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Radio atmospheric signal

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standing resonant waves modes can exit. The fundamental mode which transports electric charge to the ground most effectively, has thus a wavelength λ four times the channel length L. In the case of the K stroke, the lower boundary is the same as the upper boundary. Of course, this picture is valid only for wave mode 1 (λ/4 antenna) and perhaps for mode 2 (λ/2 antenna), because these modes do not yet "feel" the contorted configuration of the real lightning channel. The higher order modes contribute to the incoherent noisy signals in the higher frequency range (> 100 kHz).
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sources of direct information about thunderstorm activity on the ground. Transients electric currents during return strokes (R strokes) or intracloud strokes (K strokes) are the main sources for the generation of impulse-type electromagnetic radiation known as sferics (sometimes called atmospherics). While this impulsive radiation dominates at frequencies less than about 100 kHz, (loosely called long waves), a continuous noise component becomes increasingly important at higher frequencies. The longwave electromagnetic propagation of sferics takes place within the
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magnetosphere, etc. dominates. In the VLF-range, there are the coherent impulses from R- and K-strokes, appearing out of the background noise. Beyond about 100 kHz, the noise amplitude becomes more and more incoherent. In addition, technical noise from electric motors, ignition systems of motor cars, etc., are superimposed. Finally, beyond the high frequency band (3–30 MHz) extraterrestrial noise (noise of galactic origin, solar noise) dominates.
31: 424:= very low frequencies, 3–30 kHz). These waves are reflected and attenuated on the ground as well as within the ionospheric D layer, near 70 km altitude during day time conditions, and near 90 km height during the night. Reflection and attenuation on the ground depends on frequency, distance, and 452:
out of a broadband signal. The 15 kHz signal dominates at distances greater than about 5000 km. For ELF waves (< 3 kHz), ray theory becomes invalid, and only mode theory is appropriate. Here, the zeroth mode begins to dominate and is responsible for the second window at greater distances.
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channel with all its branches and its electric currents behaves like a huge antenna system from which electromagnetic waves of all frequencies are radiated. Beyond a distance where luminosity is visible and thunder can be heard (typically about 10 km), these electromagnetic impulses are the only
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of a sferic signal at different frequencies together with its direction of arrival. The group time delay difference of neighbouring frequencies in the lower VLF band is directly proportional to the distance of the source. Since the attenuation of VLF waves is smaller for west to east propagation and
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Resonant waves of this zeroth mode can be excited in the Earth–ionosphere waveguide cavity, mainly by the continuing current components of lightning flowing between two return strokes. Their wavelengths are integral fractions of the Earth's circumference, and their resonance frequencies can thus be
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T(ρ, f) depending mainly on distance ρ and frequency f. In the VLF range, only mode one is important at distances larger than about 1000 km. Least attenuation of this mode occurs at about 15 kHz. Therefore, the Earth–ionosphere waveguide behaves like a bandpass filter, selecting this band
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At distances greater than about 500 km, sky waves reflected several times at the ionosphere must be added. Therefore, mode theory is here more appropriate. The first mode is least attenuated within the Earth–ionosphere waveguide, and thus dominates at distances greater than about 1000 km.
409:. The maximum spectral amplitude of the sferic typically is near 5 kHz. Beyond this maximum, the spectral amplitude decreases as 1/f if the Earth's surface were perfectly conducting. The effect of the real ground is to attenuate the higher frequencies more strongly than the lower frequencies ( 364:
The visible part of a lightning channel has a typical length of about 5 km. Another part of comparable length may be hidden in the cloud and may have a significant horizontal branch. Evidently, the dominant wavelength of the electromagnetic waves of R- and K-strokes is much larger than their
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simulating the electric properties of the channel. At the moment of contact with the perfectly conducting Earth surface, the charge is lowered to the ground. In order to fulfill the boundary conditions at the top of the wire (zero electric current) and at the ground (zero electric voltage), only
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Both R-strokes as well as K-strokes produce sferics seen as a coherent impulse waveform within a broadband receiver tuned between 1–100 kHz. The electric field strength of the impulse increases to a maximum value within a few microseconds and then declines like a damped oscillator. The
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For the regional range (< 1,000 km), the usual way is magnetic direction finding as well as time of arrival measurements of a sferic signal observed simultaneously at several stations. Presumption of such measurements is the concentration on one individual impulse. If one measures
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The steady electric discharging currents in a lightning channel cause a series of incoherent impulses in the whole frequency range, the amplitudes of which decreases approximately with the inverse frequency. In the ELF-range, technical noise from 50 to 60 Hz, natural noise from the
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during the night, thunderstorm activity up to distances of about 10,000 km can be observed for signals arriving from the west during night time conditions. Otherwise, the transmission range is of the order of 5,000 km.
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When distances are less than about 500 km (depending on frequency), then ray theory is appropriate. The ground wave and the first hop (or sky) wave reflected at the ionospheric D layer interfere with each other.
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at only a few stations around the world can monitor the global lightning activity fairly well. One can apply the dispersive property of the Earth–ionosphere waveguide by measuring the
81:, and can be received thousands of kilometres from their source. On a time-domain plot, a sferic may appear as a single high-amplitude spike in the time-domain data. On a 365:
channel lengths. The physics of electromagnetic wave propagation within the channel must thus be derived from full wave theory, because the ray concept breaks down.
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The channel of a R stroke can be considered as a thin isolated wire of length L and diameter d in which negative electric charge has been stored. In terms of
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located mainly in the continental areas at low and middle latitudes. In order to monitor the thunderstorm activity, sferics are the appropriate means.
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Lin, Y.T.; et al. (1979). "Characterization of lightning return stroke electric and magnetic fields from simultaneous two-station measurements".
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The atmospheric noise depends on frequency, location and time of day and year. Worldwide measurements of that noise are documented in CCIR-reports.
164:, that occur at mesospheric altitudes, are short-lived electric breakdown phenomena, probably generated by giant lightning events on the ground. 1182: 386: 253:
in the upper part of the channel and an equivalent amount of negative charge in its lower part neutralize within a typical time interval of
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simultaneously several pulses, interference takes place with a beat frequency equal to the inversal average sequence time of the pulses.
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for K-strokes. Often, a continuing current component flows between successive R-strokes. Its "pulse" time typically varies between about
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Spaulding, A. D. (1995). "Atmospheric noise and its effects on telecommunication system performance". In Volland, H. (ed.).
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Weidman, C.D.; Krider, E. P. (1979). "The radiation field wave forms produced by intracloud lightning discharge processes".
1167: 579: 157: 141: 85:, a sferic appears as a vertical stripe (reflecting its broadband and impulsive nature) that may extend from a few 123:
signal. Because the source of the whistler is an impulse (i.e., the sferic), a whistler may be interpreted as the
1172: 1134: 429: 153: 66: 428:. In the case of the ionospheric D-layer, it depends, in addition, on time of day, season, latitude, and the 417: 776:
Volland, H. (1995), "Longwave sferics propagation within the atmospheric waveguide", in Volland, H. (ed.),
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Serhan, G. L.; et al. (1980), "The RF spectra of first and subsequent lightning return strokes in the
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orientation of the field strength increase depends on whether it is a negative or a positive discharge
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stored within the lightning channel is lowered to the ground within a typical impulse time interval of
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Proctor, D. E. (1995), "Radio noise above 300 kHz due to Natural Causes", in Volland, H. (ed.),
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In a typical cloud-to-ground stroke (R stroke), negative electric charge (electrons) of the order of
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The energy of K-strokes is in general two orders of magnitude weaker than the energy of R-strokes.
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is the speed of light). In typical intracloud K-strokes, positive electric charge of the order of
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Grandt, C. (1992), "Thunderstorm monitoring in South Africa and Europe by means of VLF sferics",
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The Earth–ionosphere waveguide is dispersive. Its propagation characteristics are described by a
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Sferics can be simulated approximately by the electromagnetic radiation field of a vertical
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is one of the most important sources for the limitation of the detection of radio signals.
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Orville, R. E. (1995), "Lightning detection from ground and space", in Volland, H. (ed.),
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Williams, E. R. (1995), "Meteorological aspects of thunderstorms", in Volland, H. (ed.),
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Harth, W. (1982), "Theory of low frequency wave propagation", in Volland, H. (ed.),
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The corresponding values for average electric current, frequency and wavelength are
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About 100 lightning strokes per second are generated all over the world excited by
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This corresponds to an average current flowing within the channel of the order of
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D- and E- layers. Whistlers generated by lightning strokes can propagate into the
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The typical length of lightning channels can be estimated to be of the order of
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Fraser-Smith, A. C. (1995), "Low-frequency radio noise", in Volland, H. (ed.),
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the speed of light). These resonant modes with their fundamental frequency of
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distance or greater have their frequencies slightly offset in time, producing
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discharges. Sferics may propagate from their lightning source without major
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Vonnegut, B. (1982), "The physics of thundercloudes", in Volland, H (ed.),
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When the electromagnetic energy from a sferic escapes the Earth-ionosphere
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Lewis, E. A. (1982), "High frequency radio noise", in Volland, H. (ed.),
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must clearly exceed the noise amplitude in order to become detectable.
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of the magnetosphere (for the conditions at that particular instant).
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Sentman, D. D. (1995), "Schumann resonances", in Volland, H. (ed.),
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http://www.srh.noaa.gov/oun/wxevents/19550525/stormelectricity.php
901:, vol. II, Boca Raton, Florida: CRC Press, pp. 133–202, 403: 86: 29: 1106:. Vol. I. Boca Raton, Florida: CRC Press. pp. 359–395. 1082:, vol. I, Boca Raton, Florida: CRC Press, pp. 297–310, 1058:, vol. I, Boca Raton, Florida: CRC Press, pp. 137–149, 952:, vol. I, Boca Raton, Florida: CRC Press, pp. 267–295, 925:, vol. I, Boca Raton, Florida: CRC Press, pp. 111–178, 684:, vol. I, Boca Raton, Florida: CRC Press, pp. 311–358, 723:, vol. II, Boca Raton, Florida: CRC Press, pp. 21–77, 708:, vol. II, Boca Raton, Florida: CRC Press, pp. 155–193 1000:, vol. I, Boca Raton, Florida: CRC Press, pp. 27–60, 606:(International Consultation Committee on Radio Communications). 976:, vol. I, Boca Raton, Florida: CRC Press, pp. 1–22, 921:
Polk, C. (1982), "Schumann resonances", in Volland, H. (ed.),
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R strokes emit most of their energy within the ELF/VLF range (
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to several tens of kHz, depending on atmospheric conditions.
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Maximum spectral energy is generated near frequencies of
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Hayakawa, M. (1995), "Whistlers", in Volland, H. (ed.),
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Comité Consultatif International des Radiocommunications
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impulse that occurs as a result of natural atmospheric
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Park, C. G. (1982), "Whistlers", in Volland, H (ed.),
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signals amidst a background of sferics as received at
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in a complicated manner. VLF propagation within the
436:can be described by ray theory and by wave theory. 398:Transfer function of Earth–ionosphere waveguide 538:determines the sensibility and sensitivity of 420:= extremely low frequencies, < 3 kHz; 502:Monitoring thunderstorm activity with sferics 8: 859: 857: 771: 769: 943: 941: 675: 673: 333:its electric current is of the order of 62:(sometimes also spelled "spheric") is a 1104:Handbook of Atmospheric Electrodynamics 1080:Handbook of Atmospheric Electrodynamics 1056:Handbook of Atmospheric Electrodynamics 998:Handbook of Atmospheric Electrodynamics 950:Handbook of Atmospheric Electrodynamics 778:Handbook of Atmospheric Electrodynamics 706:Handbook of Atmospheric Electrodynamics 682:Handbook of Atmospheric Electrodynamics 644: 642: 617: 591: 623: 621: 494: ≃ 7.5 Hz are known as 7: 1143:, G.Wiessala in RadioUser 1/2013, UK 653:, vol. I, Boca Raton, Florida: 542:systems (e.g., radio receivers). An 144:between the Earth's surface and the 567:1955 Great Plains tornado outbreak 25: 27:Broadband electromagnetic impulse 385:, where the charge is stored, a 340:corresponding to the numbers of 377:theory, one can adopt a simple 1: 1183:Severe weather and convection 974:CRC Handbook of Atmospherics 923:CRC Handbook of Atmospherics 899:CRC Handbook of Atmospherics 721:CRC Handbook of Atmospherics 651:CRC Handbook of Atmospherics 456:approximately determined by 92:Sferics received from about 866:Atmospheric Electrodynamics 158:upper-atmospheric lightning 34:A frequency vs. time plot ( 1199: 1135:Radio in Space and Time - 434:Earth–ionosphere waveguide 142:Earth-ionosphere waveguide 79:Earth–ionosphere waveguide 156:lines of force. Finally, 578:track using sferics and 369:Electric channel current 56:radio atmospheric signal 1158:Atmospheric electricity 881:Wave Propagation Theory 848:10.1029/JC084iC06p03159 813:10.1029/JC084iC10p06307 761:10.1029/RS015i006p01089 630:The Lightning Discharge 483:the Earth's radius and 471:) ≃ 7.5  389:of the channel, and an 173:Basic stroke parameters 51: 536:signal-to-noise ratio 225:or at wavelengths of 33: 1168:Electrical phenomena 879:Wait, J. R. (1982), 864:Volland, H. (1984), 657:, pp. 251–288, 628:Uman, M. A. (1980), 1034:1992JGR....9718215G 840:1979JGR....84.3159W 805:1979JGR....84.6307L 515:Schumann resonances 496:Schumann resonances 50:on August 24, 2005. 868:, Berlin: Springer 306:for R-strokes and 115:by the near-Earth 52: 38:) showing several 1137:Whistler, Sferics 1042:10.1029/92JD01623 548:Atmospheric noise 540:telecommunication 530:Atmospheric noise 449:transfer function 430:geomagnetic field 413:'s ground wave). 379:transmission line 168:Source properties 94:2,000 kilometres' 18:Radio atmospheric 16:(Redirected from 1190: 1173:Electromagnetism 1118: 1117: 1099: 1093: 1092: 1075: 1069: 1068: 1051: 1045: 1044: 1022:J. Geophys. Res. 1017: 1011: 1010: 993: 987: 986: 969: 963: 962: 945: 936: 935: 918: 912: 911: 894: 888: 887: 876: 870: 869: 861: 852: 851: 823: 817: 816: 788: 782: 781: 773: 764: 763: 746: 740: 734: 733: 716: 710: 709: 701: 695: 694: 677: 668: 667: 646: 637: 636: 625: 607: 596: 513:Measurements of 375:electric circuit 359: 357: 352: 350: 346: 344: 339: 337: 332: 328: 326: 324: 322: 321: 318: 315: 305: 303: 301: 299: 298: 295: 292: 279: 277: 272: 270: 266: 264: 259: 257: 252: 250: 245: 241: 239: 237: 236: 232: 224: 222: 220: 219: 215: 207: 205: 203: 202: 198: 190: 188: 183: 181: 125:impulse response 95: 21: 1198: 1197: 1193: 1192: 1191: 1189: 1188: 1187: 1148: 1147: 1126: 1121: 1114: 1101: 1100: 1096: 1090: 1077: 1076: 1072: 1066: 1053: 1052: 1048: 1019: 1018: 1014: 1008: 995: 994: 990: 984: 971: 970: 966: 960: 947: 946: 939: 933: 920: 919: 915: 909: 896: 895: 891: 878: 877: 873: 863: 862: 855: 828:J. Geophys. Res 825: 824: 820: 793:J. Geophys. Res 790: 789: 785: 775: 774: 767: 744: 742: 741: 737: 731: 718: 717: 713: 703: 702: 698: 692: 679: 678: 671: 665: 648: 647: 640: 627: 626: 619: 615: 610: 597: 593: 589: 563: 532: 504: 493: 475: Hz (with 461: 400: 371: 355: 354: 348: 347: 342: 341: 335: 334: 330: 319: 316: 313: 312: 310: 308: 307: 296: 293: 290: 289: 287: 285: 284: 275: 274: 268: 267: 262: 261: 255: 254: 248: 247: 243: 234: 230: 229: 227: 226: 217: 213: 212: 210: 209: 200: 196: 195: 193: 192: 186: 185: 179: 178: 175: 170: 133: 107:and enters the 93: 67:electromagnetic 28: 23: 22: 15: 12: 11: 5: 1196: 1194: 1186: 1185: 1180: 1175: 1170: 1165: 1160: 1150: 1149: 1146: 1145: 1132: 1125: 1124:External links 1122: 1120: 1119: 1112: 1094: 1088: 1070: 1064: 1046: 1028:(D16): 18215, 1012: 1006: 988: 982: 964: 958: 937: 931: 913: 907: 889: 885:Pergamon Press 871: 853: 818: 783: 765: 735: 729: 711: 696: 690: 669: 663: 638: 634:Academic Press 616: 614: 611: 609: 608: 590: 588: 585: 584: 583: 582:as an overture 569: 562: 559: 531: 528: 519:group velocity 503: 500: 491: 459: 407:dipole antenna 399: 396: 370: 367: 174: 171: 169: 166: 132: 129: 44:Palmer Station 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 1195: 1184: 1181: 1179: 1178:Space plasmas 1176: 1174: 1171: 1169: 1166: 1164: 1161: 1159: 1156: 1155: 1153: 1144: 1142: 1138: 1133: 1131: 1128: 1127: 1123: 1115: 1113:9780849386473 1109: 1105: 1098: 1095: 1091: 1089:9780849386473 1085: 1081: 1074: 1071: 1067: 1065:9780849386473 1061: 1057: 1050: 1047: 1043: 1039: 1035: 1031: 1027: 1023: 1016: 1013: 1009: 1007:9780849386473 1003: 999: 992: 989: 985: 983:9780849332265 979: 975: 968: 965: 961: 959:9780849386473 955: 951: 944: 942: 938: 934: 932:9780849332265 928: 924: 917: 914: 910: 904: 900: 893: 890: 886: 882: 875: 872: 867: 860: 858: 854: 849: 845: 841: 837: 833: 829: 822: 819: 814: 810: 806: 802: 799:(C10): 6307. 798: 794: 787: 784: 779: 772: 770: 766: 762: 758: 754: 750: 749:Radio Science 739: 736: 732: 726: 722: 715: 712: 707: 700: 697: 693: 691:9780849386473 687: 683: 676: 674: 670: 666: 664:9780849332265 660: 656: 652: 645: 643: 639: 635: 631: 624: 622: 618: 612: 605: 601: 595: 592: 586: 581: 577: 573: 570: 568: 565: 564: 560: 558: 555: 551: 549: 545: 544:analog signal 541: 537: 529: 527: 523: 520: 516: 511: 509: 508:thunderstorms 501: 499: 497: 490: 486: 482: 479:= 1, 2, ...; 478: 474: 470: 466: 463: ≃  462: 453: 450: 445: 441: 437: 435: 431: 427: 423: 419: 414: 412: 408: 405: 397: 395: 392: 388: 384: 381:model with a 380: 376: 368: 366: 362: 281: 172: 167: 165: 163: 159: 155: 151: 150:magnetosphere 147: 143: 138: 130: 128: 126: 122: 118: 114: 111:, it becomes 110: 109:magnetosphere 106: 101: 99: 90: 88: 84: 80: 76: 72: 68: 65: 61: 57: 49: 45: 41: 37: 32: 19: 1140: 1136: 1103: 1097: 1079: 1073: 1055: 1049: 1025: 1021: 1015: 997: 991: 973: 967: 949: 922: 916: 898: 892: 883:, New York: 880: 874: 865: 834:(C6): 3159. 831: 827: 821: 796: 792: 786: 777: 752: 748: 738: 720: 714: 705: 699: 681: 650: 632:, New York: 629: 603: 599: 598:The acronym 594: 556: 552: 533: 524: 512: 505: 488: 484: 480: 476: 472: 468: 464: 457: 454: 446: 442: 438: 415: 401: 372: 363: 282: 176: 134: 131:Introduction 119:, forming a 102: 97: 91: 59: 55: 53: 602:stands for 580:dawn chorus 572:Cluster One 331:10–150 ms , 154:geomagnetic 146:ionospheric 83:spectrogram 75:attenuation 36:spectrogram 1152:Categories 908:0849332273 745:ℓ ≈ 100 km 730:0849332273 613:References 576:Pink Floyd 411:Sommerfeld 391:inductance 387:resistance 152:along the 48:Antarctica 1163:Lightning 655:CRC Press 587:Footnotes 426:orography 383:capacitor 358:3–40 Mm . 137:lightning 113:dispersed 105:waveguide 71:lightning 64:broadband 747:range", 561:See also 404:Hertzian 351:7–100 Hz 345:1–20 C , 278:7.5 km . 271:40 kHz , 223:10 kHz , 189:100 μs . 121:whistler 40:whistler 1030:Bibcode 836:Bibcode 801:Bibcode 755:(108), 338:100 A , 323:⁠ 311:⁠ 300:⁠ 288:⁠ 265:400 A , 258:25 μs . 242:(where 233:⁄ 216:⁄ 206:10 kA . 199:⁄ 162:sprites 77:in the 1141:Tweeks 1110:  1086:  1062:  1004:  980:  956:  929:  905:  727:  688:  661:  117:plasma 98:tweeks 60:sferic 251:10 mC 240:30 km 1139:and 1108:ISBN 1084:ISBN 1060:ISBN 1002:ISBN 978:ISBN 954:ISBN 927:ISBN 903:ISBN 725:ISBN 686:ISBN 659:ISBN 600:CCIR 574:, a 534:The 467:/(2π 353:and 327:4 km 309:ℓ ≈ 304:8 km 286:ℓ ≈ 273:and 228:λ = 211:f ≈ 194:J ≈ 1038:doi 844:doi 809:doi 757:doi 422:VLF 418:ELF 356:λ ≈ 349:f ≈ 343:Q ≈ 336:J ≈ 325:λ = 302:λ = 276:λ ≈ 269:f ≈ 263:J ≈ 256:τ ≈ 249:Q ≈ 187:τ = 182:1 C 180:Q ≈ 160:or 87:kHz 58:or 1154:: 1036:, 1026:97 1024:, 940:^ 856:^ 842:. 832:84 830:. 807:. 797:84 795:. 768:^ 753:15 751:, 672:^ 641:^ 620:^ 498:. 465:mc 135:A 100:. 54:A 46:, 1116:. 1040:: 1032:: 850:. 846:: 838:: 815:. 811:: 803:: 759:: 492:1 489:f 485:c 481:a 477:m 473:m 469:a 460:m 458:f 320:2 317:/ 314:1 297:4 294:/ 291:1 244:c 238:≈ 235:f 231:c 221:= 218:τ 214:1 204:= 201:τ 197:Q 20:)

Index

Radio atmospheric

spectrogram
whistler
Palmer Station
Antarctica
broadband
electromagnetic
lightning
attenuation
Earth–ionosphere waveguide
spectrogram
kHz
waveguide
magnetosphere
dispersed
plasma
whistler
impulse response
lightning
Earth-ionosphere waveguide
ionospheric
magnetosphere
geomagnetic
upper-atmospheric lightning
sprites
electric circuit
transmission line
capacitor
resistance

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