標(biāo)題: Titlebook: Electromagnetic Coupling in the Polar Clefts and Caps; P. E. Sandholt,A. Egeland Book 1989 Kluwer Academic Publishers 1989 Ionosphere.Scal [打印本頁] 作者: 水平 時間: 2025-3-21 18:11
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps影響因子(影響力)
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps影響因子(影響力)學(xué)科排名
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps網(wǎng)絡(luò)公開度
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps被引頻次
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps被引頻次學(xué)科排名
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps年度引用
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps年度引用學(xué)科排名
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps讀者反饋
書目名稱Electromagnetic Coupling in the Polar Clefts and Caps讀者反饋學(xué)科排名
作者: 縮減了 時間: 2025-3-21 22:29 作者: integral 時間: 2025-3-22 02:28 作者: SAGE 時間: 2025-3-22 07:25
https://doi.org/10.1007/978-3-662-32923-8etically map are reviewed in light of two different polar rain models. In one model the field aligned solar wind electrons have direct entry to the magnetosphere in the distant tail where the field lines are assumed to be open. In the other, the polar rain is the potential-barrier-reflected electron作者: 熱情贊揚(yáng) 時間: 2025-3-22 11:09 作者: TRACE 時間: 2025-3-22 16:16 作者: TRACE 時間: 2025-3-22 18:15 作者: Tortuous 時間: 2025-3-23 00:50 作者: filicide 時間: 2025-3-23 05:10
Handbuch der chemischen Elementetter radar. The auroral images were recorded on video tape for later display as time lapse sequences. Reviewing the images as sequences allows the eye to discern subtle features which are not readily apparent in the individual frames. One such feature which is the subject of this study is the faint 作者: ANN 時間: 2025-3-23 07:57 作者: Self-Help-Group 時間: 2025-3-23 10:43 作者: 不斷的變動 時間: 2025-3-23 15:25 作者: 蒙太奇 時間: 2025-3-23 22:03 作者: 寬容 時間: 2025-3-24 02:04
Allgemeines über textile Fasernc 3–4 frequency range near magnetospheric cusp latitudes. Results presented show the dependence of Pc 3 occurrence at South Pole on solar wind speed and interplanetary magnetic field magnitude and direction. Although some evidence clearly supports the idea of an upstream wave source for high latitud作者: Neonatal 時間: 2025-3-24 04:26 作者: Plaque 時間: 2025-3-24 10:18
Ingeborg Fiala-Fürst,Steffen H?hneundary conditions for the more advanced dynamical models. Furthermore the empirical models may be used to test our physical models and concepts. With the vast amount of geophysical and solar data which is now available, a number of empirical models have appeared, but the different empirical models a作者: conference 時間: 2025-3-24 12:25
Handbuch der deutschen Parteiend ground magnetic perturbations. Sources of the field-aligned electric currents in the dayside polar cusp are most likely located within the boundary layers, both the frontside low latitude and the magnetotai1, where induction currents due to relative motion between the sheath plasma and the magneto作者: 揉雜 時間: 2025-3-24 18:42 作者: cutlery 時間: 2025-3-24 19:50
978-94-010-6929-8Kluwer Academic Publishers 1989作者: Flat-Feet 時間: 2025-3-25 01:23 作者: 難理解 時間: 2025-3-25 04:54 作者: Induction 時間: 2025-3-25 11:15 作者: 從容 時間: 2025-3-25 12:34
https://doi.org/10.1007/978-94-009-0979-3Ionosphere; Scale; Storm; magnetosphere; satellite; spheric; wind作者: Wallow 時間: 2025-3-25 16:51
Electromagnetic Coupling in the Polar Clefts and Caps作者: 奇怪 時間: 2025-3-25 20:06
Auroral Oval Configuration During the Quiet Condition,so-called “sun-aligned polar cap arcs” are the manifestation of the auroral oval arcs in the latitudinally expanded dawn or dusk part of the oval. The optical emission intensity and the energy flux of the oval are much weaker during the quiet time.作者: 毗鄰 時間: 2025-3-26 02:47
Ionospheric Convection in the Polar Cap as Seen by Optical Imaging,a which provided a measure of the ion drift velocities. Excellent agreement was found in this comparison, which shows that the airglow structures are non-uniformities in the ionosphere where the 6300? emissions are produced by recombination. The observation of the motion of these structures could pr作者: 或者發(fā)神韻 時間: 2025-3-26 08:16 作者: strdulate 時間: 2025-3-26 08:41 作者: 創(chuàng)作 時間: 2025-3-26 15:54
Electrodynamics of Auroral and Polar Cap Arcs at Very High Latitudes,s and field-aligned currents at very high latitudes. This information is combined with similar results obtained while the radar was at Chatanika, Alaska. Together these data can be used as a framework for a phenomenological understanding of auroral precipitation.作者: 不能平靜 時間: 2025-3-26 20:03 作者: 整頓 時間: 2025-3-26 23:37
Handbuch der chemischen Elementea which provided a measure of the ion drift velocities. Excellent agreement was found in this comparison, which shows that the airglow structures are non-uniformities in the ionosphere where the 6300? emissions are produced by recombination. The observation of the motion of these structures could pr作者: 新奇 時間: 2025-3-27 04:14
https://doi.org/10.1007/978-3-7091-7958-1d the IMF B. component prevails. The often observed spiky or transient magnetic field variations at cusp latitudes suggest a clear correlation with flux transfer events at the dayside magnetosphere or dynamic pressure changes of the magnetosheath flow.作者: 駭人 時間: 2025-3-27 06:24
Ingeborg Fiala-Fürst,Steffen H?hnets and demerits of the different averaging and normalization techniques into consideration. This is important to take into account when trying to understand the physics, which the empirical models represent.作者: 壕溝 時間: 2025-3-27 12:44
Handbuch der deutschen Parteiens and field-aligned currents at very high latitudes. This information is combined with similar results obtained while the radar was at Chatanika, Alaska. Together these data can be used as a framework for a phenomenological understanding of auroral precipitation.作者: 慢慢啃 時間: 2025-3-27 17:12 作者: Pathogen 時間: 2025-3-27 21:43 作者: 范圍廣 時間: 2025-3-27 22:25
Radioaktive Elemente: Actinoide,onvection electric field. Cusp precipitation is seen at 70°Λ and 09 MLT at the sunward/anti-sunward convection reversal immediately after a sudden turning of interplanetary magnetic field (IMF) B. from -5 nT to +5 nT while IMF B. was-10 nT.作者: Permanent 時間: 2025-3-28 05:05
Handbuch der chemischen Elementeermine if there are any differences between data obtained in this way and data obtained from other techniques. The overall patterns show the expected two-cell convection pattern. In detail, the various individual patterns show subtle but interesting departures from previous results.作者: 發(fā)酵劑 時間: 2025-3-28 09:14
https://doi.org/10.1007/978-3-7091-7968-0res known as magnetic impulse events have been shown to correspond to tailward moving ionospheric current vortices which are probably related to sudden changes in the solar wind dynamic pressure. But also other magnetopause processes may have ionospheric signatures which are seen in the ground magnetic records.作者: 鞠躬 時間: 2025-3-28 11:20
Lasertherapie in der Dermatologieron density is high. On the other hand, the intensity of unstructured Pc 1–2 band pulsations and 750 Hz ELF emission is damped drastically when the waves propagate through the dark ionosphere where the density is low.作者: Oratory 時間: 2025-3-28 16:43
On Quantifying the Distinctions Between the Cusp and the CLEFT/LLBL, time width increases (decreases) when B. changes from northward to southward. A brief review of the various previous attempts at distinctions between the cusp and the cleft is given, as is a brief summary of all known differences between the two regions as observed at low altitude.作者: 割公牛膨脹 時間: 2025-3-28 21:28
Two-Dimensional Mapping of Dayside Convection,onvection electric field. Cusp precipitation is seen at 70°Λ and 09 MLT at the sunward/anti-sunward convection reversal immediately after a sudden turning of interplanetary magnetic field (IMF) B. from -5 nT to +5 nT while IMF B. was-10 nT.作者: Classify 時間: 2025-3-29 02:02
Balloon Observations of the Electric Field Over South Pole: Convection Patterns,ermine if there are any differences between data obtained in this way and data obtained from other techniques. The overall patterns show the expected two-cell convection pattern. In detail, the various individual patterns show subtle but interesting departures from previous results.作者: 神化怪物 時間: 2025-3-29 06:28 作者: 門窗的側(cè)柱 時間: 2025-3-29 07:46
,Pc 1–5 Geomagnetic Pulsations and 750 Hz ELF Activity at Ground Level in the Northern and Southern ron density is high. On the other hand, the intensity of unstructured Pc 1–2 band pulsations and 750 Hz ELF emission is damped drastically when the waves propagate through the dark ionosphere where the density is low.作者: 使殘廢 時間: 2025-3-29 13:29
https://doi.org/10.1007/978-3-662-32927-6r the lower-latitude particle-dominated regions, the auroral oval and the plasma sheet. The basic physical processes are thought to be understood, at least qualitatively, but many unknown and/or controversial aspects remain, particularly concerning the configuration in the case of northward interplanetary magnetic field.作者: hypnotic 時間: 2025-3-29 17:14 作者: epinephrine 時間: 2025-3-29 23:23 作者: 事情 時間: 2025-3-30 01:41 作者: Occupation 時間: 2025-3-30 07:55
Impulsive Penetration of Solar Wind Plasma Irregularities into the Magnetosphere : Relevant Laboratboratory experiments have been reviewed in this article. Their application to the solar wind — magnetosphere system has been presented and discussed. But other additional laboratory experiments exist; they should also be reconsidered and possibly extended.作者: ACTIN 時間: 2025-3-30 08:26
Relationships Between Auroral and Magnetic Activity in the Polar Cusp/Cleft,layers, both the frontside low latitude and the magnetotai1, where induction currents due to relative motion between the sheath plasma and the magnetosphere produces space charges. The importance of the magnetospheric magnetic field model in the study of the cusp phenomena, especially their magnetospheric source regions, is noted.作者: Vulvodynia 時間: 2025-3-30 12:23
https://doi.org/10.1007/978-3-662-32925-2gly twisted and localized magnetic flux tube similar to a magnetic flux rope forms at the magnetopause. When the IMF B. component is small, twin flux tubes appear at the dayside magnetopause. Both types of flux tubes are consistent with several observational features of flux transfer events and are generated by antiparallel magnetic reconnection.作者: 中子 時間: 2025-3-30 16:56
https://doi.org/10.1007/978-3-662-32923-8pport one model over the other, and it is possible that both entry mechanisms contribute depending on magnetopause position, on electron energy, and on the size and extent of boundary and barrier potentials.作者: conduct 時間: 2025-3-30 22:28 作者: Eviction 時間: 2025-3-31 04:02 作者: genuine 時間: 2025-3-31 07:17 作者: 鄙視讀作 時間: 2025-3-31 11:50 作者: 類型 時間: 2025-3-31 15:23
Heating of Thermal Ions Near the Equatorward Boundary of the Mid-Altitude Polar Cleft,ic field spectra are large enough to produce the observed perpendicular oxygen temperatures in time scales determined by the measured poleward drift rate of thermal oxygen ions. The examples presented provide a good comparison of basic plasma theory and observation.作者: LASH 時間: 2025-3-31 20:10 作者: 廣告 時間: 2025-3-31 21:50
Transmission of Solar Wind Hydromagnetic Energy Into the High Latitude Magnetosphere,er research is needed to clarify the different controls between broad-banded and nearly monochromatic wave occurrences as well as to relate these high latitude conclusions to observations made deeper within the magnetosphere.作者: Initiative 時間: 2025-4-1 03:46 作者: exclusice 時間: 2025-4-1 07:16
The Formation of Isolated Magnetic Flux Tubes on the Dayside Magnetopause,wind and the magnetosphere. We found that two types of magnetic flux tubes were formed which depend on the orientation of the interplanetary magnetic field (IMF). The dayside magnetic flux tubes occur only when the IMF has a southward component. When the IMF has a large B. component as well, a stron作者: Soliloquy 時間: 2025-4-1 11:24
Impulsive Penetration of Solar Wind Plasma Irregularities into the Magnetosphere : Relevant Laboratine existing Controlled Laboratory Plasma Experiments which are relevant to the study of solar wind — magnetosphere interaction. Two series of such laboratory experiments have been reviewed in this article. Their application to the solar wind — magnetosphere system has been presented and discussed.
