagneTic (MAIGRET) instruments. The AMR goal is to characterize both the surface and subsurface and the time-varying magnetic fields, related to the crustal and the external fields respectively, at the ExoMars landing site in Oxia Planum. The operation to achieve these goals includes two phases, the first phase corresponding to the lander descent and the second phase in which the instrument is deployed on the surface. In this work, we simulate the first operations phase using synthetic magnetic field models, assuming that the different crustal units at the landing site might be magnetized. We also perform measurements in our laboratory to simulate the second phase operation of the instrument on the Martian surface. We discuss the capability of interpretation of the instrument, based on the available information of the landing site and the results from our models.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S003809462304010X</doi><tpages>17</tpages><orcidid>https://orcid.org/0000-0002-3414-7727</orcidid></addata></record>
fulltext fulltext
identifier ISSN: 0038-0946
ispartof Solar system research, 2023-08, Vol.57 (4), p.307-323
issn 0038-0946
1608-3423
language eng
recordid cdi_crossref_primary_10_1134_S003809462304010X
source SpringerLink Journals - AutoHoldings
subjects Astronomy
Astrophysics and Astroparticles
Astrophysics and Cosmology
Observations and Techniques
Physics
Physics and Astronomy
Planetology
title Anisotropic MagnetoResistance (AMR) Instrument to Study the Martian Magnetic Environment from the Surface: Expected Scientific Return
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-04T22%3A45%3A55IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-crossref_sprin&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Anisotropic%20MagnetoResistance%20(AMR)%20Instrument%20to%20Study%20the%20Martian%20Magnetic%20Environment%20from%20the%20Surface:%20Expected%20Scientific%20Return&rft.jtitle=Solar%20system%20research&rft.au=D%C3%ADaz%20Michelena,%20Marina&rft.date=2023-08-01&rft.volume=57&rft.issue=4&rft.spage=307&rft.epage=323&rft.pages=307-323&rft.issn=0038-0946&rft.eissn=1608-3423&rft_id=info:doi/10.1134/S003809462304010X&rft_dat=%3Ccrossref_sprin%3E10_1134_S003809462304010X%3C/crossref_sprin%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true