Technical Note: On the use of the mushy-layer Rayleigh number for the interpretation of sea-ice-core data
International audience We examine some practical aspects of using a mushy-layer Rayleigh number for the interpretation of sea-ice-core data. In principle, such analysis should allow one to determine convectively active regions within the ice core by identifying those regions in which the mush-Raylei...
Main Authors: | , , , , , , , , , , |
---|---|
Other Authors: | , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
HAL CCSD
2013
|
Subjects: | |
Online Access: | https://hal.science/hal-00912614 https://hal.science/hal-00912614/document https://hal.science/hal-00912614/file/tcd-7-3209-2013.pdf https://doi.org/10.5194/TCD-7-3209-2013 |
id |
ftmuseumnhn:oai:HAL:hal-00912614v1 |
---|---|
record_format |
openpolar |
institution |
Open Polar |
collection |
Muséum National d'Histoire Naturelle (MNHM): HAL |
op_collection_id |
ftmuseumnhn |
language |
English |
topic |
[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph] [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] |
spellingShingle |
[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph] [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] Vancoppenolle, Martin Notz, Dirk Vivier, Frédéric Tison, Jean-Louis Delille, Bruno Carnat, Gauthier Zhou, J. Jardon, Fernanda Griewank, P. Lourenço, Antonio Haskell, T. Technical Note: On the use of the mushy-layer Rayleigh number for the interpretation of sea-ice-core data |
topic_facet |
[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph] [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] |
description |
International audience We examine some practical aspects of using a mushy-layer Rayleigh number for the interpretation of sea-ice-core data. In principle, such analysis should allow one to determine convectively active regions within the ice core by identifying those regions in which the mush-Rayleigh number is super-critical. In practice, however, a quantitative analysis is complicated by uncertainties regarding the specific formulation of both the mush-Rayleigh number itself and of the sea-ice permeability that is crucial for quantifying the Rayleigh number. Additionally, brine loss from highly permeable sections of the ice core, in particular close to the ice-ocean interface, and typically weekly ice core sampling, limit the practical applicability of the Rayleigh number for ice-core interpretation. We here quantify these uncertainties, suggest a standard method for the computation of the Rayleigh number for sea ice and discuss possibilities and limitations of ice-core interpretation based on the Rayleigh number. |
author2 |
Laboratoire d'Océanographie et du Climat : Expérimentations et Approches Numériques (LOCEAN) Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)) École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) Max Planck Institute for Meteorology (MPI-M) Max-Planck-Gesellschaft Université libre de Bruxelles (ULB) Université de Liège Développement Instrumental et Techniques Marines (DITM) Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) Callaghan Innovation ANR-09-BLAN-0227,OPTIMISM(2009) European Project: 321938,EC:FP7:PEOPLE,FP7-PEOPLE-2012-CIG,BISICLO(2012) |
format |
Article in Journal/Newspaper |
author |
Vancoppenolle, Martin Notz, Dirk Vivier, Frédéric Tison, Jean-Louis Delille, Bruno Carnat, Gauthier Zhou, J. Jardon, Fernanda Griewank, P. Lourenço, Antonio Haskell, T. |
author_facet |
Vancoppenolle, Martin Notz, Dirk Vivier, Frédéric Tison, Jean-Louis Delille, Bruno Carnat, Gauthier Zhou, J. Jardon, Fernanda Griewank, P. Lourenço, Antonio Haskell, T. |
author_sort |
Vancoppenolle, Martin |
title |
Technical Note: On the use of the mushy-layer Rayleigh number for the interpretation of sea-ice-core data |
title_short |
Technical Note: On the use of the mushy-layer Rayleigh number for the interpretation of sea-ice-core data |
title_full |
Technical Note: On the use of the mushy-layer Rayleigh number for the interpretation of sea-ice-core data |
title_fullStr |
Technical Note: On the use of the mushy-layer Rayleigh number for the interpretation of sea-ice-core data |
title_full_unstemmed |
Technical Note: On the use of the mushy-layer Rayleigh number for the interpretation of sea-ice-core data |
title_sort |
technical note: on the use of the mushy-layer rayleigh number for the interpretation of sea-ice-core data |
publisher |
HAL CCSD |
publishDate |
2013 |
url |
https://hal.science/hal-00912614 https://hal.science/hal-00912614/document https://hal.science/hal-00912614/file/tcd-7-3209-2013.pdf https://doi.org/10.5194/TCD-7-3209-2013 |
genre |
ice core Sea ice The Cryosphere The Cryosphere Discussions |
genre_facet |
ice core Sea ice The Cryosphere The Cryosphere Discussions |
op_source |
ISSN: 1994-0432 EISSN: 1994-0440 The Cryosphere Discussions https://hal.science/hal-00912614 The Cryosphere Discussions, 2013, 7, pp.3209-3230. ⟨10.5194/TCD-7-3209-2013⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.5194/TCD-7-3209-2013 info:eu-repo/grantAgreement/EC/FP7/321938/EU/BIogeochemical cycles, Sea Ice and CLimate in the Polar Oceans/BISICLO hal-00912614 https://hal.science/hal-00912614 https://hal.science/hal-00912614/document https://hal.science/hal-00912614/file/tcd-7-3209-2013.pdf BIBCODE: 2013TCD.7.3209V doi:10.5194/TCD-7-3209-2013 |
op_rights |
http://creativecommons.org/licenses/by/ info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.5194/TCD-7-3209-2013 |
_version_ |
1799481577598615552 |
spelling |
ftmuseumnhn:oai:HAL:hal-00912614v1 2024-05-19T07:41:58+00:00 Technical Note: On the use of the mushy-layer Rayleigh number for the interpretation of sea-ice-core data Vancoppenolle, Martin Notz, Dirk Vivier, Frédéric Tison, Jean-Louis Delille, Bruno Carnat, Gauthier Zhou, J. Jardon, Fernanda Griewank, P. Lourenço, Antonio Haskell, T. Laboratoire d'Océanographie et du Climat : Expérimentations et Approches Numériques (LOCEAN) Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)) École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) Max Planck Institute for Meteorology (MPI-M) Max-Planck-Gesellschaft Université libre de Bruxelles (ULB) Université de Liège Développement Instrumental et Techniques Marines (DITM) Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) Callaghan Innovation ANR-09-BLAN-0227,OPTIMISM(2009) European Project: 321938,EC:FP7:PEOPLE,FP7-PEOPLE-2012-CIG,BISICLO(2012) 2013 https://hal.science/hal-00912614 https://hal.science/hal-00912614/document https://hal.science/hal-00912614/file/tcd-7-3209-2013.pdf https://doi.org/10.5194/TCD-7-3209-2013 en eng HAL CCSD Copernicus info:eu-repo/semantics/altIdentifier/doi/10.5194/TCD-7-3209-2013 info:eu-repo/grantAgreement/EC/FP7/321938/EU/BIogeochemical cycles, Sea Ice and CLimate in the Polar Oceans/BISICLO hal-00912614 https://hal.science/hal-00912614 https://hal.science/hal-00912614/document https://hal.science/hal-00912614/file/tcd-7-3209-2013.pdf BIBCODE: 2013TCD.7.3209V doi:10.5194/TCD-7-3209-2013 http://creativecommons.org/licenses/by/ info:eu-repo/semantics/OpenAccess ISSN: 1994-0432 EISSN: 1994-0440 The Cryosphere Discussions https://hal.science/hal-00912614 The Cryosphere Discussions, 2013, 7, pp.3209-3230. ⟨10.5194/TCD-7-3209-2013⟩ [PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph] [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] info:eu-repo/semantics/article Journal articles 2013 ftmuseumnhn https://doi.org/10.5194/TCD-7-3209-2013 2024-04-25T00:43:04Z International audience We examine some practical aspects of using a mushy-layer Rayleigh number for the interpretation of sea-ice-core data. In principle, such analysis should allow one to determine convectively active regions within the ice core by identifying those regions in which the mush-Rayleigh number is super-critical. In practice, however, a quantitative analysis is complicated by uncertainties regarding the specific formulation of both the mush-Rayleigh number itself and of the sea-ice permeability that is crucial for quantifying the Rayleigh number. Additionally, brine loss from highly permeable sections of the ice core, in particular close to the ice-ocean interface, and typically weekly ice core sampling, limit the practical applicability of the Rayleigh number for ice-core interpretation. We here quantify these uncertainties, suggest a standard method for the computation of the Rayleigh number for sea ice and discuss possibilities and limitations of ice-core interpretation based on the Rayleigh number. Article in Journal/Newspaper ice core Sea ice The Cryosphere The Cryosphere Discussions Muséum National d'Histoire Naturelle (MNHM): HAL |