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Rock magnetism

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20: 814:"When I last did a magnetic experiment (about 1909) we were warned against careless handling of permanent magnets, and the magnetism was liable to change without much carelessness. In studying the magnetism of rocks the specimen has to be broken off with a geological hammer and then carried to the laboratory. It is supposed that in the process its magnetism does not change to any important extent, and though I have often asked how this comes to be the case I have never received any answer. 184:, skeptics were quick to question whether rocks could carry a stable remanence for geological ages. Rock magnetists were able to show that rocks could have more than one component of remanence, some soft (easily removed) and some very stable. To get at the stable part, they took to "cleaning" samples by heating them or exposing them to an alternating field. However, later events, particularly the recognition that many North American rocks had been pervasively remagnetized in the 409: 370: 304: 629:. The mineral recording the field commonly is hematite, another iron oxide. Redbeds, clastic sedimentary rocks (such as sandstones) that are red primarily because of hematite formation during or after sedimentary diagenesis, may have useful CRM signatures, and magnetostratigraphy can be based on such signatures. 637:
Magnetic grains in sediments may align with the magnetic field during or soon after deposition; this is known as detrital remanent magnetization (DRM). If the magnetization is acquired as the grains are deposited, the result is a depositional detrital remanent magnetization (dDRM); if it is acquired
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is often identified with a particular kind of remanence that is obtained after exposing a magnet to a field at room temperature. However, the Earth's field is not large, and this kind of remanence would be weak and easily overwritten by later fields. A central part of rock magnetism is the study of
361:. In these compounds, the iron atoms are not close enough for direct exchange, so they are coupled by indirect exchange or superexchange. The result is that the crystal lattice is divided into two or more sublattices with different moments. 624:
Magnetic grains may precipitate from a circulating solution, or be formed during chemical reactions, and may record the direction of the magnetic field at the time of mineral formation. The field is said to be recorded by
101:
Strongly magnetic minerals have properties that depend on the size, shape, defect structure and concentration of the minerals in a rock. Rock magnetism provides non-destructive methods for analyzing these minerals such as
496:. Because numerous experiments have been done modeling different ways of acquiring remanence, pTRM can have other meanings. For example, it can also be acquired in the laboratory by cooling in zero field to a temperature 585:
wander randomly. As the rock continues to cool, there is a critical temperature at which the magnetic anisotropy becomes large enough to keep the moment from wandering: this temperature is called the
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Rock magnetism had its start when scientists brought these two fields together in the laboratory. Koenigsberger (1938), Thellier (1938) and Nagata (1943) investigated the origin of
492:
If a rock is later re-heated (as a result of burial, for example), part or all of the TRM can be replaced by a new remanence. If it is only part of the remanence, it is known as
459:(NRM) in rocks obtained from the field and remanence induced in the laboratory. Below are listed the important natural remanences and some artificially induced kinds. 614: 552: 521: 188:, showed that a single cleaning step was inadequate, and paleomagnetists began to routinely use stepwise demagnetization to strip away the remanence in small bits. 419:, like ferrimagnets, have two sublattices with opposing moments, but now the moments are equal in magnitude. If the moments are exactly opposed, the magnet has no 396:
identified four types of temperature dependence, one of which involves a reversal of the magnetization. This phenomenon played a role in controversies over marine
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The contribution of a mineral to the total magnetism of a rock depends strongly on the type of magnetic order or disorder. Magnetically disordered minerals (
70:). An understanding of remanence helps paleomagnetists to develop methods for measuring the ancient magnetic field and correct for effects like sediment 260:
is negative. This effect is weak but independent of temperature. A substance whose only magnetic response is diamagnetism is called a diamagnet.
213:. The more important minerals for rock magnetism are the minerals that can be magnetically ordered, at least at some temperatures. These are the 279:. Paramagnetism occurs in certain kinds of iron-bearing minerals because the iron contains an unpaired electron in one of their shells (see 949:
McCabe, C.; Elmore, R. D. (1989). "The occurrence and origin of Late Paleozoic remagnetization in the sedimentary rocks of North America".
291:); others are magnetically ordered below a critical temperature and the susceptibility increases as it approaches that temperature (see 114:
and so on. With such methods, rock magnetists can measure the effects of past climate change and human impacts on the mineralogy (see
1026: 939: 870: 616:. The magnetization remains in the same state as the rock is cooled to room temperature and becomes a thermoremanent magnetization. 485:). This remanence can also be very stable, lasting without significant change for millions of years. TRM is the main reason that 712: 165:) that, if fulfilled, would allow the determination of the intensity of the ancient magnetic field to be determined using the 980:
Néel, Louis (1949). "Théorie du traînage magnétique des ferromagnétiques en grains fins avec application aux terres cuites".
675: 651: 456: 78:. Rock magnetic methods are used to get a more detailed picture of the source of the distinctive striped pattern in marine 24: 468: 158: 880:
Hunt, Christopher P.; Moskowitz, Bruce P. (1995). "Magnetic properties of rocks and minerals". In Ahrens, T. J. (ed.).
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developed a theory that explained these observations, showed that the Thellier laws were satisfied by certain kinds of
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from the Earth's field. TRM can be much larger than it would be if exposed to the same field at room temperature (see
573:, responding reversibly to changes in the magnetic field. For remanence to be possible there must be a strong enough 157:. By heating rocks and archeological materials to high temperatures in a magnetic field, they gave the materials a 161:(TRM), and they investigated the properties of this magnetization. Thellier developed a series of conditions (the 389: 354: 332: 107: 315:. However, this magnetism can arise as the result of more than one kind of magnetic order. In the strict sense, 174: 682:
can be altered by this process. To remove this component, some form of stepwise demagnetization must be used.
166: 380:
have two sublattices with opposing moments. One sublattice has a larger moment, so there is a net unbalance.
1063: 697: 284: 257: 115: 111: 19: 119: 1068: 951: 931: 862: 1010: 960: 898: 578: 320: 71: 292: 1073: 804: 707: 574: 440: 162: 103: 28: 727: 914: 732: 397: 79: 384:, the most important of the magnetic minerals, is a ferrimagnet. Ferrimagnets often behave like 339:
in their response to a changing magnetic field. Most importantly for rock magnetism, they have
1022: 935: 866: 570: 562: 524: 328: 245: 181: 91: 118:). In sediments, a lot of the magnetic remanence is carried by minerals that were created by 968: 906: 722: 702: 416: 408: 222: 87: 592: 530: 499: 240:
is a magnetic response shared by all substances. In response to an applied magnetic field,
1006: 717: 582: 486: 83: 280: 964: 902: 889:
Irving, E. (1956). "Paleomagnetic and palaeoclimatological aspects of polar wandering".
671: 369: 316: 303: 288: 276: 272: 253: 143: 139: 55: 43: 1057: 993:
Runcorn, S. K. (1956). "Paleomagnetic comparisons between Europe and North America".
918: 664: 566: 393: 268: 249: 170: 692: 679: 427:), resulting in a moment nearly at right angles to the moments of the sublattices. 424: 385: 377: 358: 312: 237: 218: 214: 154: 135: 123: 75: 350: 319:
refers to magnetic ordering where neighboring electron spins are aligned by the
206: 336: 256:. Thus, the moment produced is in the opposite direction to the field and the 202: 489:
are able to deduce the direction and magnitude of the ancient Earth's field.
62:
is carried by minerals, particularly certain strongly magnetic minerals like
972: 884:. Vol. 3. Washington, DC: American Geophysical Union. pp. 189–204. 660: 558: 482: 451: 420: 381: 340: 241: 226: 210: 185: 150: 67: 63: 59: 47: 225:. These minerals have a much stronger response to the field and can have a 1018: 667: 428: 39: 349:
does not occur widely in its pure form. It is usually incorporated into
910: 569:
but is not immediately capable of carrying a remanence. Instead, it is
474: 554:, then cooling the rest of the way to room temperature in zero field. 1048: 86:. They are also used to interpret terrestrial magnetic anomalies in 311:
Collectively, strongly magnetic materials are often referred to as
180:
When paleomagnetic work in the 1950s lent support to the theory of
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Rock Physics and Phase Relations: A Handbook of Physical Constants
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The standard model for TRM is as follows. When a mineral such as
346: 324: 95: 58:
to understand how rocks record the Earth's magnetic field. This
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Schematic of alternating spin directions in an antiferromagnet.
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Schematic of unbalanced antiparallel moments in a ferrimagnet.
1043: 122:, so rock magnetists have made significant contributions to 106:
measurements, temperature-dependent remanence measurements,
620:
Chemical (or crystallization) remanent magnetization (CRM)
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to keep the magnetization near a stable state; otherwise,
527:), applying a magnetic field and cooling to a temperature 928:
The earth: its origin, history, and physical constitution
283:). Some are paramagnetic down to absolute zero and their 640:
post-depositional detrital remanent magnetization (pDRM)
177:
magnets, and introduced the concept of blocking of TRM.
134:
Until the 20th century, the study of the Earth's field (
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Schematic of parallel spin directions in a ferromagnet.
595: 533: 502: 252:they act to shield the interior of a body from the 1049:UC Davis FORC Group, Introduction to FORC Diagrams 608: 546: 515: 287:is inversely proportional to the temperature (see 840: 759: 8: 829: 494:partial thermoremanent magnetization (pTRM) 859:Rock Magnetism: Fundamentals and Frontiers 659:, also known as viscous magnetization, is 388:, but the temperature dependence of their 327:. Below a critical temperature called the 209:) contribute a weak magnetism and have no 1015:The Physical Principles of Rock Magnetism 857:Dunlop, David J.; Ă–zdemir, Ă–zden (1997). 633:Depositional remanent magnetization (DRM) 600: 594: 538: 532: 507: 501: 815: 755: 753: 751: 749: 343:, so they can record the Earth's field. 142:) and of magnetic materials (especially 792: 745: 82:that provides important information on 811:, had the following to say about it: 781: 423:. However, the moments can be tilted ( 627:chemical remanent magnetization (CRM) 54:. The field arose out of the need in 7: 770: 657:Viscous remanent magnetization (VRM) 27:, a widely used tool for measuring 479:thermoremanent magnetization (TRM) 463:Thermoremanent magnetization (TRM) 14: 271:is a weak positive response to a 66:(the main source of magnetism in 713:Paleomagnetic secular variation 638:soon after deposition, it is a 16:The study of magnetism in rocks 807:, in his influential textbook 686:Applications of rock magnetism 676:natural remanent magnetization 652:Viscous remanent magnetization 646:Viscous remanent magnetization 589:and referred to by the symbol 457:natural remanent magnetization 1: 926:Jeffreys, Sir Harold (1959). 323:. The classic ferromagnet is 25:vibrating sample magnetometer 1044:Institute for Rock Magnetism 469:Thermoremanent magnetization 455:magnetic remanence, both as 431:has this kind of magnetism. 275:due to rotation of electron 159:thermoremanent magnetization 1090: 841:Stacey & Banerjee 1974 649: 477:rock cools, it acquires a 466: 438: 995:Proc. Geol. Assoc. Canada 760:Dunlop & Ă–zdemir 1997 390:spontaneous magnetization 333:spontaneous magnetization 830:McCabe & Elmore 1989 392:can be quite different. 167:Thellier–Thellier method 146:) developed separately. 973:10.1029/RG027i004p00471 698:Environmental magnetism 197:Types of magnetic order 116:environmental magnetism 112:ferromagnetic resonance 820: 610: 548: 517: 413: 374: 331:, ferromagnets have a 308: 120:magnetotactic bacteria 108:Mössbauer spectroscopy 90:as well as the strong 32: 952:Reviews of Geophysics 932:Cambridge Univ. Press 863:Cambridge Univ. Press 812: 611: 609:{\displaystyle T_{B}} 549: 547:{\displaystyle T_{2}} 518: 516:{\displaystyle T_{1}} 411: 372: 306: 221:and certain kinds of 22: 723:Petrofabric analysis 663:that is acquired by 593: 587:blocking temperature 579:thermal fluctuations 531: 500: 483:isothermal remanence 321:exchange interaction 38:is the study of the 965:1989RvGeo..27..471M 903:1956GeoPA..33...23I 805:Sir Harold Jeffreys 708:Magnetostratigraphy 674:for some time. The 575:magnetic anisotropy 441:Magnetic mineralogy 435:Magnetic mineralogy 104:magnetic hysteresis 29:magnetic hysteresis 1011:Banerjee, Subir K. 911:10.1007/BF02629944 891:Geofis. Pura. Appl 733:Structural Geology 703:Magnetic anomalies 606: 544: 513: 446:Types of remanence 414: 404:Antiferromagnetism 398:magnetic anomalies 375: 309: 80:magnetic anomalies 33: 571:superparamagnetic 563:Curie temperature 525:Curie temperature 329:Curie temperature 246:Larmor precession 182:continental drift 92:crustal magnetism 1081: 1032: 1007:Stacey, Frank D. 1002: 989: 976: 945: 922: 885: 876: 843: 838: 832: 827: 821: 801: 795: 790: 784: 779: 773: 768: 762: 757: 670:by sitting in a 615: 613: 612: 607: 605: 604: 561:cools below the 553: 551: 550: 545: 543: 542: 522: 520: 519: 514: 512: 511: 417:Antiferromagnets 223:antiferromagnets 88:magnetic surveys 1089: 1088: 1084: 1083: 1082: 1080: 1079: 1078: 1054: 1053: 1040: 1035: 1029: 1005: 992: 979: 948: 942: 925: 888: 879: 873: 856: 852: 847: 846: 839: 835: 828: 824: 802: 798: 791: 787: 780: 776: 769: 765: 758: 747: 742: 737: 718:Plate tectonics 688: 654: 648: 635: 622: 596: 591: 590: 583:magnetic moment 534: 529: 528: 503: 498: 497: 487:paleomagnetists 471: 465: 448: 443: 437: 406: 367: 301: 293:Curie–Weiss law 266: 235: 199: 194: 132: 84:plate tectonics 17: 12: 11: 5: 1087: 1085: 1077: 1076: 1071: 1066: 1064:Rock magnetism 1056: 1055: 1052: 1051: 1046: 1039: 1038:External links 1036: 1034: 1033: 1027: 1003: 990: 977: 959:(4): 471–494. 946: 940: 923: 886: 877: 871: 853: 851: 848: 845: 844: 833: 822: 818:, p. 371 803:For example, 796: 785: 774: 763: 744: 743: 741: 738: 736: 735: 730: 725: 720: 715: 710: 705: 700: 695: 689: 687: 684: 672:magnetic field 650:Main article: 647: 644: 634: 631: 621: 618: 603: 599: 541: 537: 510: 506: 467:Main article: 464: 461: 447: 444: 439:Main article: 436: 433: 405: 402: 366: 365:Ferrimagnetism 363: 317:ferromagnetism 300: 299:Ferromagnetism 297: 285:susceptibility 273:magnetic field 265: 262: 258:susceptibility 254:magnetic field 234: 231: 198: 195: 193: 190: 144:ferromagnetism 140:paleomagnetism 131: 128: 56:paleomagnetism 42:properties of 36:Rock magnetism 15: 13: 10: 9: 6: 4: 3: 2: 1086: 1075: 1072: 1070: 1067: 1065: 1062: 1061: 1059: 1050: 1047: 1045: 1042: 1041: 1037: 1030: 1028:0-444-41084-8 1024: 1020: 1016: 1012: 1008: 1004: 1000: 996: 991: 987: 983: 978: 974: 970: 966: 962: 958: 954: 953: 947: 943: 941:0-521-20648-0 937: 933: 929: 924: 920: 916: 912: 908: 904: 900: 896: 892: 887: 883: 878: 874: 872:0-521-32514-5 868: 864: 860: 855: 854: 849: 842: 837: 834: 831: 826: 823: 819: 817: 816:Jeffreys 1959 810: 806: 800: 797: 794: 789: 786: 783: 778: 775: 772: 767: 764: 761: 756: 754: 752: 750: 746: 739: 734: 731: 729: 726: 724: 721: 719: 716: 714: 711: 709: 706: 704: 701: 699: 696: 694: 691: 690: 685: 683: 681: 677: 673: 669: 666: 665:ferromagnetic 662: 658: 653: 645: 643: 641: 632: 630: 628: 619: 617: 601: 597: 588: 584: 580: 576: 572: 568: 567:ferromagnetic 565:, it becomes 564: 560: 555: 539: 535: 526: 508: 504: 495: 490: 488: 484: 480: 476: 470: 462: 460: 458: 453: 445: 442: 434: 432: 430: 426: 422: 418: 410: 403: 401: 399: 395: 391: 387: 383: 379: 371: 364: 362: 360: 356: 355:oxyhydroxides 352: 348: 344: 342: 338: 335:and there is 334: 330: 326: 322: 318: 314: 305: 298: 296: 294: 290: 286: 282: 278: 274: 270: 269:Paramagnetism 264:Paramagnetism 263: 261: 259: 255: 251: 247: 244:precess (see 243: 239: 232: 230: 228: 224: 220: 216: 212: 208: 204: 196: 191: 189: 187: 183: 178: 176: 175:single-domain 172: 168: 164: 163:Thellier laws 160: 156: 155:igneous rocks 152: 147: 145: 141: 137: 129: 127: 125: 121: 117: 113: 109: 105: 99: 97: 93: 89: 85: 81: 77: 73: 69: 65: 61: 57: 53: 49: 45: 41: 37: 30: 26: 21: 1069:Geomagnetism 1014: 998: 994: 985: 982:Ann. GĂ©ophys 981: 956: 950: 927: 897:(1): 23–41. 894: 890: 881: 858: 836: 825: 813: 808: 799: 793:Runcorn 1956 788: 777: 766: 728:Rock Physics 693:Biomagnetism 680:igneous rock 656: 655: 639: 636: 626: 623: 586: 556: 493: 491: 478: 472: 449: 425:spin canting 415: 386:ferromagnets 378:Ferrimagnets 376: 345: 313:ferromagnets 310: 281:Hund's rules 267: 238:Diamagnetism 236: 233:Diamagnetism 219:ferrimagnets 215:ferromagnets 200: 192:Fundamentals 179: 148: 136:geomagnetism 133: 124:biomagnetism 100: 76:metamorphism 35: 34: 782:Irving 1956 523:(below the 351:iron oxides 289:Curie's law 207:paramagnets 169:. In 1949, 1074:Geophysics 1058:Categories 850:References 394:Louis NĂ©el 337:hysteresis 250:Lenz's law 248:), and by 203:diamagnets 171:Louis NĂ©el 72:compaction 988:: 99–136. 919:129781412 809:The Earth 771:NĂ©el 1949 661:remanence 581:make the 559:magnetite 452:remanence 450:Magnetic 421:remanence 382:Magnetite 341:remanence 242:electrons 227:remanence 211:remanence 186:Paleozoic 151:remanence 68:lodestone 64:magnetite 60:remanence 48:sediments 1019:Elsevier 1013:(1974). 1001:: 77–85. 668:minerals 473:When an 429:Hematite 359:sulfides 40:magnetic 961:Bibcode 899:Bibcode 475:igneous 130:History 1025:  938:  917:  869:  678:of an 915:S2CID 740:Notes 277:spins 52:soils 44:rocks 1023:ISBN 936:ISBN 867:ISBN 357:and 347:Iron 325:iron 205:and 138:and 96:Mars 74:and 50:and 969:doi 907:doi 295:). 153:in 94:on 1060:: 1021:. 1017:. 1009:; 997:. 984:. 967:. 957:27 955:. 934:. 930:. 913:. 905:. 895:33 893:. 865:. 861:. 748:^ 642:. 400:. 353:, 229:. 217:, 126:. 110:, 98:. 46:, 23:A 1031:. 999:8 986:5 975:. 971:: 963:: 944:. 921:. 909:: 901:: 875:. 602:B 598:T 540:2 536:T 509:1 505:T 31:.

Index


vibrating sample magnetometer
magnetic hysteresis
magnetic
rocks
sediments
soils
paleomagnetism
remanence
magnetite
lodestone
compaction
metamorphism
magnetic anomalies
plate tectonics
magnetic surveys
crustal magnetism
Mars
magnetic hysteresis
Mössbauer spectroscopy
ferromagnetic resonance
environmental magnetism
magnetotactic bacteria
biomagnetism
geomagnetism
paleomagnetism
ferromagnetism
remanence
igneous rocks
thermoremanent magnetization

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