Candidate models for the 1995 revision of IGRF, a worldwide evaluation based on observatory monthly means
Identifieur interne : 00D069 ( Main/Exploration ); précédent : 00D068; suivant : 00D070Candidate models for the 1995 revision of IGRF, a worldwide evaluation based on observatory monthly means
Auteurs : Y. Cohen [France] ; M. Alexandrescu [France] ; G. Hulot [France] ; J. L. Le Mouël [France]Source :
- Journal of geomagnetism and geoelectricity [ 0022-1392 ] ; 1997.
Descripteurs français
- Pascal (Inist)
- Wicri :
- geographic : Russie.
English descriptors
- KwdEn :
Abstract
Three candidate models for the IGRF 1995 description of the 1995.0 main field are evaluated. These are GS-95 proposed by the Goddard Space Flight Center (U.S.A.), IZ-95 proposed by IZMIRAN (Russia) and UB-95 proposed jointly by the US Navy (U.S.A.) and the British Geological Survey (U.K.). These models are tested against a set of December 1994 and January 1995 preliminary monthly mean values kindly provided to us by 73 observatories distributed throughout the world. This procedure has at least two advantages. First, no secular variation corrections are required for the test to be carried out. Second, all datasets used in the construction of the candidate models include observatory annual means up to at most 1993.5 and share similar links to our independent test data set. We, therefore, expect the test to be reasonably unbiased towards any ofthe models. The procedure has the inconvenience ofbeing sensitive to local crustal anomalies, as pointed out by Langel et al. (1982). Indeed, directly comparing predictions from the candidate models to the observed monthly means reveals little else than a common, correlated, hardly discriminating, disagreement mainly due to crustal anomalies. We repeated the comparison after correcting the monthly means for the crustal anomalies derived by Bloxham and Jackson (1992). This second test was much more significant and showed that the models do a comparable job, UB-95 being marginally better. We recommand equal weighing between the two GS-95 and IZ-95 candidate models, and a slightly larger weight for UB-95.
Affiliations:
Links toward previous steps (curation, corpus...)
- to stream PascalFrancis, to step Corpus: 006959
- to stream PascalFrancis, to step Curation: 006710
- to stream PascalFrancis, to step Checkpoint: 006784
- to stream Main, to step Merge: 00E220
- to stream Main, to step Curation: 00D069
Le document en format XML
<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">Candidate models for the 1995 revision of IGRF, a worldwide evaluation based on observatory monthly means</title><author><name sortKey="Cohen, Y" sort="Cohen, Y" uniqKey="Cohen Y" first="Y." last="Cohen">Y. Cohen</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Laboratoire de Géomagnétisme, URA 729 CNRS, Institut de Physique du Globe de Paris, 4 Place Jussieu</s1><s2>75252 Paris</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Paris</settlement></placeName></affiliation></author><author><name sortKey="Alexandrescu, M" sort="Alexandrescu, M" uniqKey="Alexandrescu M" first="M." last="Alexandrescu">M. Alexandrescu</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Laboratoire de Géomagnétisme, URA 729 CNRS, Institut de Physique du Globe de Paris, 4 Place Jussieu</s1><s2>75252 Paris</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Paris</settlement></placeName></affiliation></author><author><name sortKey="Hulot, G" sort="Hulot, G" uniqKey="Hulot G" first="G." last="Hulot">G. Hulot</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Laboratoire de Géomagnétisme, URA 729 CNRS, Institut de Physique du Globe de Paris, 4 Place Jussieu</s1><s2>75252 Paris</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Paris</settlement></placeName></affiliation></author><author><name sortKey="Le Mouel, J L" sort="Le Mouel, J L" uniqKey="Le Mouel J" first="J. L." last="Le Mouël">J. L. Le Mouël</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Laboratoire de Géomagnétisme, URA 729 CNRS, Institut de Physique du Globe de Paris, 4 Place Jussieu</s1><s2>75252 Paris</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Paris</settlement></placeName></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">INIST</idno><idno type="inist">97-0406882</idno><date when="1997">1997</date><idno type="stanalyst">PASCAL 97-0406882 INIST</idno><idno type="RBID">Pascal:97-0406882</idno><idno type="wicri:Area/PascalFrancis/Corpus">006959</idno><idno type="wicri:Area/PascalFrancis/Curation">006710</idno><idno type="wicri:Area/PascalFrancis/Checkpoint">006784</idno><idno type="wicri:explorRef" wicri:stream="PascalFrancis" wicri:step="Checkpoint">006784</idno><idno type="wicri:doubleKey">0022-1392:1997:Cohen Y:candidate:models:for</idno><idno type="wicri:Area/Main/Merge">00E220</idno><idno type="wicri:Area/Main/Curation">00D069</idno><idno type="wicri:Area/Main/Exploration">00D069</idno></publicationStmt><sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Candidate models for the 1995 revision of IGRF, a worldwide evaluation based on observatory monthly means</title><author><name sortKey="Cohen, Y" sort="Cohen, Y" uniqKey="Cohen Y" first="Y." last="Cohen">Y. Cohen</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Laboratoire de Géomagnétisme, URA 729 CNRS, Institut de Physique du Globe de Paris, 4 Place Jussieu</s1><s2>75252 Paris</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Paris</settlement></placeName></affiliation></author><author><name sortKey="Alexandrescu, M" sort="Alexandrescu, M" uniqKey="Alexandrescu M" first="M." last="Alexandrescu">M. Alexandrescu</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Laboratoire de Géomagnétisme, URA 729 CNRS, Institut de Physique du Globe de Paris, 4 Place Jussieu</s1><s2>75252 Paris</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Paris</settlement></placeName></affiliation></author><author><name sortKey="Hulot, G" sort="Hulot, G" uniqKey="Hulot G" first="G." last="Hulot">G. Hulot</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Laboratoire de Géomagnétisme, URA 729 CNRS, Institut de Physique du Globe de Paris, 4 Place Jussieu</s1><s2>75252 Paris</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Paris</settlement></placeName></affiliation></author><author><name sortKey="Le Mouel, J L" sort="Le Mouel, J L" uniqKey="Le Mouel J" first="J. L." last="Le Mouël">J. L. Le Mouël</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Laboratoire de Géomagnétisme, URA 729 CNRS, Institut de Physique du Globe de Paris, 4 Place Jussieu</s1><s2>75252 Paris</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Paris</settlement></placeName></affiliation></author></analytic><series><title level="j" type="main">Journal of geomagnetism and geoelectricity</title><title level="j" type="abbreviated">J. geomagn. geoelectr.</title><idno type="ISSN">0022-1392</idno><imprint><date when="1997">1997</date></imprint></series></biblStruct></sourceDesc><seriesStmt><title level="j" type="main">Journal of geomagnetism and geoelectricity</title><title level="j" type="abbreviated">J. geomagn. geoelectr.</title><idno type="ISSN">0022-1392</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Earth</term><term>Russian Federation</term><term>United Kingdom</term><term>United States</term><term>anomalies</term><term>corrections</term><term>geomagnetic field</term><term>models</term><term>observatories</term><term>revision</term><term>secular variations</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Planète Terre</term><term>Etats Unis</term><term>Russie</term><term>Royaume Uni</term><term>Révision</term><term>Champ géomagnétique</term><term>Observatoire</term><term>Correction</term><term>Modèle</term><term>Anomalie</term><term>Variation séculaire</term></keywords><keywords scheme="Wicri" type="geographic" xml:lang="fr"><term>Russie</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">Three candidate models for the IGRF 1995 description of the 1995.0 main field are evaluated. These are GS-95 proposed by the Goddard Space Flight Center (U.S.A.), IZ-95 proposed by IZMIRAN (Russia) and UB-95 proposed jointly by the US Navy (U.S.A.) and the British Geological Survey (U.K.). These models are tested against a set of December 1994 and January 1995 preliminary monthly mean values kindly provided to us by 73 observatories distributed throughout the world. This procedure has at least two advantages. First, no secular variation corrections are required for the test to be carried out. Second, all datasets used in the construction of the candidate models include observatory annual means up to at most 1993.5 and share similar links to our independent test data set. We, therefore, expect the test to be reasonably unbiased towards any ofthe models. The procedure has the inconvenience ofbeing sensitive to local crustal anomalies, as pointed out by Langel et al. (1982). Indeed, directly comparing predictions from the candidate models to the observed monthly means reveals little else than a common, correlated, hardly discriminating, disagreement mainly due to crustal anomalies. We repeated the comparison after correcting the monthly means for the crustal anomalies derived by Bloxham and Jackson (1992). This second test was much more significant and showed that the models do a comparable job, UB-95 being marginally better. We recommand equal weighing between the two GS-95 and IZ-95 candidate models, and a slightly larger weight for UB-95.</div></front></TEI><affiliations><list><country><li>France</li></country><region><li>Île-de-France</li></region><settlement><li>Paris</li></settlement></list><tree><country name="France"><region name="Île-de-France"><name sortKey="Cohen, Y" sort="Cohen, Y" uniqKey="Cohen Y" first="Y." last="Cohen">Y. Cohen</name></region><name sortKey="Alexandrescu, M" sort="Alexandrescu, M" uniqKey="Alexandrescu M" first="M." last="Alexandrescu">M. Alexandrescu</name><name sortKey="Hulot, G" sort="Hulot, G" uniqKey="Hulot G" first="G." last="Hulot">G. Hulot</name><name sortKey="Le Mouel, J L" sort="Le Mouel, J L" uniqKey="Le Mouel J" first="J. L." last="Le Mouël">J. L. Le Mouël</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Asie/explor/AustralieFrV1/Data/Main/Exploration
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 00D069 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/Main/Exploration/biblio.hfd -nk 00D069 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Wicri/Asie
|area= AustralieFrV1
|flux= Main
|étape= Exploration
|type= RBID
|clé= Pascal:97-0406882
|texte= Candidate models for the 1995 revision of IGRF, a worldwide evaluation based on observatory monthly means
}}
| This area was generated with Dilib version V0.6.33. |  |