標(biāo)題: Titlebook: ELF-VLF Radio Wave Propagation; Proceedings of the N Jan A. Holtet Conference proceedings 1974 Springer Science+Business Media Dordrecht 19 [打印本頁(yè)] 作者: 大破壞 時(shí)間: 2025-3-21 18:11
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation影響因子(影響力)
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation被引頻次
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation被引頻次學(xué)科排名
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation年度引用
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation年度引用學(xué)科排名
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation讀者反饋
書(shū)目名稱(chēng)ELF-VLF Radio Wave Propagation讀者反饋學(xué)科排名
作者: 背書(shū) 時(shí)間: 2025-3-21 20:14
Nazi Massacres and Divided Memory,y processes that takes place in the lower thermosphere since some species, which are produced in the lower thermosphere, are brought into the mesosphere by eddy diffusion. It is therefore convenient to include heights up to 110–100 km when photochemical processes in the mesosphere are considered. In作者: 放逐某人 時(shí)間: 2025-3-22 03:34
Random Sequence Model for Nonlinear Systemsd magnetospheric sources. Variations in the energy input to the earth’s atmosphere from these sources have been observed for nearly a half-century by means of a variety of ground based measurements including VLF (3–30 kHz) radio transmissions (e.g. Espenshied 1926; Lauter 1950, 1961; Bracewell et al作者: Benzodiazepines 時(shí)間: 2025-3-22 08:37 作者: instructive 時(shí)間: 2025-3-22 09:56
F. J. van Spronsen,A. Bélanger-Quintanaticles within the Earth1s atmosphere. This plasma component of the air is essential for the conversion of kinetic energy of the gas into electromagnetic energy. Electromagnetic energy can be transported within the various height regions and ultimately will be dissipated through Ohm losses. Thus, the作者: 空氣傳播 時(shí)間: 2025-3-22 13:05
https://doi.org/10.1007/978-3-642-24936-5adio propagation in the ionosphere. The method differed from other approaches (see, for example, Budden, 1955a, b; Barron and Budden, 1959; Barron 1961; Johler and Harper, 1962; Keller and Keller, 1962; Price, 1964; Inoue and Horowitz, 1966) in its choice of the two solutions which correspond to wav作者: 空氣傳播 時(shí)間: 2025-3-22 20:22 作者: Mangle 時(shí)間: 2025-3-22 23:31 作者: FRAUD 時(shí)間: 2025-3-23 03:41 作者: 青春期 時(shí)間: 2025-3-23 07:41 作者: 到婚嫁年齡 時(shí)間: 2025-3-23 10:04 作者: NEX 時(shí)間: 2025-3-23 16:08 作者: 審問(wèn),審訊 時(shí)間: 2025-3-23 19:38 作者: 生命 時(shí)間: 2025-3-23 22:25
https://doi.org/10.1007/978-3-642-28096-2The phenomenon of “cross-over” is important in the theory of ion cyclotron whistlers observed in satellites (Barrington et al 1966). It is studied here for radio waves vertically incident on the ionosphere, when the earth’s magnetic field is nearly vertical, and when the wave frequency is less than the gyrofrequency for protons.作者: Root494 時(shí)間: 2025-3-24 02:33 作者: 起草 時(shí)間: 2025-3-24 06:39
,Spezielle Weierstra?sche Sigma-Funktionen,In VLF model computations the influence of ground conductivity is often neglected. There are several reasons why this procedure may seem justified:作者: 太空 時(shí)間: 2025-3-24 13:26 作者: outer-ear 時(shí)間: 2025-3-24 16:27 作者: 黑豹 時(shí)間: 2025-3-24 22:59
The Coalescence of Coupling Points and “Cross-Over” for Ion Cyclotron WhistlersThe phenomenon of “cross-over” is important in the theory of ion cyclotron whistlers observed in satellites (Barrington et al 1966). It is studied here for radio waves vertically incident on the ionosphere, when the earth’s magnetic field is nearly vertical, and when the wave frequency is less than the gyrofrequency for protons.作者: HOWL 時(shí)間: 2025-3-25 03:09
A Numerical Method for the Integration of the Equations Governing the Propagation of E.M. Waves in aThe behaviour of the horizontal components of the fields of E.M. waves in an horizontally stratified magneto- ionic medium depends on the Clemmow and Heading (C.H.) vectorial equation ?? . where . in a four dimensional basis system and where T is the propagation matrix.作者: Favorable 時(shí)間: 2025-3-25 04:01
The Effect of Ground Conductivity on VLF PropagationIn VLF model computations the influence of ground conductivity is often neglected. There are several reasons why this procedure may seem justified:作者: 眼界 時(shí)間: 2025-3-25 10:37 作者: 磨碎 時(shí)間: 2025-3-25 13:50 作者: Decongestant 時(shí)間: 2025-3-25 18:43
978-94-010-2267-5Springer Science+Business Media Dordrecht 1974作者: Camouflage 時(shí)間: 2025-3-25 23:11 作者: obnoxious 時(shí)間: 2025-3-26 01:55
https://doi.org/10.1007/978-3-662-32877-4ling from a given set of VLF radiowave propagation parameters. A typical D-region electron density profile is exairdned in detail and the height resolution and accuracy obtainable from the amount of observational data used in constructing the profile is determined.作者: 財(cái)產(chǎn) 時(shí)間: 2025-3-26 08:19
The Application of Inversion Techniques to Determine the Accuracy and Resolution of Electron Densityling from a given set of VLF radiowave propagation parameters. A typical D-region electron density profile is exairdned in detail and the height resolution and accuracy obtainable from the amount of observational data used in constructing the profile is determined.作者: 靦腆 時(shí)間: 2025-3-26 11:47 作者: LIMIT 時(shí)間: 2025-3-26 14:35
Random Sequence Model for Nonlinear Systems 1973; and Banks and Kockarts 1973). All these studies point out the difficulty in providing a definitive description of the sources of the lower ionosphere, because the atmospheric constituents, chemistry, and energy inputs have yet to be completely identified and accurately measured.作者: 詼諧 時(shí)間: 2025-3-26 17:21
Ionizing Radiation Affecting the Lower Ionosphere 1973; and Banks and Kockarts 1973). All these studies point out the difficulty in providing a definitive description of the sources of the lower ionosphere, because the atmospheric constituents, chemistry, and energy inputs have yet to be completely identified and accurately measured.作者: Left-Atrium 時(shí)間: 2025-3-27 00:19
Coupling Between the Neutral and the Ionized Atmosphere plasma serves as a medium to redistribute the external heat input into the atmosphere. The electromagnetic coupling between plasma and the neutral air within lower atmosphere, ionosphere and magnetosphere will be discussed.作者: 縫紉 時(shí)間: 2025-3-27 01:38
Fortran Program for Obtaining Wavefields of Penetrating, Nonpenetrating, and Whistler Modes of Radioes incident onto the ionosphere from below, with polarizations chosen to give the greatest and the least penetration at great heights. These two solutions are called the penetrating and nonpenetrating modes, respectively.作者: 使成波狀 時(shí)間: 2025-3-27 08:49 作者: Stricture 時(shí)間: 2025-3-27 13:28
VLF Phase Perturbations Associated with Geomagnetic Activityng paths to the east and west limited the analysis to a determination of the equatorward extent. All events occurred during nighttime conditions over the North American continent, and under a wide range of geomagnetic disturbance.作者: deviate 時(shí)間: 2025-3-27 13:47
Lower Ionosphere Ion Chemistrytion may be significant during disturbed conditions such as a PCA or auroral absorption event. Cole and Pierce (1965) found that the dominant influence changes from electrons above to ions below at about 50 km altitude.作者: 季雨 時(shí)間: 2025-3-27 18:21
Theory of the Terrestrial Propagation of VLF Electromagnetic Waveshe principal reason being that the attenuation of the waves is very low and the phase stability of the waves is very high. Thus, these waves find numerous applications in global communications and in long-range navigation systems.作者: 同謀 時(shí)間: 2025-3-27 22:19
The Use of VLF Propagation Results in Ionospheric Modellingograms written to implement this work. However in practice one is faced with the problem of determining the field at a point situated a given distance from a transmitter of known frequency, and it may not be immediately obvious how to apply full-wave theory in this situation.作者: Creatinine-Test 時(shí)間: 2025-3-28 02:05
F. J. van Spronsen,A. Bélanger-Quintana plasma serves as a medium to redistribute the external heat input into the atmosphere. The electromagnetic coupling between plasma and the neutral air within lower atmosphere, ionosphere and magnetosphere will be discussed.作者: 沉積物 時(shí)間: 2025-3-28 07:35 作者: 釘牢 時(shí)間: 2025-3-28 11:34 作者: 高原 時(shí)間: 2025-3-28 17:53 作者: plasma 時(shí)間: 2025-3-28 20:59 作者: 用手捏 時(shí)間: 2025-3-29 02:12
LCM Laboratorio de la Ciudad de Mexico,tion may be significant during disturbed conditions such as a PCA or auroral absorption event. Cole and Pierce (1965) found that the dominant influence changes from electrons above to ions below at about 50 km altitude.作者: 標(biāo)準(zhǔn) 時(shí)間: 2025-3-29 03:27
he principal reason being that the attenuation of the waves is very low and the phase stability of the waves is very high. Thus, these waves find numerous applications in global communications and in long-range navigation systems.作者: 警告 時(shí)間: 2025-3-29 09:18 作者: Juvenile 時(shí)間: 2025-3-29 15:03
The Photochemistry of the Mesospherer ions in the D-region. If we therefore know the abundance of these species, their diurnal and seasonal variations, and also possible variations with the solar cycle, we might be able to explain some of the discrepancies which are obtained in measurements performed under different atmospheric condit作者: Capitulate 時(shí)間: 2025-3-29 17:03
Theory of Energy Flux and Polarisation Changes of a Radio Wave with Two Magnetoionic Components Undee is reduced. This is called ‘self-demodulation’, and is the main subject of this discussion. If the power of the disturbing wave is very large, ‘self-demodulation’ is accompanied by ‘self-distortion’ effects because of the large change in collision frequency distorting the original wave form of the作者: 膽小懦夫 時(shí)間: 2025-3-29 20:34 作者: 神化怪物 時(shí)間: 2025-3-30 02:01 作者: PALSY 時(shí)間: 2025-3-30 04:52
Nazi Massacres and Divided Memory,r ions in the D-region. If we therefore know the abundance of these species, their diurnal and seasonal variations, and also possible variations with the solar cycle, we might be able to explain some of the discrepancies which are obtained in measurements performed under different atmospheric condit作者: condemn 時(shí)間: 2025-3-30 11:56
R. Cheung,D. O. Sillence,M. C. Tchane is reduced. This is called ‘self-demodulation’, and is the main subject of this discussion. If the power of the disturbing wave is very large, ‘self-demodulation’ is accompanied by ‘self-distortion’ effects because of the large change in collision frequency distorting the original wave form of the作者: Basal-Ganglia 時(shí)間: 2025-3-30 13:27
The Photochemistry of the Mesospherey processes that takes place in the lower thermosphere since some species, which are produced in the lower thermosphere, are brought into the mesosphere by eddy diffusion. It is therefore convenient to include heights up to 110–100 km when photochemical processes in the mesosphere are considered. In作者: 該得 時(shí)間: 2025-3-30 16:59
Ionizing Radiation Affecting the Lower Ionosphered magnetospheric sources. Variations in the energy input to the earth’s atmosphere from these sources have been observed for nearly a half-century by means of a variety of ground based measurements including VLF (3–30 kHz) radio transmissions (e.g. Espenshied 1926; Lauter 1950, 1961; Bracewell et al作者: ALIEN 時(shí)間: 2025-3-30 22:23
Lower Ionosphere Ion Chemistryquency, during undisturbed conditions. However, according to Crain and Booker (1964) and Thomas (1969) the effects of ions on VLF and ELF wave propagation may be significant during disturbed conditions such as a PCA or auroral absorption event. Cole and Pierce (1965) found that the dominant influenc作者: 孤僻 時(shí)間: 2025-3-31 04:33
Coupling Between the Neutral and the Ionized Atmosphereticles within the Earth1s atmosphere. This plasma component of the air is essential for the conversion of kinetic energy of the gas into electromagnetic energy. Electromagnetic energy can be transported within the various height regions and ultimately will be dissipated through Ohm losses. Thus, the
