標(biāo)題: Titlebook: Wave Propagation in the Ionosphere; Karl Rawer Book 1993 Springer Science+Business Media Dordrecht 1993 eigenvalue.electromagnetic wave.gr [打印本頁] 作者: expenditure 時(shí)間: 2025-3-21 17:04
書目名稱Wave Propagation in the Ionosphere影響因子(影響力)
書目名稱Wave Propagation in the Ionosphere影響因子(影響力)學(xué)科排名
書目名稱Wave Propagation in the Ionosphere網(wǎng)絡(luò)公開度
書目名稱Wave Propagation in the Ionosphere網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Wave Propagation in the Ionosphere被引頻次
書目名稱Wave Propagation in the Ionosphere被引頻次學(xué)科排名
書目名稱Wave Propagation in the Ionosphere年度引用
書目名稱Wave Propagation in the Ionosphere年度引用學(xué)科排名
書目名稱Wave Propagation in the Ionosphere讀者反饋
書目名稱Wave Propagation in the Ionosphere讀者反饋學(xué)科排名
作者: 收到 時(shí)間: 2025-3-21 21:24 作者: 象形文字 時(shí)間: 2025-3-22 00:49 作者: refine 時(shí)間: 2025-3-22 08:03
ospheric structure suchas sound and gravity waves are also considered..Warm plasma and the effects of ions are considered in the third part,which includes a discussion of sound-like waves in electron and ionplasmas. Nonlinear effects and instabilities are described in thefourth part.978-90-481-4069-5978-94-017-3665-7作者: audiologist 時(shí)間: 2025-3-22 12:12 作者: 蔑視 時(shí)間: 2025-3-22 14:21 作者: 賞錢 時(shí)間: 2025-3-22 20:42
https://doi.org/10.1007/978-94-017-3665-7eigenvalue; electromagnetic wave; gravity; ionosphere; numerical method作者: 一瞥 時(shí)間: 2025-3-22 21:54 作者: Cupping 時(shí)間: 2025-3-23 03:31 作者: Isolate 時(shí)間: 2025-3-23 08:59
Refraction of radio waves in a plasma. Simplest caseAstonishingly enough, the foundations of the theory of radio wave propagation in an ionospheric plasma were laid long before the existence of an ionosphere was known and even before the electron was discovered, not to speak of plasma theory as such.作者: Conclave 時(shí)間: 2025-3-23 13:19 作者: 證明無罪 時(shí)間: 2025-3-23 17:24 作者: oblique 時(shí)間: 2025-3-23 18:07 作者: 微粒 時(shí)間: 2025-3-23 23:17 作者: PLE 時(shí)間: 2025-3-24 04:15
Electromagnetic waves in a cold gyrotropic plasmaave in a magnetized plasma. With the information obtained in the last Chapter we are now in -a position to find out whether this notion is, at least, applicable under certain restrictive conditions. If so, these need to be specified.作者: Robust 時(shí)間: 2025-3-24 09:37
Propagation in the space between Earth and ionosphere (deka- and hektometer-waves)ortance, on the other hand, is mainly still due to the fact that it allows waves with frequencies in the HF-band and below to propagate from ground to ground over very large distances, and that it influences quite considerably the ground-to-space and space-to-ground propagation of radio waves of higher frequencies.作者: 不開心 時(shí)間: 2025-3-24 13:25
Propagation in the space between Earth and ionosphere (deka- and hektometer-waves)ortance, on the other hand, is mainly still due to the fact that it allows waves with frequencies in the HF-band and below to propagate from ground to ground over very large distances, and that it influences quite considerably the ground-to-space and space-to-ground propagation of radio waves of higher frequencies.作者: extrovert 時(shí)間: 2025-3-24 16:28
Propagation through the ionosphere the ultraviolet ranges. In fact, absorption sets the decisive limits to groundbased optical astronomy. The situation is quite different with radio waves. While strong absorption occurs only in certain frequency ranges and at certain hours (e.g. for LF and MF waves during daylight hours), the most important ionospheric effect is due to refraction.作者: anatomical 時(shí)間: 2025-3-24 20:12
Propagation through the ionosphere the ultraviolet ranges. In fact, absorption sets the decisive limits to groundbased optical astronomy. The situation is quite different with radio waves. While strong absorption occurs only in certain frequency ranges and at certain hours (e.g. for LF and MF waves during daylight hours), the most important ionospheric effect is due to refraction.作者: Ligament 時(shí)間: 2025-3-25 01:50
Collisional attenuationsion frequency”, ., which was not physically specified. In Equation (4.5) we have merely replaced the average particle acceleration by a formal tenir . instead of .. The conditions under which collisions influence the propagation of radio waves shall now be considered in more detail..作者: 黃瓜 時(shí)間: 2025-3-25 04:51
Kinetic theory of a Lorentz plasmaopagation has not been admitted in Chapters 1 to 12. This was justified by the fact that the individual contributions to the current density should compensate each other due to the isotropy of the thermal motions. Almost all phenomena observed with ground-based ionospheric sounding can indeed be explained satisfactorily by cold plasma theory.作者: 暴露他抗議 時(shí)間: 2025-3-25 10:43 作者: 內(nèi)行 時(shí)間: 2025-3-25 14:44
Kinetic theory of a Lorentz plasmaopagation has not been admitted in Chapters 1 to 12. This was justified by the fact that the individual contributions to the current density should compensate each other due to the isotropy of the thermal motions. Almost all phenomena observed with ground-based ionospheric sounding can indeed be explained satisfactorily by cold plasma theory.作者: 炸壞 時(shí)間: 2025-3-25 15:54 作者: 新字 時(shí)間: 2025-3-25 20:56 作者: Picks-Disease 時(shí)間: 2025-3-26 00:43 作者: 客觀 時(shí)間: 2025-3-26 07:41
Waves in a warm isotropic plasmaic variables, namely radius vector . and particle momentum .. In this notation, the acceleration term in Newton’s fundamental law is simply d./d.. If the force in Equations (14.1,2) derives from an electric . and a magnetic field ., one obtains作者: helper-T-cells 時(shí)間: 2025-3-26 12:17
Introductiond neutral particles which tend to restore electric neutrality. Since the probability of such reactions increases in the downward direction as does the air density, an ionized . is formed with at least one peak at an altitude which depends on this balance. Vertical transport of ionization may be quite important in this context.作者: 放氣 時(shí)間: 2025-3-26 16:13
Introductiond neutral particles which tend to restore electric neutrality. Since the probability of such reactions increases in the downward direction as does the air density, an ionized . is formed with at least one peak at an altitude which depends on this balance. Vertical transport of ionization may be quite important in this context.作者: immunity 時(shí)間: 2025-3-26 17:09
Echoes from a plasma layerl (wave-) optics is needed only under very special conditions, the most common of which are: total reflection at normal incidence, and coupling (when the parameter . approaches a coupling condition, . = ± .).作者: 情感脆弱 時(shí)間: 2025-3-26 22:33 作者: 類人猿 時(shí)間: 2025-3-27 04:18
Properties of a magnetized plasmafore a linear excitation produces a charge oscillation outside the plane of polarization of the primary field. Thus the secondary waves radiated by the individual electrons do not have the same polarization but another, usually elliptical.作者: Chauvinistic 時(shí)間: 2025-3-27 08:25 作者: FOVEA 時(shí)間: 2025-3-27 11:21
Propagation in the Earth-ionosphere waveguide (Kilometric and longer waves)hapter 2) only the steady state oscillation which was loss-less but phase-shifted. The consequence was that the medium behaved like a capacitor. In other words the medium could be described by a (real) dielectric constant with negligible conductivity.作者: Ejaculate 時(shí)間: 2025-3-27 16:47 作者: reperfusion 時(shí)間: 2025-3-27 19:40 作者: Crohns-disease 時(shí)間: 2025-3-27 23:49
Introductionization depends on the intensity of the incoming radiation and on the — normally complicated — chemical follow-up reactions between ions, electrons and neutral particles which tend to restore electric neutrality. Since the probability of such reactions increases in the downward direction as does the作者: 流眼淚 時(shí)間: 2025-3-28 02:11
Introductionization depends on the intensity of the incoming radiation and on the — normally complicated — chemical follow-up reactions between ions, electrons and neutral particles which tend to restore electric neutrality. Since the probability of such reactions increases in the downward direction as does the作者: Jargon 時(shí)間: 2025-3-28 08:22 作者: capsule 時(shí)間: 2025-3-28 12:26
Electromagnetic waves in a cold gyrotropic plasmaave in a magnetized plasma. With the information obtained in the last Chapter we are now in -a position to find out whether this notion is, at least, applicable under certain restrictive conditions. If so, these need to be specified.作者: LAY 時(shí)間: 2025-3-28 17:23
Properties of a magnetized plasmaere. It was soon found that the terrestrial magnetic field must be the source of this phenomenon. In fact, the oscillation of each individual electron excited by the electric field of the wave is disturbed by the magnetic field which exercises a force perpendicular to the motion of the charge. There作者: AXIOM 時(shí)間: 2025-3-28 20:22 作者: 明確 時(shí)間: 2025-3-28 23:24 作者: 正常 時(shí)間: 2025-3-29 06:46 作者: BAIL 時(shí)間: 2025-3-29 09:50 作者: 積云 時(shí)間: 2025-3-29 15:01 作者: 時(shí)間等 時(shí)間: 2025-3-29 16:45
Propagation in the space between Earth and ionosphere (deka- and hektometer-waves)ortance, on the other hand, is mainly still due to the fact that it allows waves with frequencies in the HF-band and below to propagate from ground to ground over very large distances, and that it influences quite considerably the ground-to-space and space-to-ground propagation of radio waves of hig作者: 懲罰 時(shí)間: 2025-3-29 20:58
Propagation through the ionosphere the ultraviolet ranges. In fact, absorption sets the decisive limits to groundbased optical astronomy. The situation is quite different with radio waves. While strong absorption occurs only in certain frequency ranges and at certain hours (e.g. for LF and MF waves during daylight hours), the most i作者: 清唱?jiǎng)?nbsp; 時(shí)間: 2025-3-30 01:20
Propagation in the Earth-ionosphere waveguide (Kilometric and longer waves)low, in the D-layer. Our considerations in Section 3.3 and Chapter 6 were for small . (= ./.) so that the collisional influence remained weak. The reflection mechanism was “refractive” because an electron made many oscillations before it was stopped by a collision. It was justified to consider (in C作者: ABYSS 時(shí)間: 2025-3-30 06:09
The real ionosphere: Irregularities and acoustic-gravity waves depending only on the vertical coordinate. This, however, is an oversimplification because the actual conditions in the terrestrial ionosphere are more involved. Since the ionosphere is under solar control, all ionospheric parameters vary with local time so that large-scale horizontal gradients exi作者: MOTTO 時(shí)間: 2025-3-30 09:04
Propagation through the ionosphere the ultraviolet ranges. In fact, absorption sets the decisive limits to groundbased optical astronomy. The situation is quite different with radio waves. While strong absorption occurs only in certain frequency ranges and at certain hours (e.g. for LF and MF waves during daylight hours), the most i作者: VOK 時(shí)間: 2025-3-30 14:03 作者: 文藝 時(shí)間: 2025-3-30 19:23 作者: Conscientious 時(shí)間: 2025-3-30 22:44
Collisional attenuationsion frequency”, ., which was not physically specified. In Equation (4.5) we have merely replaced the average particle acceleration by a formal tenir . instead of .. The conditions under which collisions influence the propagation of radio waves shall now be considered in more detail..作者: 變態(tài) 時(shí)間: 2025-3-31 03:38 作者: Glossy 時(shí)間: 2025-3-31 06:02
Kinetic theory of a Lorentz plasmaopagation has not been admitted in Chapters 1 to 12. This was justified by the fact that the individual contributions to the current density should compensate each other due to the isotropy of the thermal motions. Almost all phenomena observed with ground-based ionospheric sounding can indeed be exp作者: voluble 時(shí)間: 2025-3-31 11:29 作者: 哀悼 時(shí)間: 2025-3-31 16:15 作者: 稱贊 時(shí)間: 2025-3-31 19:37
The Boltzmann equation of a compressible plasma a sound basis for discussing a large variety of phenomena that cannot be understood in the framework of the “cold theory” considered in Part A. Some simplifications are, fortunately, permitted in many applications.作者: 江湖郎中 時(shí)間: 2025-3-31 22:08 作者: 抵消 時(shí)間: 2025-4-1 04:05
Waves in a warm isotropic plasmaic variables, namely radius vector . and particle momentum .. In this notation, the acceleration term in Newton’s fundamental law is simply d./d.. If the force in Equations (14.1,2) derives from an electric . and a magnetic field ., one obtains作者: 充氣女 時(shí)間: 2025-4-1 08:50 作者: Cytokines 時(shí)間: 2025-4-1 11:22
Book 1993 in four parts and the sequence of theseparts reflect the development of ionospheric and propagationalresearch in areas such as space research geophysics andcommunications..The first part of the book presents an outline of the theory ofelectromagnetic waves propagating in a cold electron plasma. For作者: Mitigate 時(shí)間: 2025-4-1 17:21 作者: JECT 時(shí)間: 2025-4-1 19:14
Propagation in structured mediao-electronic surfaces are concentric spheres around the centre of Earth. Horizontal gradients are not admitted in this zero order approach in which the radio waves propagate in the great circle plane connecting sender and receiver locations. Consequently, the normals to the iso-electronic surfaces lie in the same plane.作者: Matrimony 時(shí)間: 2025-4-2 00:37 作者: LAPSE 時(shí)間: 2025-4-2 04:30
Lernen lernened?chtnis“ erkl?ren. Lernmotivation kann auf unterschiedlichen Wegen erlangt werden. Der Begriff der ?Wissenschaft“ kann erkl?rt werden. M?glichkeiten zur Themenfindung zur Erstellung wissenschaftlicher Arbeiten sind bekannt.作者: Tdd526 時(shí)間: 2025-4-2 07:07
Molecular Docking Analysis: Interaction Studies of Natural Compounds with Human TG2 Protein, properties. In present study natural compound from different classes were subjected for screening ADME/T properties and molecular docking analysis to investigate their interaction modes with the potential TG2 target. The result revealed that Artobiloxanthone have the highest affinity to TG2 and the highest consistency of interaction model.作者: N斯巴達(dá)人 時(shí)間: 2025-4-2 14:42 作者: 蒸發(fā) 時(shí)間: 2025-4-2 18:52 作者: CURL 時(shí)間: 2025-4-2 21:01 作者: DEVIL 時(shí)間: 2025-4-3 03:09 作者: indoctrinate 時(shí)間: 2025-4-3 04:11 作者: Magisterial 時(shí)間: 2025-4-3 12:00
C. Julien,J. P. Pereira-Ramos,A. Momchilovse early observations, several different types of lipid transfer have been discerned: (1) lipid transfer mediated by soluble proteins; (2) lipid transfer due to vesicle budding from one membrane followed by fusion with a target membrane; and (3) lipid transfer that occurs spontaneously either by lip作者: 悅耳 時(shí)間: 2025-4-3 13:22
