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International Geomagnetic Reference Field

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Fratter, Isabelle; Gillet, Nicolas; Hamilton, Brian; Hamoudi, Mohamed; Hulot, Gauthier; Jager, Thomas; Korte, Monika; Kuang, Weijia; Lalanne, Xavier; Langlais, Benoit; Léger, Jean-Michel; Lesur, Vincent; Lowes, Frank J; Macmillan, Susan; Mandea, Mioara; Manoj, Chandrasekharan; Maus, Stefan; Olsen, Nils; Petrov, Valeriy; Ridley, Victoria; Rother, Martin; Sabaka, Terence J; Saturnino, Diana; Schachtschneider, Reyko; Sirol, Olivier; Tangborn, Andrew; Thomson, Alan; Tøffner-Clausen, Lars; Vigneron, Pierre; Wardinski, Ingo; Zvereva, Tatiana (27 May 2015).
25: 144:, which is intended for navigation in the next few years.) It is updated at 5-year intervals, reflecting the most accurate measurements available at that time. The current 13th edition of the IGRF model (IGRF-13) was released in December 2019 and is valid from 1900 until 2025. For the interval from 1945 to 2015, it is "definitive" (a "DGRF"), meaning that future updates are unlikely to improve the model in any significant way. 476: 1538: 754: 263: 1355: 1451:
Thébault, Erwan; Finlay, Christopher C; Beggan, Ciarán D; Alken, Patrick; Aubert, Julien; Barrois, Olivier; Bertrand, Francois; Bondar, Tatiana; Boness, Axel; Brocco, Laura; Canet, Elisabeth; Chambodut, Aude; Chulliat, Arnaud; Coïsson, Pierdavide; Civet, François; Du, Aimin; Fournier, Alexandre;
1185: 514: 133:. It was created by fitting parameters of a mathematical model of the magnetic field to measured magnetic field data from surveys, observatories and satellites across the globe. The IGRF has been produced and updated under the direction of the 471:{\displaystyle {\vec {B}}(r,\phi ,\theta ,t)=-\nabla V(r,\phi ,\theta ,t)=-\left({\dfrac {\partial V}{\partial r}},{\dfrac {1}{r}}{\dfrac {\partial V}{\partial \theta }},{\dfrac {1}{r\sin \theta }}{\dfrac {\partial V}{\partial \phi }}\right)} 1196: 1023: 749:{\displaystyle V(r,\phi ,\theta ,t)=a\sum _{n=1}^{N}\sum _{m=0}^{n}\left({\frac {a}{r}}\right)^{n+1}\left(g_{n}^{m}(t)\cos m\phi +h_{n}^{m}(t)\sin m\phi \right)P_{n}^{m}\left(\cos \theta \right)} 972: 206: 256: 921: 889: 1397: 42: 837: 817: 1350:{\displaystyle K_{n}={\begin{cases}{\frac {1}{2^{n}}}&{\text{; }}m=0\\{\frac {1}{2^{n}}}{\sqrt {\frac {2(n-m)!}{(n+m)!}}}&{\text{; }}m>0\end{cases}}} 1016: 996: 857: 797: 777: 507: 134: 482: 89: 61: 1399:
term usually present in the associated Legendre functions is omitted in this formulation and is instead accounted for in the Gauss coefficients.
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The IGRF model covers a significant time span, and so is useful for interpreting historical data. (This is unlike the
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The Gauss coefficients are modelled as a piecewise-linear function of time with a 5-year step size.
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is the normalization coefficient for the Schmidt quasi-normalized formulation.
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is a standard mathematical description of the large-scale structure of the
1545: 24: 1501:"The International Geomagnetic Reference Field: A "Health" Warning" 1454:"International Geomagnetic Reference Field: the 12th generation" 1416: 1343: 1503:. IAGA working group V-MOD: Geomagnetic Field Modeling. 1450: 16:
Standard model of the structure of Earth's magnetic field
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International Association of Geomagnetism and Aeronomy
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Notes concerning correct use and limitations of IGRF
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The magnetic scalar potential model consists of the
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Unsourced material may be challenged and removed. 1391: 1349: 1179: 1010: 990: 967:{\displaystyle P_{n}^{m}\left(\cos \theta \right)} 966: 915: 883: 851: 831: 811: 791: 771: 748: 501: 470: 250: 200: 1590: 123:International Geomagnetic Reference Field (IGRF) 1446: 1444: 1442: 1573: 201:{\displaystyle {\vec {B}}(r,\phi ,\theta ,t)} 779:is radial distance from the Earth's center, 1439: 58:"International Geomagnetic Reference Field" 1580: 1566: 1480: 109:Learn how and when to remove this message 1494: 1492: 799:is the maximum degree of the expansion, 1591: 152:The IGRF models the geomagnetic field 147: 1498: 1489: 1532: 251:{\displaystyle V(r,\phi ,\theta ,t)} 47:adding citations to reliable sources 18: 13: 453: 445: 405: 397: 368: 360: 312: 14: 1620: 1515: 974:are the Schmidt quasi-normalized 839:is colatitude (the polar angle), 1536: 1507:from the original on 2018-06-30. 23: 34:needs additional citations for 1522:IGRF Model Description by IAGA 1380: 1370: 1314: 1302: 1294: 1282: 1168: 1142: 1124: 1111: 1054: 1042: 692: 686: 653: 647: 545: 521: 342: 318: 303: 279: 273: 245: 221: 195: 171: 165: 1: 1432: 976:associated Legendre functions 1552:. You can help Knowledge by 1499:Lowes, F.J. (January 2010). 923:are Gauss coefficients, and 7: 1609:Magnetic field of the Earth 1405: 127:Earth's main magnetic field 10: 1625: 1531: 1482:10.1186/s40623-015-0228-9 916:{\displaystyle h_{n}^{m}} 884:{\displaystyle g_{n}^{m}} 210:magnetic scalar potential 1461:Earth, Planets and Space 1392:{\displaystyle (-1)^{m}} 1473:2015EP&S...67...79T 859:is the Earth's radius, 832:{\displaystyle \theta } 1548:-related article is a 1393: 1351: 1181: 1012: 992: 968: 917: 885: 853: 833: 813: 793: 773: 750: 595: 574: 503: 472: 252: 202: 1394: 1352: 1182: 1013: 993: 969: 918: 886: 854: 834: 814: 812:{\displaystyle \phi } 794: 774: 751: 575: 554: 504: 473: 253: 203: 1412:Geomagnetic latitude 1367: 1197: 1024: 1002: 982: 927: 895: 863: 843: 823: 803: 783: 763: 515: 493: 264: 215: 156: 142:World Magnetic Model 43:improve this article 1041: 944: 912: 880: 819:is East longitude, 726: 685: 646: 208:as a gradient of a 148:Spherical Harmonics 137:(IAGA) since 1965. 1422:Ørsted (satellite) 1389: 1347: 1342: 1177: 1027: 1008: 988: 964: 930: 913: 898: 881: 866: 849: 829: 809: 789: 769: 746: 712: 671: 632: 499: 487:spherical harmonic 483:Gauss coefficients 468: 461: 439: 413: 391: 376: 248: 198: 1561: 1560: 1427:CHAMP (satellite) 1329: 1322: 1321: 1273: 1243: 1236: 1140: 1088: 1011:{\displaystyle m} 991:{\displaystyle n} 852:{\displaystyle a} 792:{\displaystyle N} 772:{\displaystyle r} 609: 502:{\displaystyle V} 460: 438: 412: 390: 375: 276: 168: 131:secular variation 119: 118: 111: 93: 1616: 1599:Geophysics stubs 1582: 1575: 1568: 1540: 1533: 1509: 1508: 1496: 1487: 1486: 1484: 1458: 1448: 1398: 1396: 1395: 1390: 1388: 1387: 1356: 1354: 1353: 1348: 1346: 1345: 1330: 1327: 1323: 1320: 1300: 1277: 1276: 1274: 1272: 1271: 1259: 1244: 1241: 1237: 1235: 1234: 1222: 1209: 1208: 1186: 1184: 1183: 1178: 1176: 1175: 1154: 1153: 1141: 1139: 1138: 1137: 1106: 1105: 1090: 1086: 1079: 1078: 1069: 1068: 1040: 1035: 1017: 1015: 1014: 1009: 997: 995: 994: 989: 973: 971: 970: 965: 963: 959: 943: 938: 922: 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591: 586: 583: 580: 576: 570: 565: 562: 559: 555: 551: 548: 542: 539: 536: 533: 530: 527: 524: 518: 511: 510: 509: 496: 489:expansion of 488: 484: 464: 456: 448: 434: 431: 428: 425: 421: 415: 408: 400: 387: 384: 378: 371: 363: 352: 348: 345: 339: 336: 333: 330: 327: 324: 321: 315: 309: 306: 300: 297: 294: 291: 288: 285: 282: 270: 260: 259: 258: 242: 239: 236: 233: 230: 227: 224: 218: 211: 192: 189: 186: 183: 180: 177: 174: 162: 145: 143: 138: 136: 132: 128: 124: 113: 110: 102: 91: 88: 84: 81: 77: 74: 70: 67: 63: 60: –  59: 55: 54:Find sources: 48: 44: 38: 37: 32:This article 30: 26: 21: 20: 1604:Geomagnetism 1554:expanding it 1543: 1464: 1460: 1401: 1362: 1359: 1189: 758: 480: 151: 139: 122: 120: 105: 96: 86: 79: 72: 65: 53: 41:Please help 36:verification 33: 1593:Categories 1546:geophysics 1433:References 998:and order 978:of degree 69:newspapers 1374:− 1289:− 1162:− 1159:θ 1156:⁡ 1121:θ 1118:⁡ 1084:θ 1081:⁡ 1052:θ 1049:⁡ 957:θ 954:⁡ 827:θ 807:ϕ 739:θ 736:⁡ 705:ϕ 699:⁡ 666:ϕ 660:⁡ 577:∑ 556:∑ 537:θ 531:ϕ 457:ϕ 454:∂ 446:∂ 435:θ 432:⁡ 409:θ 406:∂ 398:∂ 369:∂ 361:∂ 349:− 334:θ 328:ϕ 313:∇ 310:− 295:θ 289:ϕ 274:→ 237:θ 231:ϕ 187:θ 181:ϕ 166:→ 99:June 2016 1505:Archived 1406:See also 129:and its 1469:Bibcode 1328:;  1242:;  83:scholar 1467:(79). 1417:Magsat 1190:where 1087:  759:where 85:  78:  71:  64:  56:  1544:This 1457:(PDF) 90:JSTOR 76:books 1550:stub 1363:The 1335:> 891:and 121:The 62:news 1477:doi 1147:cos 1115:cos 1072:sin 1046:cos 951:cos 733:cos 696:sin 657:cos 429:sin 45:by 1595:: 1491:^ 1475:. 1465:67 1463:. 1459:. 1441:^ 1581:e 1574:t 1567:v 1556:. 1485:. 1479:: 1471:: 1385:m 1381:) 1377:1 1371:( 1338:0 1332:m 1318:! 1315:) 1312:m 1309:+ 1306:n 1303:( 1298:! 1295:) 1292:m 1286:n 1283:( 1280:2 1269:n 1265:2 1261:1 1252:0 1249:= 1246:m 1232:n 1228:2 1224:1 1216:{ 1211:= 1206:n 1202:K 1173:n 1169:) 1165:1 1151:2 1143:( 1135:n 1132:+ 1129:m 1125:) 1112:( 1109:d 1103:n 1100:+ 1097:m 1093:d 1076:m 1066:n 1062:K 1058:= 1055:) 1043:( 1038:m 1033:n 1029:P 1006:m 986:n 961:) 947:( 941:m 936:n 932:P 909:m 904:n 900:h 877:m 872:n 868:g 847:a 787:N 767:r 743:) 729:( 723:m 718:n 714:P 709:) 702:m 693:) 690:t 687:( 682:m 677:n 673:h 669:+ 663:m 654:) 651:t 648:( 643:m 638:n 634:g 629:( 623:1 620:+ 617:n 612:) 607:r 604:a 599:( 592:n 587:0 584:= 581:m 571:N 566:1 563:= 560:n 552:a 549:= 546:) 543:t 540:, 534:, 528:, 525:r 522:( 519:V 497:V 465:) 449:V 426:r 422:1 416:, 401:V 388:r 385:1 379:, 372:r 364:V 353:( 346:= 343:) 340:t 337:, 331:, 325:, 322:r 319:( 316:V 307:= 304:) 301:t 298:, 292:, 286:, 283:r 280:( 271:B 246:) 243:t 240:, 234:, 228:, 225:r 222:( 219:V 196:) 193:t 190:, 184:, 178:, 175:r 172:( 163:B 112:) 106:( 101:) 97:( 87:· 80:· 73:· 66:· 39:.

Index


verification
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adding citations to reliable sources
"International Geomagnetic Reference Field"
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JSTOR
Learn how and when to remove this message
Earth's main magnetic field
secular variation
International Association of Geomagnetism and Aeronomy
World Magnetic Model
magnetic scalar potential
Gauss coefficients
spherical harmonic
associated Legendre functions
Geomagnetic latitude
Magsat
Ørsted (satellite)
CHAMP (satellite)



"International Geomagnetic Reference Field: the 12th generation"
Bibcode
2015EP&S...67...79T
doi

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