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Magnetic Reynolds number

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1439:. All three can be regarded as giving the ratio of advective to diffusive effects for a particular physical field and have the form of the product of a velocity and a length divided by a diffusivity. While the magnetic Reynolds number is related to the magnetic field in an magnetohydrodynamic flow, the Reynolds number is related to the fluid velocity itself and the PĂ©clet number is related to heat. The dimensionless groups arise in the non-dimensionalization of the respective governing equations: the induction equation, the 963:
is estimated to be of order 10 . Dissipation is more significant, but a magnetic field is supported by motion in the liquid iron outer core. There are other bodies in the solar system that have working dynamos, e.g. Jupiter, Saturn, and Mercury, and others that do not, e.g. Mars, Venus and the Moon.
1047:
must be large enough such that induction outweighs diffusion. It is not the absolute magnitude of velocity that is important for induction, but rather the relative differences and shearing in the flow, which stretch and fold magnetic field lines . A more appropriate form for the magnetic Reynolds
383: 194: 669: 1112: 738: 796: 1200: 300: 278:. When the magnetic Reynolds number is very large, however, diffusion and the dynamo are less of a concern, and in this case focus instead often rests on the influence of the magnetic field on the flow. 890:. Flux lines of the magnetic field are then advected with the fluid flow, until such time as gradients are concentrated into regions of short enough length scale that diffusion can balance advection. 1318: 79: 1401: 1002: 884: 844: 1146: 1045: 961: 927: 504: 2166: 846:, advection is relatively unimportant, and so the magnetic field will tend to relax towards a purely diffusive state, determined by the boundary conditions rather than the flow. 606: 1519: 558: 435: 411: 1649: 1605: 1268: 1566: 1480: 1364: 457: 264: 1544: 1229: 1421: 1341: 1004:. The generation of magnetic field by the motion of a conducting fluid has been achieved in only a handful of large experiments using mercury or liquid sodium. 578: 524: 242: 220: 2159: 1273:
Many studies of the generation of magnetic field by a flow consider the computationally-convenient periodic cube. In this case the minimum is found to be
614: 2511: 2152: 1054: 680: 1651:
the skin effect dominates and the braking torque decreases much slower with increasing speed than predicted by the induction motor model.
378:{\displaystyle {\frac {\partial \mathbf {B} }{\partial t}}=\nabla \times (\mathbf {u} \times \mathbf {B} )+\eta \nabla ^{2}\mathbf {B} } 929:, of order 10. Dissipative affects are generally small, and there is no difficulty in maintaining a magnetic field against diffusion. 749: 1154: 2175: 17: 2099: 1279: 1833:
Moncheaux, R.; et al. (2007). "Generation of a Magnetic Field by Dynamo Action in a Turbulent Flow of Liquid Sodium".
189:{\displaystyle \mathrm {R} _{\mathrm {m} }={\frac {UL}{\eta }}~~\sim {\frac {\mathrm {induction} }{\mathrm {diffusion} }}} 1369: 970: 852: 812: 2134: 2115: 1117:
where S is a measure of strain. One of the most well known results is due to Backus which states that the minimum
1120: 1019: 935: 901: 478: 1696: 475:. The relative importance of these two terms can be found by taking their ratio, the magnetic Reynolds number 2521: 2321: 1440: 2064:
Ripper, M.D; Endean, V.G (Mar 1975). "Eddy-Current Braking-Torque Measurements on a Thick Copper Disc".
583: 2138: 2119: 1488: 529: 468: 274:
The mechanism by which the motion of a conducting fluid generates a magnetic field is the subject of
1919: 2381: 418: 394: 2516: 2376: 1798:
Steiglitz, R.; U. Muller (2001). "Experimental demonstration of a homogeneous two-scale dynamo".
1621: 1577: 1270:
is the maximum strain rate. This bound has since been improved by approximately 25% by Proctor.
2276: 1968:
Proctor, M. (1977). "On Backus' necessary condition for dynamo action in a conducting sphere".
1234: 46: 1906: 1737:
Gailitis, A.; et al. (2001). "Magnetic field saturation in the Riga dynamo experiment".
1551: 2231: 2144: 2022: 1977: 1942: 1852: 1807: 1756: 1711: 1665: 1458: 1346: 460: 442: 287: 267: 249: 31: 2236: 1529: 8: 1208: 2301: 2026: 1981: 1946: 1856: 1811: 1760: 1715: 2485: 2271: 2211: 2046: 2012: 1876: 1842: 1780: 1746: 1612: 1406: 1326: 563: 509: 472: 291: 227: 205: 62: 54: 2440: 2405: 2186: 2130: 2111: 2095: 2038: 1954: 1895: 1868: 1772: 1013: 2050: 1880: 1697:"Constraints from material properties on the dynamics and evolution of Earth's core" 2490: 2361: 2346: 2311: 2221: 2073: 2034: 2030: 1985: 1950: 1860: 1815: 1764: 1719: 1660: 664:{\displaystyle \nabla \times (\mathbf {u} \times \mathbf {B} )\sim {\frac {UB}{L}}} 2366: 1864: 1784: 1675: 1432: 2455: 2435: 2393: 2388: 2216: 2103: 1670: 1436: 70: 66: 1768: 2465: 2445: 2430: 2425: 2371: 2356: 2331: 2326: 2316: 2296: 2286: 2251: 2196: 1933:
Backus, G. (1958). "A class of self-sustaining dissipative spherical dynamos".
58: 1989: 2505: 2475: 2470: 2460: 2450: 2415: 2410: 2351: 2291: 2281: 2261: 2256: 2226: 2191: 1444: 275: 1012:
In situations where permanent magnetisation is not possible, e.g. above the
2480: 2420: 2336: 2306: 2266: 2241: 2201: 2077: 2042: 1872: 1776: 1107:{\displaystyle \mathrm {\hat {R}} _{\mathrm {m} }={\frac {L^{2}S}{\eta }}} 2341: 2246: 2206: 1608: 1343:
is the root-mean-square strain over a scaled domain with sides of length
733:{\displaystyle \eta \nabla ^{2}\mathbf {B} \sim {\frac {\eta B}{L^{2}}}.} 1847: 1751: 1366:. If shearing over small length scales in the cube is ruled out, then 1819: 1723: 50: 1426: 1148:
for generation of a magnetic field by flow in a sphere is such that
1482:, is also used in cases where there is no physical fluid involved. 2017: 801: 1521:× (characteristic length) × (characteristic velocity) 791:{\displaystyle \mathrm {R} _{\mathrm {m} }={\frac {UL}{\eta }}.} 467:
The first term on the right hand side accounts for effects from
1195:{\displaystyle \mathrm {\hat {R}} _{\mathrm {m} }\geq \pi ^{2}} 2174: 1615:
torque follows the theoretical curve of an induction motor.
1431:
The magnetic Reynolds number has a similar form to both the
471:
in the plasma and the second term accounts for effects from
2003:
Willis, A. (2012). "Optimization of the Magnetic Dynamo".
886:, diffusion is relatively unimportant on the length scale 506:. If it is assumed that both terms share the scale length 2118:) (Ed. G.K. Batchelor, H.K. Moffatt & M.G. Worster) 1450: 1313:{\displaystyle \mathrm {\hat {R}} _{\mathrm {m} }=2.48} 967:
The human length scale is very small so that typically
290:, the magnetic Reynolds number can be derived from the 1624: 1580: 1554: 1532: 1491: 1461: 1409: 1372: 1349: 1329: 1282: 1237: 1211: 1157: 1123: 1057: 1022: 973: 938: 904: 855: 815: 752: 683: 617: 586: 566: 532: 512: 481: 445: 421: 397: 303: 252: 230: 208: 82: 1797: 1643: 1599: 1560: 1538: 1513: 1474: 1415: 1395: 1358: 1335: 1312: 1262: 1223: 1194: 1140: 1106: 1039: 996: 955: 921: 878: 838: 790: 732: 663: 600: 572: 552: 518: 498: 451: 429: 405: 377: 258: 236: 214: 188: 1427:Relationship to Reynolds number and PĂ©clet number 2503: 1396:{\displaystyle \mathrm {R} _{\mathrm {m} }=1.73} 997:{\displaystyle \mathrm {R} _{\mathrm {m} }\ll 1} 879:{\displaystyle \mathrm {R} _{\mathrm {m} }\gg 1} 839:{\displaystyle \mathrm {R} _{\mathrm {m} }\ll 1} 1970:Geophysical & Astrophysical Fluid Dynamics 27:Dimensionless quantity in magnetohydrodynamics 2160: 802:General characteristics for large and small R 2063: 1455:The dimensionless magnetic Reynolds number, 61:by the motion of a conducting medium to the 1141:{\displaystyle \mathrm {R} _{\mathrm {m} }} 1040:{\displaystyle \mathrm {R} _{\mathrm {m} }} 956:{\displaystyle \mathrm {R} _{\mathrm {m} }} 922:{\displaystyle \mathrm {R} _{\mathrm {m} }} 499:{\displaystyle \mathrm {R} _{\mathrm {m} }} 2167: 2153: 2016: 1846: 1832: 1750: 2512:Dimensionless numbers of fluid mechanics 2176:Dimensionless numbers in fluid mechanics 1736: 743:The ratio of the two terms is therefore 222:is a typical velocity scale of the flow, 2127:An Introduction to Magnetohydrodynamics 1967: 1893: 608:, the induction term can be written as 49:that estimates the relative effects of 14: 2504: 2002: 1932: 1694: 244:is a typical length scale of the flow, 2148: 1896:"Reflections on Magnetohydrodynamics" 65:. It is the magnetic analogue of the 1451:Relationship to eddy current braking 2096:Reflections on Magnetohydrodynamics 24: 2088: 1381: 1375: 1298: 1287: 1173: 1162: 1132: 1126: 1073: 1062: 1031: 1025: 982: 976: 947: 941: 913: 907: 893: 864: 858: 824: 818: 761: 755: 688: 618: 601:{\displaystyle \mathbf {u} \sim U} 533: 490: 484: 361: 329: 317: 307: 180: 177: 174: 171: 168: 165: 162: 159: 156: 151: 148: 145: 142: 139: 136: 133: 130: 127: 91: 85: 25: 2533: 1514:{\displaystyle R_{m}=\mu \sigma } 1048:number in this case is therefore 1695:Davies, C.; et al. (2015). 1231:is the radius of the sphere and 698: 636: 628: 588: 423: 399: 371: 347: 339: 311: 1568:is the electrical conductivity. 1423:is the root-mean-square value. 1016:, to maintain a magnetic field 553:{\displaystyle \nabla \sim 1/L} 2108:Perspectives in Fluid Dynamics 2057: 2035:10.1103/PhysRevLett.109.251101 1996: 1961: 1926: 1887: 1826: 1791: 1730: 1688: 1290: 1165: 1065: 640: 624: 351: 335: 13: 1: 1865:10.1103/PhysRevLett.98.044502 1681: 281: 73:and is typically defined by: 1955:10.1016/0003-4916(58)90054-X 1546:is the magnetic permeability 430:{\displaystyle \mathbf {u} } 406:{\displaystyle \mathbf {B} } 7: 1769:10.1103/PhysRevLett.86.3024 1654: 1644:{\displaystyle R_{m}>30} 10: 2538: 2139:Cambridge University Press 2120:Cambridge University Press 2094:Moffatt, H. Keith, 2000, " 1600:{\displaystyle R_{m}<1} 674:and the diffusion term as 2182: 1990:10.1080/03091927708242317 1263:{\displaystyle S=e_{max}} 1007: 36:magnetic Reynolds number 18:Magnetic Reynolds Number 2005:Physical Review Letters 1835:Physical Review Letters 1739:Physical Review Letters 1561:{\displaystyle \sigma } 1441:Navier–Stokes equations 560:and the scale velocity 2125:P. A. Davidson, 2001, 2078:10.1049/piee.1975.0080 1914:Cite journal requires 1645: 1611:is negligible and the 1601: 1562: 1540: 1515: 1476: 1417: 1403:is the minimum, where 1397: 1360: 1337: 1314: 1264: 1225: 1196: 1142: 1108: 1041: 998: 957: 923: 880: 840: 792: 734: 665: 602: 574: 554: 520: 500: 453: 437:is the fluid velocity, 431: 413:is the magnetic field, 407: 379: 260: 238: 216: 190: 47:dimensionless quantity 1646: 1602: 1563: 1541: 1516: 1477: 1475:{\displaystyle R_{m}} 1418: 1398: 1361: 1359:{\displaystyle 2\pi } 1338: 1315: 1265: 1226: 1197: 1143: 1109: 1042: 999: 958: 924: 881: 841: 793: 735: 666: 603: 575: 555: 521: 501: 454: 452:{\displaystyle \eta } 432: 408: 380: 261: 259:{\displaystyle \eta } 239: 217: 191: 2522:Magnetohydrodynamics 1894:Moffatt, K. (2000). 1666:Magnetohydrodynamics 1622: 1613:eddy current braking 1578: 1552: 1539:{\displaystyle \mu } 1530: 1489: 1459: 1407: 1370: 1347: 1327: 1280: 1235: 1209: 1155: 1121: 1055: 1020: 971: 936: 902: 898:The Sun has a large 853: 813: 750: 681: 615: 584: 564: 530: 510: 479: 461:magnetic diffusivity 443: 419: 395: 301: 288:magnetohydrodynamics 268:magnetic diffusivity 250: 228: 206: 80: 32:magnetohydrodynamics 2027:2012PhRvL.109y1101W 1982:1977GApFD...9...89P 1947:1958AnPhy...4..372B 1857:2007PhRvL..98d4502M 1812:2001PhFl...13..561S 1761:2001PhRvL..86.3024G 1716:2015NatGe...8..678D 1224:{\displaystyle L=a} 2322:Keulegan–Carpenter 2102:2007-09-29 at the 1641: 1597: 1558: 1536: 1511: 1472: 1413: 1393: 1356: 1333: 1310: 1260: 1221: 1192: 1138: 1104: 1037: 994: 953: 919: 876: 836: 788: 730: 661: 598: 570: 550: 516: 496: 473:magnetic diffusion 469:magnetic induction 449: 427: 403: 375: 292:induction equation 256: 234: 212: 186: 63:magnetic diffusion 2499: 2498: 1820:10.1063/1.1331315 1800:Physics of Fluids 1745:(14): 3024–3027. 1704:Nature Geoscience 1416:{\displaystyle U} 1336:{\displaystyle S} 1293: 1168: 1102: 1068: 1014:Curie temperature 783: 725: 659: 573:{\displaystyle U} 519:{\displaystyle L} 324: 286:In the theory of 237:{\displaystyle L} 215:{\displaystyle U} 184: 120: 117: 113: 16:(Redirected from 2529: 2169: 2162: 2155: 2146: 2145: 2082: 2081: 2061: 2055: 2054: 2020: 2000: 1994: 1993: 1965: 1959: 1958: 1930: 1924: 1923: 1917: 1912: 1910: 1902: 1900: 1891: 1885: 1884: 1850: 1830: 1824: 1823: 1795: 1789: 1788: 1754: 1734: 1728: 1727: 1724:10.1038/ngeo2492 1701: 1692: 1661:Lundquist number 1650: 1648: 1647: 1642: 1634: 1633: 1606: 1604: 1603: 1598: 1590: 1589: 1567: 1565: 1564: 1559: 1545: 1543: 1542: 1537: 1520: 1518: 1517: 1512: 1501: 1500: 1481: 1479: 1478: 1473: 1471: 1470: 1422: 1420: 1419: 1414: 1402: 1400: 1399: 1394: 1386: 1385: 1384: 1378: 1365: 1363: 1362: 1357: 1342: 1340: 1339: 1334: 1319: 1317: 1316: 1311: 1303: 1302: 1301: 1295: 1294: 1286: 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218: 213: 195: 193: 192: 187: 185: 183: 154: 125: 118: 115: 114: 109: 101: 96: 95: 94: 88: 21: 2537: 2536: 2532: 2531: 2530: 2528: 2527: 2526: 2502: 2501: 2500: 2495: 2178: 2173: 2104:Wayback Machine 2091: 2089:Further reading 2086: 2085: 2062: 2058: 2001: 1997: 1966: 1962: 1931: 1927: 1915: 1913: 1904: 1903: 1898: 1892: 1888: 1848:physics/0701075 1831: 1827: 1796: 1792: 1752:physics/0010047 1735: 1731: 1699: 1693: 1689: 1684: 1671:Reynolds number 1657: 1629: 1625: 1623: 1620: 1619: 1585: 1581: 1579: 1576: 1575: 1553: 1550: 1549: 1531: 1528: 1527: 1496: 1492: 1490: 1487: 1486: 1466: 1462: 1460: 1457: 1456: 1453: 1437:Reynolds number 1429: 1408: 1405: 1404: 1380: 1379: 1374: 1373: 1371: 1368: 1367: 1348: 1345: 1344: 1328: 1325: 1324: 1297: 1296: 1285: 1284: 1283: 1281: 1278: 1277: 1248: 1244: 1236: 1233: 1232: 1210: 1207: 1206: 1186: 1182: 1172: 1171: 1160: 1159: 1158: 1156: 1153: 1152: 1131: 1130: 1125: 1124: 1122: 1119: 1118: 1089: 1085: 1084: 1082: 1072: 1071: 1060: 1059: 1058: 1056: 1053: 1052: 1030: 1029: 1024: 1023: 1021: 1018: 1017: 1010: 981: 980: 975: 974: 972: 969: 968: 946: 945: 940: 939: 937: 934: 933: 932:For the Earth, 912: 911: 906: 905: 903: 900: 899: 896: 894:Range of values 863: 862: 857: 856: 854: 851: 850: 823: 822: 817: 816: 814: 811: 810: 807: 805: 772: 770: 760: 759: 754: 753: 751: 748: 747: 719: 715: 707: 705: 697: 691: 687: 682: 679: 678: 648: 646: 635: 627: 616: 613: 612: 587: 585: 582: 581: 565: 562: 561: 542: 531: 528: 527: 511: 508: 507: 489: 488: 483: 482: 480: 477: 476: 444: 441: 440: 422: 420: 417: 416: 398: 396: 393: 392: 370: 364: 360: 346: 338: 316: 310: 306: 304: 302: 299: 298: 284: 251: 248: 247: 229: 226: 225: 207: 204: 203: 155: 126: 124: 102: 100: 90: 89: 84: 83: 81: 78: 77: 71:fluid mechanics 67:Reynolds number 43: 28: 23: 22: 15: 12: 11: 5: 2535: 2525: 2524: 2519: 2517:Fluid dynamics 2514: 2497: 2496: 2494: 2493: 2488: 2483: 2478: 2473: 2468: 2463: 2458: 2453: 2448: 2443: 2438: 2433: 2428: 2423: 2418: 2413: 2408: 2403: 2402: 2401: 2391: 2386: 2385: 2384: 2379: 2369: 2364: 2359: 2354: 2349: 2344: 2339: 2334: 2329: 2324: 2319: 2314: 2309: 2304: 2299: 2294: 2289: 2284: 2279: 2274: 2269: 2264: 2259: 2254: 2249: 2244: 2239: 2234: 2229: 2224: 2219: 2214: 2209: 2204: 2199: 2194: 2189: 2183: 2180: 2179: 2172: 2171: 2164: 2157: 2149: 2143: 2142: 2123: 2090: 2087: 2084: 2083: 2072:(3): 301–302. 2056: 2011:(25): 251101. 1995: 1960: 1941:(4): 372–447. 1925: 1916:|journal= 1886: 1825: 1806:(3): 561–564. 1790: 1729: 1710:(9): 678–685. 1686: 1685: 1683: 1680: 1679: 1678: 1673: 1668: 1663: 1656: 1653: 1640: 1637: 1632: 1628: 1596: 1593: 1588: 1584: 1572: 1571: 1570: 1569: 1557: 1547: 1535: 1525: 1510: 1507: 1504: 1499: 1495: 1469: 1465: 1452: 1449: 1428: 1425: 1412: 1392: 1389: 1383: 1377: 1355: 1352: 1332: 1321: 1320: 1309: 1306: 1300: 1292: 1289: 1257: 1254: 1251: 1247: 1243: 1240: 1220: 1217: 1214: 1203: 1202: 1189: 1185: 1181: 1175: 1167: 1164: 1134: 1128: 1115: 1114: 1101: 1097: 1092: 1088: 1081: 1075: 1067: 1064: 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044502. 1840: 1836: 1829: 1821: 1817: 1813: 1809: 1805: 1801: 1794: 1786: 1782: 1778: 1774: 1770: 1766: 1762: 1758: 1753: 1748: 1744: 1740: 1733: 1725: 1721: 1717: 1713: 1709: 1705: 1698: 1691: 1687: 1677: 1676:PĂ©clet number 1674: 1672: 1669: 1667: 1664: 1662: 1659: 1658: 1652: 1638: 1635: 1630: 1626: 1616: 1614: 1610: 1594: 1591: 1586: 1582: 1555: 1548: 1533: 1526: 1523: 1522: 1508: 1505: 1502: 1497: 1493: 1485: 1484: 1483: 1467: 1463: 1448: 1446: 1445:heat equation 1442: 1438: 1434: 1433:PĂ©clet number 1424: 1410: 1390: 1387: 1353: 1350: 1330: 1307: 1304: 1276: 1275: 1274: 1271: 1255: 1252: 1249: 1245: 1241: 1238: 1218: 1215: 1212: 1187: 1183: 1179: 1151: 1150: 1149: 1099: 1095: 1090: 1086: 1079: 1051: 1050: 1049: 1015: 1005: 991: 988: 965: 930: 891: 889: 873: 870: 847: 833: 830: 785: 780: 776: 773: 767: 746: 745: 744: 727: 720: 716: 711: 708: 702: 692: 684: 677: 676: 675: 656: 652: 649: 643: 632: 621: 611: 610: 609: 595: 592: 567: 547: 543: 539: 536: 513: 474: 470: 462: 446: 439: 415: 391: 390: 389: 365: 357: 354: 343: 332: 326: 320: 297: 296: 295: 293: 289: 279: 277: 276:dynamo theory 269: 253: 246: 231: 224: 209: 202: 201: 200: 121: 110: 106: 103: 97: 76: 75: 74: 72: 68: 64: 60: 56: 52: 48: 44: 37: 33: 19: 2398: 2126: 2122:, p 347–391. 2107: 2069: 2065: 2059: 2008: 2004: 1998: 1976:(1): 89–93. 1973: 1969: 1963: 1938: 1934: 1928: 1907:cite journal 1889: 1838: 1834: 1828: 1803: 1799: 1793: 1742: 1738: 1732: 1707: 1703: 1690: 1617: 1573: 1454: 1430: 1322: 1272: 1204: 1116: 1011: 966: 931: 897: 887: 848: 808: 742: 673: 466: 387: 285: 273: 198: 39: 35: 29: 2486:Weissenberg 1609:skin effect 2506:Categories 2406:Richardson 2187:Archimedes 1901:: 347–391. 1682:References 1443:, and the 580:such that 526:such that 282:Derivation 2491:Womersley 2382:turbulent 2362:Ohnesorge 2347:Marangoni 2312:Iribarren 2237:Damköhler 2222:Capillary 2018:1209.1559 1935:Ann. Phys 1556:σ 1534:μ 1509:σ 1506:μ 1354:π 1291:^ 1184:π 1180:≥ 1166:^ 1100:η 1066:^ 989:≪ 871:≫ 831:≪ 781:η 709:η 703:∼ 689:∇ 685:η 644:∼ 633:× 622:× 619:∇ 593:∼ 537:∼ 534:∇ 447:η 362:∇ 358:η 344:× 333:× 330:∇ 318:∂ 308:∂ 254:η 122:∼ 111:η 55:induction 51:advection 2466:Suratman 2456:Strouhal 2436:Sherwood 2399:magnetic 2394:Reynolds 2389:Rayleigh 2377:magnetic 2217:Brinkman 2100:Archived 2066:Proc IEE 2051:23466555 2043:23368443 1881:21114816 1873:17358779 1777:11290098 1655:See also 1435:and the 2446:Stanton 2441:Shields 2431:Scruton 2426:Schmidt 2372:Prandtl 2357:Nusselt 2332:Laplace 2327:Knudsen 2317:Kapitza 2302:Görtler 2297:Grashof 2287:Galilei 2252:Deborah 2197:Bagnold 2023:Bibcode 1978:Bibcode 1943:Bibcode 1853:Bibcode 1808:Bibcode 1757:Bibcode 1712:Bibcode 459:is the 266:is the 45:) is a 2476:Ursell 2471:Taylor 2461:Stuart 2451:Stokes 2416:Rossby 2411:Roshko 2367:PĂ©clet 2352:Morton 2292:Graetz 2282:Froude 2272:Eötvös 2262:Eckert 2257:Dukhin 2227:Cauchy 2192:Atwood 2133:  2114:  2106:. In: 2049:  2041:  1879:  1871:  1785:638748 1783:  1775:  1323:where 1205:where 1008:Bounds 388:where 199:where 119:  116:  34:, the 2481:Weber 2421:Rouse 2337:Lewis 2307:Hagen 2277:Euler 2267:Ekman 2242:Darcy 2202:Bejan 2047:S2CID 2013:arXiv 1899:(PDF) 1877:S2CID 1843:arXiv 1781:S2CID 1747:arXiv 1700:(PDF) 1524:where 57:of a 2342:Mach 2247:Dean 2212:Bond 2207:Biot 2131:ISBN 2112:ISBN 2039:PMID 1920:help 1869:PMID 1773:PMID 1636:> 1618:For 1607:the 1592:< 1574:For 1391:1.73 1308:2.48 849:For 809:For 2137:), 2074:doi 2070:122 2031:doi 2009:109 1986:doi 1951:doi 1861:doi 1816:doi 1765:doi 1720:doi 69:in 53:or 30:In 2508:: 2098:" 2068:. 2045:. 2037:. 2029:. 2021:. 2007:. 1984:. 1972:. 1949:. 1937:. 1911:: 1909:}} 1905:{{ 1875:. 1867:. 1859:. 1851:. 1839:98 1837:. 1814:. 1804:13 1802:. 1779:. 1771:. 1763:. 1755:. 1743:86 1741:. 1718:. 1706:. 1702:. 1639:30 1447:. 294:: 2168:e 2161:t 2154:v 2141:. 2129:( 2110:( 2080:. 2076:: 2053:. 2033:: 2025:: 2015:: 1992:. 1988:: 1980:: 1974:9 1957:. 1953:: 1945:: 1939:4 1922:) 1918:( 1883:. 1863:: 1855:: 1845:: 1822:. 1818:: 1810:: 1787:. 1767:: 1759:: 1749:: 1726:. 1722:: 1714:: 1708:8 1631:m 1627:R 1595:1 1587:m 1583:R 1503:= 1498:m 1494:R 1468:m 1464:R 1411:U 1388:= 1382:m 1376:R 1351:2 1331:S 1305:= 1299:m 1288:R 1256:x 1253:a 1250:m 1246:e 1242:= 1239:S 1219:a 1216:= 1213:L 1188:2 1174:m 1163:R 1133:m 1127:R 1096:S 1091:2 1087:L 1080:= 1074:m 1063:R 1032:m 1026:R 992:1 983:m 977:R 948:m 942:R 914:m 908:R 888:L 874:1 865:m 859:R 834:1 825:m 819:R 804:m 786:. 777:L 774:U 768:= 762:m 756:R 728:. 721:2 717:L 712:B 699:B 693:2 657:L 653:B 650:U 641:) 637:B 629:u 625:( 596:U 589:u 568:U 548:L 544:/ 540:1 514:L 491:m 485:R 463:. 424:u 400:B 372:B 366:2 355:+ 352:) 348:B 340:u 336:( 327:= 321:t 312:B 270:. 232:L 210:U 181:n 178:o 175:i 172:s 169:u 166:f 163:f 160:i 157:d 152:n 149:o 146:i 143:t 140:c 137:u 134:d 131:n 128:i 107:L 104:U 98:= 92:m 86:R 42:m 40:R 38:( 20:)

Index

Magnetic Reynolds Number
magnetohydrodynamics
dimensionless quantity
advection
induction
magnetic field
magnetic diffusion
Reynolds number
fluid mechanics
magnetic diffusivity
dynamo theory
magnetohydrodynamics
induction equation
magnetic diffusivity
magnetic induction
magnetic diffusion
Curie temperature
PĂ©clet number
Reynolds number
Navier–Stokes equations
heat equation
skin effect
eddy current braking
Lundquist number
Magnetohydrodynamics
Reynolds number
PĂ©clet number
"Constraints from material properties on the dynamics and evolution of Earth's core"
Bibcode
2015NatGe...8..678D

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