標題: Titlebook: Wave Instabilities in Space Plasmas; Proceedings of a Sym Peter J. Palmadesso,Konstantinos Papadopoulos Conference proceedings 1979 D. Reid [打印本頁] 作者: CK828 時間: 2025-3-21 18:00
書目名稱Wave Instabilities in Space Plasmas影響因子(影響力)
書目名稱Wave Instabilities in Space Plasmas影響因子(影響力)學科排名
書目名稱Wave Instabilities in Space Plasmas網絡公開度
書目名稱Wave Instabilities in Space Plasmas網絡公開度學科排名
書目名稱Wave Instabilities in Space Plasmas被引頻次
書目名稱Wave Instabilities in Space Plasmas被引頻次學科排名
書目名稱Wave Instabilities in Space Plasmas年度引用
書目名稱Wave Instabilities in Space Plasmas年度引用學科排名
書目名稱Wave Instabilities in Space Plasmas讀者反饋
書目名稱Wave Instabilities in Space Plasmas讀者反饋學科排名
作者: 種子 時間: 2025-3-21 22:33
ELF and VLF Activity Associated with High Latitude Holepitation; (6)the electric field reversal; (7) the convective flow reversal; (8) the polar cap boundary. These observations are often well correlated with ELF and VLF activity, exhibiting enhancements in broadband auroral hiss, ELF noise and/or auroral kilometric radiation in the HLH region.作者: pantomime 時間: 2025-3-22 00:46 作者: flex336 時間: 2025-3-22 05:54
Quenching of Natural Cyclotron Instability by Large Amplitude Monochromatic Waves Propagating in an ) is studied. We show that the frequency range ΔF which is concerned by this effect is proportional to b., where b is The field intensity of the monochromatic wave. ΔF is also an increasing function of the transmitter frequency.作者: 信徒 時間: 2025-3-22 09:57 作者: Amorous 時間: 2025-3-22 16:46
Anomalous Transition from Buneman to Ion Sound Instabilityruptly terminated by the emergence of long wavelength modes, a substantial drop in electric field energy and resistivity, and the formation of electron tails. In two dimensions, heating then proceeds as for ion sound turbulence.作者: PURG 時間: 2025-3-22 18:08 作者: 致命 時間: 2025-3-23 01:17
Effects of Power Line Radiation into the Magnetosphere OGO-3 spectral data show evidence of enhanced chorus activity over centers of population and industry, indicating that PLR may play a significant role in the excitation of VLF whistler-mode noise and the associated precipitation of electrons. Sampled OGO-3 data showed chorus elements starting in mu作者: 不妥協 時間: 2025-3-23 02:05
ELF and VLF Activity Associated with High Latitude Hole) in the topside ionosphere are summarized and correlated with the following terms, specifically in relation to ELF and VLF activity: (1) distinction from the midlatitude light ion trough (LIT) in H., associated with the plasmapause; (2) a narrow, abrupt depletion in the concentrations of atomic ion作者: chandel 時間: 2025-3-23 05:39 作者: burnish 時間: 2025-3-23 10:09
Effects of Power Line Radiation into the Magnetosphere OGO-3 spectral data show evidence of enhanced chorus activity over centers of population and industry, indicating that PLR may play a significant role in the excitation of VLF whistler-mode noise and the associated precipitation of electrons. Sampled OGO-3 data showed chorus elements starting in mu作者: Intervention 時間: 2025-3-23 15:52 作者: 發(fā)芽 時間: 2025-3-23 20:30
Ariel 3 and 4 Studies of Power Line Harmonic RadiationR and associated emissions above the ionosphere and their frequency of occurrence as a function of location, intensity, storm-time, season and solar cycle..A particularly prominent zone of emission is obtained at VLF (3.2 kHz over N. America where frequent PLHR induced magnetospheric wave amplificat作者: prediabetes 時間: 2025-3-23 22:26
Chorus, Energetic Electrons and Magnetospheric Substormsorus, energetic (79 ± 23 keV) electron fluxes and pitch angle distributions and ambient magnetic fields obtained with OGO 5. It is found that chorus occurring within 15° of the magnetic equator (equatorial chorus) was detected during magnetospheric sub-storms and is closely related to enhanced, anis作者: 赦免 時間: 2025-3-24 05:19 作者: ascend 時間: 2025-3-24 09:14 作者: ANT 時間: 2025-3-24 14:45
Chorus, Energetic Electrons and Magnetospheric Substormsorus, energetic (79 ± 23 keV) electron fluxes and pitch angle distributions and ambient magnetic fields obtained with OGO 5. It is found that chorus occurring within 15° of the magnetic equator (equatorial chorus) was detected during magnetospheric sub-storms and is closely related to enhanced, anis作者: Lineage 時間: 2025-3-24 17:41
Some Theoretical Aspects of Electrostatic Double Layersnsidered. Then the time-independent double layer is discussed. The discussion deals with the potential drop, the thickness, and some necessary criteria for the existence and stability of the layer. As a complement to the study of the time-independent double layer a few remarks are also made upon the作者: duplicate 時間: 2025-3-24 21:21
Magnetospheric Multiharmonic Instabilitiesron harmonic waves in a plasma consisting of a hot electron component with a loss-cone type of free energy source and a cold electron component of presumably ionospheric origin. When T./T., the ratio of cold to hot electron temperature is small, the cold upper hybrid frequency controls the harmonic 作者: esthetician 時間: 2025-3-25 01:36 作者: 慷慨不好 時間: 2025-3-25 06:20 作者: 少量 時間: 2025-3-25 10:29 作者: urethritis 時間: 2025-3-25 13:15
Anomalous Transition from Buneman to Ion Sound Instabilityof evolution are in accordance with quasi-linear theories for the Buneman and ion sound instability, respectively. Large deviations from Maxwellian distributions and resonant wave-particle interactions occur, however, already in the “hydrodynamic” phase and have to be accounted for. This phase is ab作者: 聯想記憶 時間: 2025-3-25 17:40 作者: 僵硬 時間: 2025-3-25 21:09 作者: 用肘 時間: 2025-3-26 00:42 作者: 運動的我 時間: 2025-3-26 07:54 作者: 銼屑 時間: 2025-3-26 09:30
Nonlinear Whistler-Mode Interaction and Triggered Emissions in the Magnetosphere: A Reviewmong various nonlinear wave-wave and wave-particle interactions in the magnetosphere, the whistler-mode interaction appears to be one of the most exciting phenomena which have been observed in space plasmas but not in laboratory plasmas. The present review may be far from complete since much of the 作者: cognizant 時間: 2025-3-26 14:37
Siple Station Experiments on Wave-Particle Interactions in the Magnetosphereve growth and wave-wave interactions (WWI) in the magnetosphere. Three general classes of WWI (triggering, suppression, and entrainment) are identified and interpreted in terms of a model based on cyclotron resonance interaction. A new type of triggered emission, the ‘band-limited impulse’ (BLI), of作者: 真實的人 時間: 2025-3-26 19:30
Siple Station Experiments on Wave-Particle Interactions in the Magnetosphereve growth and wave-wave interactions (WWI) in the magnetosphere. Three general classes of WWI (triggering, suppression, and entrainment) are identified and interpreted in terms of a model based on cyclotron resonance interaction. A new type of triggered emission, the ‘band-limited impulse’ (BLI), of作者: Biomarker 時間: 2025-3-26 22:57
Non Linear Wave Particle Interaction Theory Applied to Siple Triggered Emissions Important aspects of the theory are underlined. Parameters for Siple triggered emissions are used and “quasi-static” generation regions are constructed. Siple results are found to fit the theory very well.作者: 旋轉一周 時間: 2025-3-27 02:49 作者: Anthem 時間: 2025-3-27 07:31
Quenching of Natural Cyclotron Instability by Large Amplitude Monochromatic Waves Propagating in an emissions over a frequency range Δf of the order of 50–;150 Hz below the transmitter frequency. We show that this effect can be interpreted by trapping, inside the monochromatic wave, of a certain amount of particles which were contributing to the generation of hiss in the equatorial region before 作者: FAST 時間: 2025-3-27 10:08
Quenching of Natural Cyclotron Instability by Large Amplitude Monochromatic Waves Propagating in an emissions over a frequency range Δf of the order of 50–;150 Hz below the transmitter frequency. We show that this effect can be interpreted by trapping, inside the monochromatic wave, of a certain amount of particles which were contributing to the generation of hiss in the equatorial region before 作者: Glycogen 時間: 2025-3-27 13:43
Some Theoretical Aspects of Electrostatic Double Layersa for the existence and stability of the layer. As a complement to the study of the time-independent double layer a few remarks are also made upon the time-dependent double layer. Finally the question of how double layers are formed and maintained is treated. Several possible formation mechanisms are considered.作者: GLUT 時間: 2025-3-27 19:31 作者: 無瑕疵 時間: 2025-3-27 23:00 作者: albuminuria 時間: 2025-3-28 03:20 作者: Devastate 時間: 2025-3-28 09:11 作者: 束以馬具 時間: 2025-3-28 14:07 作者: 樂章 時間: 2025-3-28 18:12
Nonlinear Whistler-Mode Interaction and Triggered Emissions in the Magnetosphere: A Reviewting phenomena which have been observed in space plasmas but not in laboratory plasmas. The present review may be far from complete since much of the research, both theoretical and experimental, is still in progress.作者: 的事物 時間: 2025-3-28 21:58
Nonlinear Whistler-Mode Interaction and Triggered Emissions in the Magnetosphere: A Reviewting phenomena which have been observed in space plasmas but not in laboratory plasmas. The present review may be far from complete since much of the research, both theoretical and experimental, is still in progress.作者: jocular 時間: 2025-3-29 01:51 作者: CULP 時間: 2025-3-29 04:22 作者: VEST 時間: 2025-3-29 08:32 作者: Meditate 時間: 2025-3-29 12:52
Laboratory Simulation of Ionospheric Double-LayersA mechanism for double-layer formation in partially- or fully-ionized plasmas is described, founded on beam-plasma interaction: rf growth along the beam excites a rectified, ponderomotive electric field, which in turn causes charge separation. Laboratory studies of the mechanism are described.作者: 北極熊 時間: 2025-3-29 17:04
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/w/image/1021195.jpg作者: 成績上升 時間: 2025-3-29 22:59 作者: 倔強不能 時間: 2025-3-30 00:28 作者: 使服水土 時間: 2025-3-30 05:21
Non Linear Wave Particle Interaction Theory Applied to Siple Triggered Emissions Important aspects of the theory are underlined. Parameters for Siple triggered emissions are used and “quasi-static” generation regions are constructed. Siple results are found to fit the theory very well.作者: 倒轉 時間: 2025-3-30 08:18 作者: 碎片 時間: 2025-3-30 12:40
Wave Instabilities in Space Plasmas978-94-009-9500-0Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 主講人 時間: 2025-3-30 19:19 作者: 財主 時間: 2025-3-30 23:27
n ihn.“ — Wo, verdammt, war mein Telefonbuch? In diesen Minuten beginnen die Tagesthemen! Anruf in Hamburg: Jürgen Schneider verhaftet, ich versuch’, noch eine Meldung zu machen, brauche aber eine zweite Quelle. — Ich hatte ja nur diese drei Worte. Es war wie im richtigen Leben: die zweite Informati作者: 身體萌芽 時間: 2025-3-31 04:47 作者: 名詞 時間: 2025-3-31 05:34
Ja. I. Likhter to enhance the clearance and expectoration of sputum and breathing training or exercises to improve the marked dyspnoe are widely used. Most clinicians do not realize that up to now many methods of physical therapy are lacking a scientific background..Using breathing exercise and intermittent posit作者: FLINT 時間: 2025-3-31 12:04
stungsbegriffe im Drehstromnetz systematisch zusammenzustellen. W?hrend die Definition der Wirkleistung keine Schwierigkeiten bereitet, lassen sich die Blind- und Scheinleistung weniger eindeutig festlegen. Geht man vom Zeitverlauf der Drehstromleistung p(t) aus, so kann man neben der Wirkleistung d作者: GLADE 時間: 2025-3-31 13:45 作者: gnarled 時間: 2025-3-31 21:08
C. T. Dum,R. Chodurag über diese Behandlungsmethode in der ?rzteschaft, zu einer Zunahme sowohl von Wartelistenpatienten als auch von Herztransplantationszentren, jedoch nicht der Organspenderzahlen. Dies wiederum verl?ngerte die Wartezeiten, verst?rkte die Nachfrage nach Ventrikelunterstützungssystemen und führte zu e作者: Antarctic 時間: 2025-3-31 22:46
C. Hanuise,M. Crochetder ersten Klassifikation einer linksventrikul?ren Ausflusstraktobstruktion von Lev [82] 1952, wurde diese 1958 von Noonan u. Nadas [108] verfeinert, und die Definition des hypoplastischen Linksherzsyndroms wurde eingeführt. Letzteres umfasst ein weites Spektrum angeborener Fehlbildungen, welche von作者: progestogen 時間: 2025-4-1 04:50
Hiroshi Matsumoto Di?tetik geht es so sehr darum, wirkliche Koch. anzuwenden. Sobald man den oft vorhandenen Widerwillen der betreffenden Patienten gegen die meisten Speisen überwunden hat, hat man schon halb gewonnen. In F?llen schwerer Magersucht ist es empfehlenswert, den Patienten für die ersten Wochen — falls d作者: largesse 時間: 2025-4-1 06:55 作者: expound 時間: 2025-4-1 10:49
David Nunnlogische Einzelleistungen: Die T?tigkeit der Leber oder des Darms, sondern auch die Gesamtleistung des K?rpers zu ver?ndern, zu f?rdern oder zu hemmen. Das w?re nicht m?glich, wenn nicht ein morphologischer Zusammenhang aller Teile des K?rpers bestünde. Der aber ist gew?hrleistet durch drei Gewebe, 作者: 抗體 時間: 2025-4-1 17:49
David Nunnngen selten, insgesamt betreffen sie aber mehr als 1% der Bev?lkerung. Für die genetische Beratung besitzen sie dreifache Bedeutung: Erstens ist es wichtig, eine betroffene Familie, ungeachtet der Seltenheit des Merkmals, korrekt zu beraten. Zweitens k?nnen Verwechselungen dieser seltenen, hoch risk作者: Dysarthria 時間: 2025-4-1 18:49 作者: Hallmark 時間: 2025-4-2 00:02
Nicole Cornilleau-Wehrlin,Roger Gendrinwort, die im Vergleich zur Prim?rantwort verst?rkt und beschleunigt ausf?llt. Diese Reaktion kann jedoch überschie?end verlaufen und gro?e Gewebssch?digungen hervorrufen (Hypersensibilit?t), wenn das Antigen in gro?en Mengen vorliegt oder wenn die immunologische Abwehrbereitschaft der zellul?ren und作者: 果仁 時間: 2025-4-2 04:29
B. T. Tsurutani,E. J. Smith,S. R. Church,R. M. Thorne,R. E. Holzer作者: 使殘廢 時間: 2025-4-2 09:08 作者: Myocarditis 時間: 2025-4-2 11:35
B. T. Tsurutani,E. J. Smith,S. R. Church,R. M. Thorne,R. E. Holzer作者: heirloom 時間: 2025-4-2 18:09
Effects of Power Line Radiation into the Magnetosphereeiver (150–1500 Hz; 200 orbits; 1966–67) detected PLR from both 50-Hz and 60-Hz systems with average intensities near 1.0 mγ; PLR intensities greater than 10 mγ were detected less than 10% of the time. Intensities were low in the midnight and dawn sector..Antarctic data from Eights (L = 3.9; 1963–65作者: detach 時間: 2025-4-2 22:07
Ariel 3 and 4 Studies of Power Line Harmonic Radiationf the waves to become entrapped in ducts. The dependence of signal intensity on storm-time is similarly attributed to duct formation and wave-trapping therein. One and two (or multi) hop emissions occur with about equal probability at 3.2 kHz; at 9.6 kHz one hop are predominant..There is evidence of作者: Intervention 時間: 2025-4-3 03:34 作者: 外科醫(yī)生 時間: 2025-4-3 06:05
Does ELF Chorus Show Evidence of Power Line Stimulation?or minima are then statistically significant (<2σ). Thus, we find no statistically significant correlation between longitude and chorus occurrence which implies that there is little or no evidence of PLR effects on chorus triggering.作者: artifice 時間: 2025-4-3 08:24
Ariel 3 and 4 Studies of Power Line Harmonic Radiationf the waves to become entrapped in ducts. The dependence of signal intensity on storm-time is similarly attributed to duct formation and wave-trapping therein. One and two (or multi) hop emissions occur with about equal probability at 3.2 kHz; at 9.6 kHz one hop are predominant..There is evidence of作者: 佛刊 時間: 2025-4-3 13:19
