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Kennelly–Heaviside layer

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133: 36: 254:), scientists were unwilling to believe the speed in the ionosphere could be higher. Nevertheless, Marconi had received signals in Newfoundland that were broadcast in England, so clearly there must be some mechanism allowing the transmission to reach that far. The paradox was resolved by the discovery that there were two velocities of light, the 321:
proposed the name "Heaviside Layer" for the radio-wave reflecting layer in the upper atmosphere, and the name has subsequently been widely adopted. The name Kennelly–Heaviside layer was proposed in 1925 to give credit to the work of Kennelly, which predated the proposal by Heaviside by several
205:) side of the Earth, the solar wind drags the ionosphere further away, thereby greatly increasing the range which radio waves can travel by reflection. The extent of the effect is further influenced by the 248:, which in turn would require that the speed of light in the ionosphere would be greater than in the atmosphere below it. Since the latter speed is essentially the same as the speed of light in vacuum ( 282:, and that makes total internal reflection possible, and so the ionosphere can reflect radio waves. The geometric mean of the phase velocity and the group velocity cannot exceed 53: 100: 194:" or "skip" propagation technique has been used since the 1920s for radio communication at long distances, up to transcontinental distances. 72: 582: 79: 305:
standard model of absorption and reflection of radio waves by the Heaviside Layer was developed by the British Ionospheric physicist
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Existence of a reflective layer was predicted in 1902 independently and almost simultaneously by the American electrical engineer
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occurring roughly between 90km and 150 km (56 and 93 mi) above the ground — one of several layers in the
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presses this layer closer to the Earth, thereby limiting how far it can reflect radio waves. Conversely, on the night (
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Proceedings of the Royal Society of London, Series A, Containing Papers of a Mathematical and Physical Character,
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Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences,
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Physicists resisted the idea of the reflecting layer for one very good reason; it would require
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in 1901. However, it was not until 1924 that its existence was shown by British scientist
557: 440: 381: 331: 262: 256: 249: 571: 298: 294: 132: 483: 466: 270:, but the group velocity, being capable of transmitting information, cannot, by 35: 504:"On some direct evidence for downward atmospheric reflection of electric rays" 278:. The phase velocity for radio waves in the ionosphere is indeed greater than 198: 183: 180: 172: 161: 137: 458: 544:
L.M. Muggleton (1975). "A method of predicting foE at any time and place".
523: 423:"Atmospheric Pressure and the Ionisation of the Kennelly-Heaviside Layer" 365: 17: 210: 191: 187: 449: 422: 206: 524:
Nobel Prizes for 1947: Sir Edward Appleton, G.B.E., K.C.B., F.R.S."
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Propagation is affected by the time of day. During the daytime the
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first mapped the Heaviside layer's variations in altitude. The
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Appleton, Edward V., and Barnett, M. A. F. (1 December 1925).
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Proceedings of the Institute of Radio Engineers, 4,
60:. Unsourced material may be challenged and removed. 266:. The phase velocity can in fact be greater than 140:. The Kennelly–Heaviside layer is the E region 478: 476: 376: 374: 8: 396: 394: 349: 347: 448: 355:Oliver Heaviside and the Heaviside layer" 120:Learn how and when to remove this message 290:, the group velocity must go below it. 286:, so when the phase velocity goes above 343: 366:https://doi.org/10.1098/rsta.2017.0459 353:Griffiths, Hugh (15 November 2018). " 225:(1861–1939) and the British polymath 7: 58:adding citations to reliable sources 25: 400:McAdie, Alexander (22 May 1925) " 237:, for which he received the 1947 482:Russell, A. (24 October 1925). " 34: 484:The “Kennelly-Heaviside” Layer" 45:needs additional citations for 27:Layer of the Earth's ionosphere 493:, p. 609. doi:10.1038/116609c0 380:Marchant, E. W. (Dec. 1916). " 1: 546:ITU Telecommunication Journal 402:The Kennelly-Heaviside Layer" 583:Radio frequency propagation 599: 175:. It is also known as the 69:"Kennelly–Heaviside layer" 368:. Retrieved 14 June 2019. 246:total internal reflection 150:Kennelly–Heaviside layer 148:, sometimes called the 421:Martyn, D. F. (1934). 239:Nobel Prize in Physics 141: 223:Arthur Edwin Kennelly 135: 382:The Heaviside layer" 209:, and the amount of 54:improve this article 558:1975ITUTJ..42..413M 441:1934Natur.133R.294M 388:No. 6, pp. 511–520. 293:In 1925, Americans 274:, be greater than 272:special relativity 235:Edward V. Appleton 154:Arthur E. Kennelly 142: 513:.752 pp. 621–641. 231:Guglielmo Marconi 130: 129: 122: 104: 16:(Redirected from 590: 562: 561: 541: 535: 520: 514: 500: 494: 480: 471: 470: 452: 450:10.1038/133294b0 418: 412: 398: 389: 378: 369: 351: 227:Oliver Heaviside 181:medium-frequency 160:, is a layer of 158:Oliver Heaviside 125: 118: 114: 111: 105: 103: 62: 38: 30: 21: 598: 597: 593: 592: 591: 589: 588: 587: 568: 567: 566: 565: 543: 542: 538: 521: 517: 501: 497: 481: 474: 420: 419: 415: 399: 392: 379: 372: 352: 345: 340: 328: 315: 307:Louis Muggleton 219: 179:. It reflects 146:Heaviside layer 126: 115: 109: 106: 63: 61: 51: 39: 28: 23: 22: 15: 12: 11: 5: 596: 594: 586: 585: 580: 570: 569: 564: 563: 536: 515: 495: 472: 413: 390: 370: 342: 341: 339: 336: 335: 334: 332:Van Allen Belt 327: 324: 319:William Eccles 314: 311: 309:in the 1970s. 263:group velocity 257:phase velocity 218: 215: 152:, named after 136:Layers of the 128: 127: 110:September 2015 42: 40: 33: 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 595: 584: 581: 579: 576: 575: 573: 559: 555: 551: 547: 540: 537: 533: 529: 525: 519: 516: 512: 509: 505: 499: 496: 492: 489: 485: 479: 477: 473: 468: 464: 460: 456: 451: 446: 442: 438: 435:(3356): 294. 434: 430: 429: 424: 417: 414: 410: 407: 403: 397: 395: 391: 387: 383: 377: 375: 371: 367: 363: 360: 356: 350: 348: 344: 337: 333: 330: 329: 325: 323: 320: 317:Around 1910, 312: 310: 308: 304: 300: 299:Merle A. Tuve 296: 295:Gregory Breit 291: 289: 285: 281: 277: 273: 269: 265: 264: 259: 258: 253: 252: 247: 242: 240: 236: 232: 228: 224: 216: 214: 212: 208: 204: 200: 195: 193: 189: 185: 182: 178: 174: 170: 166: 163: 159: 155: 151: 147: 139: 134: 124: 121: 113: 102: 99: 95: 92: 88: 85: 81: 78: 74: 71: –  70: 66: 65:Find sources: 59: 55: 49: 48: 43:This article 41: 37: 32: 31: 19: 549: 545: 539: 531: 527: 518: 510: 507: 498: 490: 487: 432: 426: 416: 408: 405: 385: 364:: No. 2134. 361: 358: 316: 292: 287: 283: 279: 275: 267: 261: 255: 250: 243: 220: 196: 176: 149: 145: 143: 116: 107: 97: 90: 83: 76: 64: 52:Please help 47:verification 44: 552:: 413–418. 184:radio waves 578:Ionosphere 572:Categories 338:References 213:activity. 199:solar wind 173:ionosphere 138:ionosphere 80:newspapers 459:0028-0836 313:Etymology 190:. This " 406:Science, 326:See also 322:months. 260:and the 177:E region 18:E region 554:Bibcode 437:Bibcode 217:History 211:sunspot 192:skywave 188:horizon 162:ionised 94:scholar 528:Nature 488:Nature 467:684206 465:  457:  428:Nature 207:season 96:  89:  82:  75:  67:  463:S2CID 169:Earth 101:JSTOR 87:books 455:ISSN 297:and 156:and 144:The 73:news 532:160 511:109 491:116 445:doi 433:133 362:376 303:ITU 203:lee 171:'s 165:gas 56:by 574:: 550:42 548:. 530:, 526:, 506:, 486:, 475:^ 461:. 453:. 443:. 431:. 425:. 409:61 404:, 393:^ 384:, 373:^ 357:, 346:^ 241:. 560:. 556:: 522:" 469:. 447:: 439:: 288:c 284:c 280:c 276:c 268:c 251:c 123:) 117:( 112:) 108:( 98:· 91:· 84:· 77:· 50:. 20:)

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ionosphere
Arthur E. Kennelly
Oliver Heaviside
ionised
gas
Earth
ionosphere
medium-frequency
radio waves
horizon
skywave
solar wind
lee
season
sunspot
Arthur Edwin Kennelly
Oliver Heaviside

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