標題: Titlebook: Cosmic Plasma Physics; Proceedings of the C Karl Schindler Conference proceedings 1972 Plenum Press, New York 1972 Plasma.electron.fields.i [打印本頁] 作者: 營養(yǎng)品 時間: 2025-3-21 20:03
書目名稱Cosmic Plasma Physics影響因子(影響力)
作者: maroon 時間: 2025-3-21 23:35
Parametric Instabilities Generated in the Ionosphere by Intense Radio Wavesy. The energy content of 100 cubic kilometers of ionospheric plasma is of the order of 10 megawatt-secs. This estimate, coupled with an electron-ion temperature relaxation time ~ 10 secs, suggests the H. F. frequency transmitters in the megawatt power range can significantly alter the ionosphere pro作者: FOLLY 時間: 2025-3-22 00:50
Study of a Jovian Plasmasphere and the Occurrence of Jupiter Radioburstsuence of Io on the emission of the radiobursts. Duncan (1970) proposed that Io stimulates the emission when it crosses the “magnetopause” of Jupiter, Melrose (1967) suggested that the motion of Io through a “corotating region” inside the magnetosphere of Jupiter may be the cause.作者: 尋找 時間: 2025-3-22 07:01 作者: judicial 時間: 2025-3-22 12:32
Universal Instability Associated with the Plasmapause and Its Role in Geomagnetic Micropulsationse theory and laboratory experiments of a non-homogeneous magnetoplasma. Drift waves excited at the plasmapause may be unstable in the direction of the electron drift and propagate eastwards nearly perpendicular to the magnetic field. The drift waves, however, tend to convert very soon to ion sound o作者: Texture 時間: 2025-3-22 14:26
Deformation and Striation of Barium Clouds in the Ionospherevoted to the theory of plasma clouds which are sufficiently large to dominate the Pederson conductivity on lines of force which pass through the cloud and sufficiently high so that K. = Ω./.. ? 1. Figure 1 shows the model.作者: Texture 時間: 2025-3-22 20:20
Thermal Energy Transport in the Solar Winds with the theory for collision-dominated heat transport in a fully ionized medium developed by Spitzer and H?rm [1953]. A short discussion of some recent models is included to illustrate the role of thermal conduction in the expansion. In addition, a brief description of the steady state solar wind作者: 非實體 時間: 2025-3-23 00:29
Influence of Neutral Interstellar Matter on the Expansion of the Solar Windially constant expansion velocity. This solution is derived from a hydrodynamical treatment of the coronal expansion that does not take into account any interaction of the solar wind plasma with neutral interstellar matter which enters the solar system. In that case the supersonic solar wind expands作者: Urea508 時間: 2025-3-23 02:26 作者: THROB 時間: 2025-3-23 06:11
Heating of the Solar Wind Ionsn influx of neutral hydrogen from the boundary of the heliospher’e. Photoionisation and charge exchange trans-form neutral hydrogen atoms into protons. The ionised hydrogen component near the Earth’s orbit is then double-peaked and unstable. The kinetic energy of the protons (originating from the ne作者: 發(fā)酵劑 時間: 2025-3-23 13:42
Spectral Anisotropy of Alfvén-Waves in the Solar Windte the microscale fluctuations in the solar wind for at least 50% of the time. This claim is disputed by other observers and it may have to be revised towards a weaker statement regarding the dominant occurrence of these waves.作者: Muscularis 時間: 2025-3-23 14:57
Evidence for Waves and/or Turbulence in the Vicinity of Shocks in Spacehalov et al., 1969, Chao, 1970, Lepping and Argentiero, 1971, and others). This was possible because more refined plasma and magnetic field data have been collected by various spacecraft during recent years. In the previous studies, plasma data were not complete enough, so that only the magnetic fie作者: 同謀 時間: 2025-3-23 20:22 作者: PALMY 時間: 2025-3-24 00:14 作者: 破譯 時間: 2025-3-24 02:51 作者: Capitulate 時間: 2025-3-24 07:34 作者: 惡意 時間: 2025-3-24 11:11 作者: Rinne-Test 時間: 2025-3-24 18:50 作者: Dislocation 時間: 2025-3-24 21:29
Comets in the Solar Windatmosphere of atomic hydrogen visible in the resonance line Lyman α 1216 ?; the probability for excitation of this line by the flux of solar Lyman α quanta is once every few minutes, at the solar distance in question.作者: CHIP 時間: 2025-3-25 00:35
Rodrigo Fuster,Guillermo Donosovided the electromagnetic energy can be absorbed. Normally, radio waves incident on the ionosphere are reflected. But, as Perkins and Kaw. have shown, the power densities needed to produce heating of the ionosphere are also sufficient to trigger parametric instabilities. which cause an anomalous ac resistivity.作者: 靈敏 時間: 2025-3-25 07:17
Introduction, Objectives, and Scope,ov et al (1961, 1962), Engel (1965), Andronov and Trakhtengerts (1964), and Lutomirskiand Sudan (1966), but the problem was treated in a slightly different way which is applicable to the physical situation.作者: 格子架 時間: 2025-3-25 08:42 作者: homeostasis 時間: 2025-3-25 13:30 作者: 相符 時間: 2025-3-25 19:38
Effect of a Large Amplitude Wave Packet and Second Order Resonance on the Stimulation of VLF Emissioov et al (1961, 1962), Engel (1965), Andronov and Trakhtengerts (1964), and Lutomirskiand Sudan (1966), but the problem was treated in a slightly different way which is applicable to the physical situation.作者: 牽連 時間: 2025-3-25 21:41 作者: 流浪 時間: 2025-3-26 02:52 作者: optional 時間: 2025-3-26 05:59 作者: Fallibility 時間: 2025-3-26 11:42 作者: 宇宙你 時間: 2025-3-26 12:41 作者: blister 時間: 2025-3-26 17:08
Wind Field Probabilistic Forecastingatmosphere of atomic hydrogen visible in the resonance line Lyman α 1216 ?; the probability for excitation of this line by the flux of solar Lyman α quanta is once every few minutes, at the solar distance in question.作者: Clumsy 時間: 2025-3-27 00:41
Why Focus on Reducing Women’s Imprisonment? all in trying to understand the motion of such a two-ion gas, let us use the simplest of all possible models, being fully aware of its shortcomings yet hoping that we might learn something from its, admittedly crude, quantitative and qualitative features.作者: etiquette 時間: 2025-3-27 05:11 作者: 不來 時間: 2025-3-27 06:35
Hydrogen — Helium Expansion from the Sun all in trying to understand the motion of such a two-ion gas, let us use the simplest of all possible models, being fully aware of its shortcomings yet hoping that we might learn something from its, admittedly crude, quantitative and qualitative features.作者: chisel 時間: 2025-3-27 12:40 作者: Dysarthria 時間: 2025-3-27 14:46 作者: 憤世嫉俗者 時間: 2025-3-27 19:16 作者: 過剩 時間: 2025-3-27 22:04 作者: 舊石器時代 時間: 2025-3-28 05:18
Rape Myths in the Criminal Justice Systemvoted to the theory of plasma clouds which are sufficiently large to dominate the Pederson conductivity on lines of force which pass through the cloud and sufficiently high so that K. = Ω./.. ? 1. Figure 1 shows the model.作者: 附錄 時間: 2025-3-28 07:04 作者: 災(zāi)禍 時間: 2025-3-28 13:56 作者: 和平 時間: 2025-3-28 15:02 作者: Excitotoxin 時間: 2025-3-28 21:40
Solar Radiation Probabilistic Forecastingtion. This behaviour is analyzed in terms of a Kelvin-Helmholtz instability developing in the tail itself, rather than in the comet head as proposed by Ioffe. Reasonable agreement is obtained with the “parallel” and “perpendicular” wavelengths of the observed features, the periods of wave motion and the growth rates.作者: Tdd526 時間: 2025-3-29 01:08
Introduction, Objectives, and Scope,incipal dissipation process for the energy coupled into the magnetosphere by the solar wind, and provide the energy source for geomagnetic storms. Many theories for the rapid dissipation phase, known as substorm breakup, have been advanced., but there remains the question of how the magnetosphere te作者: 細菌等 時間: 2025-3-29 03:45
Rodrigo Fuster,Guillermo Donosoy. The energy content of 100 cubic kilometers of ionospheric plasma is of the order of 10 megawatt-secs. This estimate, coupled with an electron-ion temperature relaxation time ~ 10 secs, suggests the H. F. frequency transmitters in the megawatt power range can significantly alter the ionosphere pro作者: 劇毒 時間: 2025-3-29 09:22
Water Quality: Trends and Challengesuence of Io on the emission of the radiobursts. Duncan (1970) proposed that Io stimulates the emission when it crosses the “magnetopause” of Jupiter, Melrose (1967) suggested that the motion of Io through a “corotating region” inside the magnetosphere of Jupiter may be the cause.作者: 聾子 時間: 2025-3-29 12:12
Introduction, Objectives, and Scope,needed. Following the work of Kennel and Petschek (1966) a background noise level was assumed in the model;then the effect of a whistler mode wave packet on the particles was studied, which can be compared to pitch angle diffusion. The concept is equivalent to that of the quasilinear theory by Veden作者: Nebulous 時間: 2025-3-29 19:15 作者: 縮短 時間: 2025-3-29 21:40
Rape Myths in the Criminal Justice Systemvoted to the theory of plasma clouds which are sufficiently large to dominate the Pederson conductivity on lines of force which pass through the cloud and sufficiently high so that K. = Ω./.. ? 1. Figure 1 shows the model.作者: alliance 時間: 2025-3-30 02:50 作者: interrogate 時間: 2025-3-30 07:27
Aviah Sarah Day,Angela Jenner,Ruth Weirially constant expansion velocity. This solution is derived from a hydrodynamical treatment of the coronal expansion that does not take into account any interaction of the solar wind plasma with neutral interstellar matter which enters the solar system. In that case the supersonic solar wind expands作者: Subdue 時間: 2025-3-30 08:39 作者: 無脊椎 時間: 2025-3-30 14:14 作者: 燈泡 時間: 2025-3-30 17:48 作者: 遠地點 時間: 2025-3-30 21:20
Elizabeth A. Stanko OBE,Katrin Hohlhalov et al., 1969, Chao, 1970, Lepping and Argentiero, 1971, and others). This was possible because more refined plasma and magnetic field data have been collected by various spacecraft during recent years. In the previous studies, plasma data were not complete enough, so that only the magnetic fie作者: Original 時間: 2025-3-31 02:12
Wind Field Probabilistic Forecastinglite-borne instruments in the UV down to approximately 900 ?. The most important discovery made during these observations was the existence of a huge atmosphere of atomic hydrogen visible in the resonance line Lyman α 1216 ?; the probability for excitation of this line by the flux of solar Lyman α q作者: 凝視 時間: 2025-3-31 08:57 作者: FOVEA 時間: 2025-3-31 10:32
Wind Field Probabilistic Forecastingverywhere. Attempts to increase the energy beyond this limit will only achieve additional ionization. Further, this ionization seems to be extremely efficient even if the electrons, which must cause most of the ionization, are initially cold.作者: 反省 時間: 2025-3-31 16:48 作者: covert 時間: 2025-3-31 17:39 作者: 輕快來事 時間: 2025-3-31 22:14
https://doi.org/10.1007/978-1-4615-6758-5Plasma; electron; fields; ion; magnetohydrodynamics; physics; plasma physics; radiation; society; structure作者: Osteoarthritis 時間: 2025-4-1 02:02
978-1-4615-6760-8Plenum Press, New York 1972作者: 打折 時間: 2025-4-1 09:32 作者: 含沙射影 時間: 2025-4-1 11:54
Deformation and Striation of Barium Clouds in the Ionospherevoted to the theory of plasma clouds which are sufficiently large to dominate the Pederson conductivity on lines of force which pass through the cloud and sufficiently high so that K. = Ω./.. ? 1. Figure 1 shows the model.
