Knowledge (XXG)

Field line

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the simultaneous begin and end of field lines takes place. This situation happens, for instance, in the middle between two identical positive electric point charges. There, the field vanishes and the lines coming axially from the charges end. At the same time, in the transverse plane passing through the middle point, an infinite number of field lines diverge radially. The concomitant presence of the lines that end and begin preserves the divergence-free character of the field in the point.
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confusing most field line diagrams are of this type. Since at each point where it is nonzero and finite the vector field has a unique direction, field lines can never intersect, so there is exactly one field line passing through each point at which the vector field is nonzero and finite. Points where the field is zero or infinite have no field line through them, since direction cannot be defined there, but can be the
28: 1013:(i.e., a vector field where the divergence is zero everywhere), the field lines neither begin nor end; they either form closed loops, or go off to infinity in both directions. If a vector field has positive divergence in some area, there will be field lines starting from points in that area. If a vector field has negative divergence in some area, there will be field lines ending at points in that area. 1053: 1057: 1056: 1052: 1051: 1058: 101: 1055: 129:
vector field may be depicted by different sets of field lines. A field line diagram is necessarily an incomplete description of a vector field, since it gives no information about the field between the drawn field lines, and the choice of how many and which lines to show determines how much useful information the diagram gives.
148:. Then the density of field lines (number of field lines per unit perpendicular area) at any location is proportional to the magnitude of the vector field at that point. Areas in which neighboring field lines are converging (getting closer together) indicates that the field is getting stronger in that direction. 875:
By repeating this and connecting the points, the field line can be extended as far as desired. This is only an approximation to the actual field line, since each straight segment isn't actually tangent to the field along its length, just at its starting point. But by using a small enough value for
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form closed loops, extend to infinity in both directions, or continue indefinitely without ever crossing itself. However, as stated above, a special situation may occur around points where the field is zero (that cannot be intersected by field lines, because their direction would not be defined) and
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properties of the filings they damp the field to either side, creating the apparent spaces between the lines that we see. Of course the two stages described here happen concurrently until an equilibrium is achieved. Because the intrinsic magnetism of the filings modifies the field, the lines shown
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The iron filings in the photo appear to be aligning themselves with discrete field lines, but the situation is more complex. It is easy to visualize as a two-stage-process: first, the filings are spread evenly over the magnetic field but all aligned in the direction of the field. Then, based on the
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Since there are an infinite number of points in any region, an infinite number of field lines can be drawn; but only a limited number can be shown on a field line diagram. Therefore which field lines are shown is a choice made by the person or computer program which draws the diagram, and a single
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may be easily seen through field lines, assuming the lines are drawn such that the density of field lines is proportional to the magnitude of the field (see above). In this case, the divergence may be seen as the beginning and ending of field lines. If the vector field is the resultant of radial
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to the field vector at each point. A field line is usually shown as a directed line segment, with an arrowhead indicating the direction of the vector field. For two-dimensional fields the field lines are plane curves; since a plane drawing of a 3-dimensional set of field lines can be visually
624: 198:, sinks at negative charges, and neither elsewhere, so electric field lines start at positive charges and end at negative charges. A gravitational field has no sources, it has sinks at masses, and it has neither elsewhere, gravitational field lines come from infinity and end at masses. A 1054: 214:
Note that for this kind of drawing, where the field-line density is intended to be proportional to the field magnitude, it is important to represent all three dimensions. For example, consider the electric field arising from a single, isolated
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that happen to be on the same field line interact strongly, while particles on different field lines in general do not interact. This is the same behavior that the particles of iron filings exhibit in a magnetic field.
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at each point along its length. A diagram showing a representative set of neighboring field lines is a common way of depicting a vector field in scientific and mathematical literature; this is called a
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This article is about the modern use of "field lines" as a way to depict electromagnetic and other vector fields. For the role of these lines in the early history and philosophy of electromagnetism, see
727: 664: 402: 219:. The electric field lines in this case are straight lines that emanate from the charge uniformly in all directions in three-dimensional space. This means that their density is proportional to 104:
The figure at left shows the electric field lines of two isolated equal positive charges. The figure at right shows the electric field lines of two isolated equal charges of opposite sign.
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In physics, drawings of field lines are mainly useful in cases where the sources and sinks, if any, have a physical meaning, as opposed to e.g. the case of a force field of a
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for that vector field and may be constructed by starting at a point and tracing a line through space that follows the direction of the vector field, by making the field line
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inverse-square law fields with respect to one or more sources then this corresponds to the fact that the divergence of such a field is zero outside the sources. In a
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for this case. However, if the electric field lines for this setup were just drawn on a two-dimensional plane, their two-dimensional density would be proportional to
252: 899:, taking a greater number of shorter steps, the field line can be approximated as closely as desired. The field line can be extended in the opposite direction from 411: 952: 284: 897: 687: 507: 1036:) cannot be closed loops. In other words, curl is always present when a field line forms a closed loop. It may be present in other situations too, such as a 1104:
by the filings are only an approximation of the field lines of the original magnetic field. Magnetic fields are continuous, and do not have discrete lines.
868:{\displaystyle \mathbf {x} _{\text{i+1}}=\mathbf {x} _{\text{i}}+{\mathbf {F} (\mathbf {x} _{\text{i}}) \over |\mathbf {F} (\mathbf {x} _{\text{i}})|}ds} 619:{\displaystyle \mathbf {x} _{\text{1}}=\mathbf {x} _{\text{0}}+{\mathbf {F} (\mathbf {x} _{\text{0}}) \over |\mathbf {F} (\mathbf {x} _{\text{0}})|}ds} 1079: 89: 1389: 1202: 1170: 1440: 31:
Field lines depicting the electric field created by a positive charge (left), negative charge (center), and uncharged object (right).
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While field lines are a "mere" mathematical construction, in some circumstances they take on physical significance. In
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filings arrange themselves so as to approximately depict some magnetic field lines. The magnetic field is created by a
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of the field, field line diagrams are often drawn so that each line represents the same quantity of
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in the flow. Perhaps the most familiar example of a vector field described by field lines is the
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a field line can be constructed iteratively by finding the field vector at that point
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Interactive Java applet showing the electric field lines of selected pairs of charges
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defines a direction and magnitude at each point in space. A field line is an
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course notes from a course at the Massachusetts Institute of Technology.
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by taking each step in the opposite direction by using a negative step
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and end on negative charges. In fields which are divergenceless (
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along the field direction a new point on the line can be found
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Field lines can be used to trace familiar quantities from
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Visualization of Fields and Applications in Engineering
155:, field lines begin on points of positive divergence ( 1420:"Visualization of Fields and the Divergence and Curl" 934: 905: 882: 764: 735: 722:{\displaystyle \mathbf {F} (\mathbf {x} _{\text{2}})} 695: 672: 659:{\displaystyle \mathbf {F} (\mathbf {x} _{\text{1}})} 632: 515: 492: 414: 397:{\displaystyle \mathbf {F} (\mathbf {x} _{\text{0}})} 370: 341: 308: 264: 225: 206:), so its field lines have no start or end: they can 1126:— field lines of Douady–Hubbard potential of 1020:shows that field lines of a vector field with zero 1373: 1354:Am. J. Phys., Vol. 64, No. 6. (1996), pp. 714–724 946: 920: 891: 867: 750: 721: 681: 658: 618: 501: 478: 396: 356: 327: 278: 246: 1304:"The Misconception of Closed Magnetic Flux Lines" 1062:When randomly dropped (as with the shaker here), 966:Different ways to depict the field of a magnet. 8: 159:) and end on points of negative divergence ( 1231:Haus, Herman A.; Mechior, James R. (1998). 729:of the field line is found. At each point 328:{\displaystyle \mathbf {F} (\mathbf {x} )} 286:, an incorrect result for this situation. 1376:Introduction to Electrodynamics (3rd ed.) 1327: 1283: 1196: 1194: 1192: 933: 912: 907: 904: 881: 851: 842: 837: 828: 823: 812: 807: 798: 795: 786: 781: 771: 766: 763: 742: 737: 734: 710: 705: 696: 694: 671: 647: 642: 633: 631: 602: 593: 588: 579: 574: 563: 558: 549: 546: 537: 532: 522: 517: 514: 491: 471: 462: 457: 448: 443: 438: 429: 424: 415: 413: 385: 380: 371: 369: 348: 343: 340: 317: 309: 307: 268: 263: 238: 229: 224: 16:Visual aid to depiction of a vector field 1048: 961: 163:), or extend to infinity. For example, 1352:Electric field line diagrams don't work 1158: 921:{\displaystyle \mathbf {x} _{\text{0}}} 751:{\displaystyle \mathbf {x} _{\text{i}}} 666:is found and moving a further distance 357:{\displaystyle \mathbf {x} _{\text{0}}} 1350:A. Wolf, S. J. Van Hook, E. R. Weeks, 1226: 1224: 1164: 1162: 254:, the correct result consistent with 7: 1297: 1295: 151:In vector fields which have nonzero 1175:. John Wiley and Sons. p. 64. 132:An individual field line shows the 1258:Lieberherr, Martin (6 July 2010). 1204:Vectors in Physics and Engineering 14: 1237:Electromagnetic fields and energy 689:in that direction the next point 1302:Zilberti, Luca (25 April 2017). 970:If the vector field describes a 908: 838: 829: 808: 799: 782: 767: 738: 706: 697: 643: 634: 589: 580: 559: 550: 533: 518: 458: 449: 425: 416: 381: 372: 344: 318: 310: 136:of the vector field but not the 1207:. CRC Press. pp. 129–130. 758:the next point can be found by 977:, then the field lines follow 852: 848: 833: 824: 818: 803: 716: 701: 653: 638: 603: 599: 584: 575: 569: 554: 486:. By moving a short distance 472: 468: 453: 444: 435: 420: 391: 376: 322: 314: 140:. In order to also depict the 47:. It consists of an imaginary 1: 1070:underneath the glass surface. 626:Then the field at that point 1372:Griffiths, David J. (1998). 1078:, the velocity field lines ( 298:Construction of a field line 76:among many other types. In 1264:American Journal of Physics 1457: 1441:Numerical function drawing 1380:. Prentice Hall. pp.  96:Definition and description 80:, field lines showing the 18: 1320:10.1109/LMAG.2017.2698038 1147:Line integral convolution 1119:Field lines of Julia sets 1026:conservative vector field 204:Gauss's law for magnetism 202:has no sources or sinks ( 64:. They are used to show 194:has sources at positive 167:lines begin on positive 1011:solenoidal vector field 247:{\displaystyle 1/r^{2}} 1308:IEEE Magnetics Letters 1201:Durrant, Alan (1996). 1071: 967: 948: 922: 893: 869: 752: 723: 683: 660: 620: 503: 480: 398: 358: 329: 299: 280: 248: 105: 32: 1169:Tou, Stephen (2011). 1114:Force field (physics) 1061: 1045:Physical significance 1040:shape of field lines. 1018:Kelvin–Stokes theorem 965: 949: 923: 894: 870: 753: 724: 684: 661: 621: 504: 481: 399: 359: 335:and a starting point 330: 302:Given a vector field 297: 281: 249: 103: 30: 1132:filled-in Julia sets 932: 903: 880: 762: 733: 693: 670: 630: 513: 490: 412: 368: 339: 306: 262: 223: 74:gravitational fields 1356:DOI 10.1119/1.18237 1340:– via Zenodo. 1276:2010AmJPh..78.1117L 1034:electrostatic field 1030:gravitational field 993:Divergence and curl 947:{\displaystyle -ds} 279:{\displaystyle 1/r} 1412:2011-08-13 at the 1072: 968: 944: 918: 892:{\displaystyle ds} 889: 865: 748: 719: 682:{\displaystyle ds} 679: 656: 616: 502:{\displaystyle ds} 499: 476: 408:at that point is: 394: 354: 325: 300: 276: 244: 125:of field lines. 106: 62:field line diagram 33: 1416:by Wolfgang Bauer 1391:978-0-13-805326-0 1285:10.1119/1.3471233 1270:(11): 1117–1119. 1059: 915: 857: 845: 815: 789: 774: 745: 713: 650: 608: 596: 566: 540: 525: 465: 432: 388: 351: 1448: 1395: 1379: 1358: 1348: 1342: 1341: 1331: 1299: 1290: 1289: 1287: 1255: 1249: 1248: 1246: 1244: 1228: 1219: 1218: 1198: 1187: 1186: 1166: 1068:permanent magnet 1060: 953: 951: 950: 945: 927: 925: 924: 919: 917: 916: 913: 911: 898: 896: 895: 890: 874: 872: 871: 866: 858: 856: 855: 847: 846: 843: 841: 832: 827: 821: 817: 816: 813: 811: 802: 796: 791: 790: 787: 785: 776: 775: 772: 770: 757: 755: 754: 749: 747: 746: 743: 741: 728: 726: 725: 720: 715: 714: 711: 709: 700: 688: 686: 685: 680: 665: 663: 662: 657: 652: 651: 648: 646: 637: 625: 623: 622: 617: 609: 607: 606: 598: 597: 594: 592: 583: 578: 572: 568: 567: 564: 562: 553: 547: 542: 541: 538: 536: 527: 526: 523: 521: 508: 506: 505: 500: 485: 483: 482: 477: 475: 467: 466: 463: 461: 452: 447: 442: 434: 433: 430: 428: 419: 403: 401: 400: 395: 390: 389: 386: 384: 375: 363: 361: 360: 355: 353: 352: 349: 347: 334: 332: 331: 326: 321: 313: 285: 283: 282: 277: 272: 253: 251: 250: 245: 243: 242: 233: 169:electric charges 43:for visualizing 1456: 1455: 1451: 1450: 1449: 1447: 1446: 1445: 1436:Vector calculus 1426: 1425: 1414:Wayback Machine 1403: 1398: 1392: 1371: 1367: 1365:Further reading 1362: 1361: 1349: 1345: 1301: 1300: 1293: 1257: 1256: 1252: 1242: 1240: 1230: 1229: 1222: 1215: 1200: 1199: 1190: 1183: 1168: 1167: 1160: 1155: 1110: 1076:fluid mechanics 1049: 1047: 999:vector calculus 995: 960: 930: 929: 906: 901: 900: 878: 877: 836: 822: 806: 797: 780: 765: 760: 759: 736: 731: 730: 704: 691: 690: 668: 667: 641: 628: 627: 587: 573: 557: 548: 531: 516: 511: 510: 488: 487: 456: 423: 410: 409: 379: 366: 365: 342: 337: 336: 304: 303: 292: 260: 259: 234: 221: 220: 190:states that an 186:. For example, 184:radial harmonic 177:magnetic fields 98: 78:fluid mechanics 70:magnetic fields 66:electric fields 39:is a graphical 25: 17: 12: 11: 5: 1454: 1452: 1444: 1443: 1438: 1428: 1427: 1424: 1423: 1417: 1402: 1401:External links 1399: 1397: 1396: 1390: 1368: 1366: 1363: 1360: 1359: 1343: 1291: 1250: 1220: 1213: 1188: 1181: 1157: 1156: 1154: 1151: 1150: 1149: 1144: 1139: 1134: 1128:Mandelbrot set 1121: 1116: 1109: 1106: 1084:plasma physics 1046: 1043: 1042: 1041: 1014: 994: 991: 983:magnetic field 959: 956: 943: 940: 937: 910: 888: 885: 864: 861: 854: 850: 840: 835: 831: 826: 820: 810: 805: 801: 794: 784: 779: 769: 740: 718: 708: 703: 699: 678: 675: 655: 645: 640: 636: 615: 612: 605: 601: 591: 586: 582: 577: 571: 561: 556: 552: 545: 535: 530: 520: 498: 495: 474: 470: 460: 455: 451: 446: 441: 437: 427: 422: 418: 406:tangent vector 393: 383: 378: 374: 346: 324: 320: 316: 312: 291: 288: 275: 271: 267: 241: 237: 232: 228: 200:magnetic field 192:electric field 165:electric field 114:integral curve 97: 94: 49:integral curve 15: 13: 10: 9: 6: 4: 3: 2: 1453: 1442: 1439: 1437: 1434: 1433: 1431: 1421: 1418: 1415: 1411: 1408: 1405: 1404: 1400: 1393: 1387: 1383: 1382:65–67 and 232 1378: 1377: 1370: 1369: 1364: 1357: 1353: 1347: 1344: 1339: 1335: 1330: 1325: 1321: 1317: 1313: 1309: 1305: 1298: 1296: 1292: 1286: 1281: 1277: 1273: 1269: 1265: 1261: 1254: 1251: 1238: 1234: 1227: 1225: 1221: 1216: 1214:9780412627101 1210: 1206: 1205: 1197: 1195: 1193: 1189: 1184: 1182:9780470978467 1178: 1174: 1173: 1165: 1163: 1159: 1152: 1148: 1145: 1143: 1140: 1138: 1137:Line of force 1135: 1133: 1129: 1125: 1122: 1120: 1117: 1115: 1112: 1111: 1107: 1105: 1102: 1101:ferromagnetic 1096: 1093: 1089: 1085: 1081: 1077: 1069: 1065: 1044: 1039: 1035: 1031: 1027: 1023: 1019: 1015: 1012: 1007: 1004: 1003: 1002: 1000: 992: 990: 988: 984: 980: 976: 973: 964: 957: 955: 941: 938: 935: 886: 883: 862: 859: 792: 777: 676: 673: 613: 610: 543: 528: 496: 493: 439: 407: 296: 289: 287: 273: 269: 265: 257: 256:Coulomb's law 239: 235: 230: 226: 218: 212: 209: 205: 201: 197: 193: 189: 185: 180: 178: 174: 170: 166: 162: 158: 154: 149: 147: 143: 139: 135: 130: 126: 124: 119: 115: 111: 102: 95: 93: 91: 87: 83: 79: 75: 71: 67: 63: 58: 55:to the field 54: 50: 46: 45:vector fields 42: 38: 29: 23: 22:Line of force 1375: 1351: 1346: 1311: 1307: 1267: 1263: 1253: 1241:. Retrieved 1236: 1203: 1171: 1142:Vector field 1124:External ray 1097: 1073: 996: 979:stream lines 969: 301: 290:Construction 217:point charge 213: 207: 181: 160: 156: 150: 141: 137: 133: 131: 127: 122: 110:vector field 107: 61: 36: 34: 1329:11696/56339 1080:streamlines 404:. The unit 188:Gauss's law 175:), such as 90:streamlines 88:are called 84:field of a 1430:Categories 1243:9 November 1153:References 1099:scale and 1006:Divergence 173:solenoidal 153:divergence 86:fluid flow 41:visual aid 37:field line 1088:electrons 1028:, e.g. a 1024:(i.e., a 936:− 142:magnitude 138:magnitude 134:direction 123:endpoints 51:which is 1410:Archived 1338:39584751 1108:See also 972:velocity 958:Examples 82:velocity 1314:: 1–5. 1272:Bibcode 1038:helical 196:charges 157:sources 118:tangent 53:tangent 1388:  1336:  1211:  1179:  1032:or an 987:magnet 72:, and 57:vector 1334:S2CID 975:field 161:sinks 1386:ISBN 1245:2019 1209:ISBN 1177:ISBN 1092:ions 1064:iron 1022:curl 1016:The 208:only 146:flux 1324:hdl 1316:doi 1280:doi 1130:or 1090:or 773:i+1 1432:: 1384:. 1332:. 1322:. 1310:. 1306:. 1294:^ 1278:. 1268:78 1266:. 1262:. 1235:. 1223:^ 1191:^ 1161:^ 1086:, 1001:: 989:. 954:. 108:A 92:. 68:, 35:A 1394:. 1326:: 1318:: 1312:8 1288:. 1282:: 1274:: 1247:. 1217:. 1185:. 942:s 939:d 914:0 909:x 887:s 884:d 863:s 860:d 853:| 849:) 844:i 839:x 834:( 830:F 825:| 819:) 814:i 809:x 804:( 800:F 793:+ 788:i 783:x 778:= 768:x 744:i 739:x 717:) 712:2 707:x 702:( 698:F 677:s 674:d 654:) 649:1 644:x 639:( 635:F 614:s 611:d 604:| 600:) 595:0 590:x 585:( 581:F 576:| 570:) 565:0 560:x 555:( 551:F 544:+ 539:0 534:x 529:= 524:1 519:x 497:s 494:d 473:| 469:) 464:0 459:x 454:( 450:F 445:| 440:/ 436:) 431:0 426:x 421:( 417:F 392:) 387:0 382:x 377:( 373:F 350:0 345:x 323:) 319:x 315:( 311:F 274:r 270:/ 266:1 240:2 236:r 231:/ 227:1 24:.

Index

Line of force

visual aid
vector fields
integral curve
tangent
vector
electric fields
magnetic fields
gravitational fields
fluid mechanics
velocity
fluid flow
streamlines

vector field
integral curve
tangent
flux
divergence
electric field
electric charges
solenoidal
magnetic fields
radial harmonic
Gauss's law
electric field
charges
magnetic field
Gauss's law for magnetism

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