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New Saharan wind observations reveal substantial biases in analysed dust‐generating winds
The Sahara is the largest source of airborne mineral dust on Earth. New data from the Fennec field campaign from remote Sahara allow evaluation of ECMWF ERA‐Interim analysed winds. High winds and diurnal variation are under‐represented in analyses, which perform less well during the summer monsoon (...
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Published in: | Atmospheric science letters 2017-09, Vol.18 (9), p.366-372 |
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description | The Sahara is the largest source of airborne mineral dust on Earth. New data from the Fennec field campaign from remote Sahara allow evaluation of ECMWF ERA‐Interim analysed winds. High winds and diurnal variation are under‐represented in analyses, which perform less well during the summer monsoon (even in the isolated central Sahara). Analyses do not capture the seasonal cycle, missing the summertime maximum in winds in the central Sahara summer time dust hotspot.
For the remote Sahara, the Earth's largest dust source, there has always been a near‐absence of data for evaluating models. Here, new observations from the Fennec project are used along with Sahelian data from the African Monsoon Multidisciplinary Analysis (AMMA) to give an unprecedented evaluation of dust‐generating winds in the European Centre for Medium‐Range Weather Forecasts ERA‐Interim reanalysis (ERA‐I). Consistent with past studies, near‐surface, high‐speed winds are lacking in ERA‐I and the diurnal variability is under‐represented. During the summer monsoon season, correlations of ERA‐I with observed wind‐speed are low (∼0.35 in Sahel and 0.25–0.4 in the Sahara). Fennec data show for the first time that: (1) correlations are reduced even in the Sahara, not directly influenced by the monsoon, (2) the systematic underestimation of observed winds by ERA‐I in the summertime Sahel extends into the central Sahara: potentially explaining the failure of global models to capture the observed global dust maximum that occurs over the summertime Sahara (such as CMIP5), and demonstrates that modelled winds must be improved if they are to capture this key feature of the climatology. |
doi_str_mv | 10.1002/asl.765 |
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For the remote Sahara, the Earth's largest dust source, there has always been a near‐absence of data for evaluating models. Here, new observations from the Fennec project are used along with Sahelian data from the African Monsoon Multidisciplinary Analysis (AMMA) to give an unprecedented evaluation of dust‐generating winds in the European Centre for Medium‐Range Weather Forecasts ERA‐Interim reanalysis (ERA‐I). Consistent with past studies, near‐surface, high‐speed winds are lacking in ERA‐I and the diurnal variability is under‐represented. During the summer monsoon season, correlations of ERA‐I with observed wind‐speed are low (∼0.35 in Sahel and 0.25–0.4 in the Sahara). Fennec data show for the first time that: (1) correlations are reduced even in the Sahara, not directly influenced by the monsoon, (2) the systematic underestimation of observed winds by ERA‐I in the summertime Sahel extends into the central Sahara: potentially explaining the failure of global models to capture the observed global dust maximum that occurs over the summertime Sahara (such as CMIP5), and demonstrates that modelled winds must be improved if they are to capture this key feature of the climatology.</description><identifier>ISSN: 1530-261X</identifier><identifier>EISSN: 1530-261X</identifier><identifier>DOI: 10.1002/asl.765</identifier><language>eng</language><publisher>Chichester, UK: John Wiley & Sons, Ltd</publisher><subject>African monsoon ; AMMA ; Atmospheric particulates ; Atmospheric sciences ; Climate models ; Climatology ; Correlation ; Data ; Dust ; Dust storms ; Earth ; Evaluation ; fennec ; monsoon ; Monsoons ; reanalysis ; Sahara ; Summer monsoon ; Weather forecasting ; Wind ; Wind observation ; Wind speed ; Winds</subject><ispartof>Atmospheric science letters, 2017-09, Vol.18 (9), p.366-372</ispartof><rights>2017 The Authors. published by John Wiley & Sons Ltd on behalf of the Royal Meteorological Society.</rights><rights>2017. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c3235-650dc5490594b44f882d81012a77a40e71572e4ae36bfc91f3381d041cf16c183</citedby><cites>FETCH-LOGICAL-c3235-650dc5490594b44f882d81012a77a40e71572e4ae36bfc91f3381d041cf16c183</cites><orcidid>0000-0002-4970-9032</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/1937292073/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/1937292073?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,11562,25753,27924,27925,37012,44590,46052,46476,75126</link.rule.ids></links><search><creatorcontrib>Roberts, Alexander J.</creatorcontrib><creatorcontrib>Marsham, John H.</creatorcontrib><creatorcontrib>Knippertz, Peter</creatorcontrib><creatorcontrib>Parker, Douglas J.</creatorcontrib><creatorcontrib>Bart, Mark</creatorcontrib><creatorcontrib>Garcia‐Carreras, Luis</creatorcontrib><creatorcontrib>Hobby, Matthew</creatorcontrib><creatorcontrib>McQuaid, James B.</creatorcontrib><creatorcontrib>Rosenberg, Philip D.</creatorcontrib><creatorcontrib>Walker, Daniel</creatorcontrib><title>New Saharan wind observations reveal substantial biases in analysed dust‐generating winds</title><title>Atmospheric science letters</title><description>The Sahara is the largest source of airborne mineral dust on Earth. New data from the Fennec field campaign from remote Sahara allow evaluation of ECMWF ERA‐Interim analysed winds. High winds and diurnal variation are under‐represented in analyses, which perform less well during the summer monsoon (even in the isolated central Sahara). Analyses do not capture the seasonal cycle, missing the summertime maximum in winds in the central Sahara summer time dust hotspot.
For the remote Sahara, the Earth's largest dust source, there has always been a near‐absence of data for evaluating models. Here, new observations from the Fennec project are used along with Sahelian data from the African Monsoon Multidisciplinary Analysis (AMMA) to give an unprecedented evaluation of dust‐generating winds in the European Centre for Medium‐Range Weather Forecasts ERA‐Interim reanalysis (ERA‐I). Consistent with past studies, near‐surface, high‐speed winds are lacking in ERA‐I and the diurnal variability is under‐represented. During the summer monsoon season, correlations of ERA‐I with observed wind‐speed are low (∼0.35 in Sahel and 0.25–0.4 in the Sahara). Fennec data show for the first time that: (1) correlations are reduced even in the Sahara, not directly influenced by the monsoon, (2) the systematic underestimation of observed winds by ERA‐I in the summertime Sahel extends into the central Sahara: potentially explaining the failure of global models to capture the observed global dust maximum that occurs over the summertime Sahara (such as CMIP5), and demonstrates that modelled winds must be improved if they are to capture this key feature of the climatology.</description><subject>African monsoon</subject><subject>AMMA</subject><subject>Atmospheric particulates</subject><subject>Atmospheric sciences</subject><subject>Climate models</subject><subject>Climatology</subject><subject>Correlation</subject><subject>Data</subject><subject>Dust</subject><subject>Dust storms</subject><subject>Earth</subject><subject>Evaluation</subject><subject>fennec</subject><subject>monsoon</subject><subject>Monsoons</subject><subject>reanalysis</subject><subject>Sahara</subject><subject>Summer monsoon</subject><subject>Weather forecasting</subject><subject>Wind</subject><subject>Wind observation</subject><subject>Wind speed</subject><subject>Winds</subject><issn>1530-261X</issn><issn>1530-261X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>24P</sourceid><sourceid>PIMPY</sourceid><recordid>eNp1kM1Kw0AUhQdRsFbxFQZcuDF17vxkkmUp_kHRRRUEF8MkmdSUOKlzk5bufASf0ScxtS7cuLpn8Z3D5SPkFNgIGOOXFuuRjtUeGYASLOIxPO__yYfkCHHBGICM9YC83Ls1ndlXG6yn68oXtMnQhZVtq8YjDW7lbE2xy7C1vq36nFUWHdLKU-ttvUFX0KLD9uvjc-68C33Rz3-W8JgclLZGd_J7h-Tp-upxchtNH27uJuNplAsuVBQrVuRKpkylMpOyTBJeJMCAW62tZE6D0txJ60SclXkKpRAJFExCXkKcQyKG5Gy3uwzNe-ewNYumC_1zaCAVmqecadFT5zsqDw1icKVZhurNho0BZrbmTG_O9OZ68mJHrqvabf7DzHg25Vv8G3bRb_8</recordid><startdate>201709</startdate><enddate>201709</enddate><creator>Roberts, Alexander J.</creator><creator>Marsham, John H.</creator><creator>Knippertz, Peter</creator><creator>Parker, Douglas J.</creator><creator>Bart, Mark</creator><creator>Garcia‐Carreras, Luis</creator><creator>Hobby, Matthew</creator><creator>McQuaid, James B.</creator><creator>Rosenberg, Philip D.</creator><creator>Walker, Daniel</creator><general>John Wiley & Sons, Ltd</general><general>John Wiley & Sons, Inc</general><scope>24P</scope><scope>WIN</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7QH</scope><scope>7TG</scope><scope>7TN</scope><scope>7UA</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>H96</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L.G</scope><scope>PCBAR</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><orcidid>https://orcid.org/0000-0002-4970-9032</orcidid></search><sort><creationdate>201709</creationdate><title>New Saharan wind observations reveal substantial biases in analysed dust‐generating winds</title><author>Roberts, Alexander J. ; 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New data from the Fennec field campaign from remote Sahara allow evaluation of ECMWF ERA‐Interim analysed winds. High winds and diurnal variation are under‐represented in analyses, which perform less well during the summer monsoon (even in the isolated central Sahara). Analyses do not capture the seasonal cycle, missing the summertime maximum in winds in the central Sahara summer time dust hotspot.
For the remote Sahara, the Earth's largest dust source, there has always been a near‐absence of data for evaluating models. Here, new observations from the Fennec project are used along with Sahelian data from the African Monsoon Multidisciplinary Analysis (AMMA) to give an unprecedented evaluation of dust‐generating winds in the European Centre for Medium‐Range Weather Forecasts ERA‐Interim reanalysis (ERA‐I). Consistent with past studies, near‐surface, high‐speed winds are lacking in ERA‐I and the diurnal variability is under‐represented. During the summer monsoon season, correlations of ERA‐I with observed wind‐speed are low (∼0.35 in Sahel and 0.25–0.4 in the Sahara). Fennec data show for the first time that: (1) correlations are reduced even in the Sahara, not directly influenced by the monsoon, (2) the systematic underestimation of observed winds by ERA‐I in the summertime Sahel extends into the central Sahara: potentially explaining the failure of global models to capture the observed global dust maximum that occurs over the summertime Sahara (such as CMIP5), and demonstrates that modelled winds must be improved if they are to capture this key feature of the climatology.</abstract><cop>Chichester, UK</cop><pub>John Wiley & Sons, Ltd</pub><doi>10.1002/asl.765</doi><tpages>7</tpages><orcidid>https://orcid.org/0000-0002-4970-9032</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | African monsoon AMMA Atmospheric particulates Atmospheric sciences Climate models Climatology Correlation Data Dust Dust storms Earth Evaluation fennec monsoon Monsoons reanalysis Sahara Summer monsoon Weather forecasting Wind Wind observation Wind speed Winds |
title | New Saharan wind observations reveal substantial biases in analysed dust‐generating winds |
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