標題: Titlebook: Earth’s Magnetospheric Processes; Proceedings of a Sym B. M. McCormac Conference proceedings 1972 D. Reidel Publishing Company, Dordrecht, [打印本頁] 作者: obdurate 時間: 2025-3-21 18:44
書目名稱Earth’s Magnetospheric Processes影響因子(影響力)
書目名稱Earth’s Magnetospheric Processes影響因子(影響力)學科排名
書目名稱Earth’s Magnetospheric Processes網絡公開度
書目名稱Earth’s Magnetospheric Processes網絡公開度學科排名
書目名稱Earth’s Magnetospheric Processes被引頻次
書目名稱Earth’s Magnetospheric Processes被引頻次學科排名
書目名稱Earth’s Magnetospheric Processes年度引用
書目名稱Earth’s Magnetospheric Processes年度引用學科排名
書目名稱Earth’s Magnetospheric Processes讀者反饋
書目名稱Earth’s Magnetospheric Processes讀者反饋學科排名
作者: 定點 時間: 2025-3-21 21:35
https://doi.org/10.1007/978-0-8176-8124-1cription of this phenomenon and of the special features of the orbit of AZUR resulting in the tangential passes appears in Rossberg and Theile (1971), Rossberg (1971). This paper deals with the relation of these asymmetric disturbances to geomagnetic activity.作者: Radiation 時間: 2025-3-22 01:50 作者: Allege 時間: 2025-3-22 07:31 作者: obsession 時間: 2025-3-22 12:14
Conference proceedings 1972eriod August 30 through September 10, 1971. One hundred seventy-nine persons from eight- een different countries attended. The authors and the publisher have made a special effort for rapid publication of an up-to-date status of the particles, fields, and processes in the earth‘s magnetosphere, whic作者: 灌溉 時間: 2025-3-22 14:30
https://doi.org/10.1007/978-1-84800-913-4ns over a wide spatial region. In the inner belt, measurements of protons with energies below about 10 MeV have been generally scarce due to instrumental problems caused by penetrating protons or by electrons.作者: 灌溉 時間: 2025-3-22 19:03 作者: 小爭吵 時間: 2025-3-23 00:56 作者: BRAVE 時間: 2025-3-23 02:22
Auroral Particle Precipitation Patterns flux distributions in the noon/dusk sector, (c) latitudinal cross over of 5.8 keV electron and proton precipitation, and (d) K.-dependent 5.8 keV proton population at low latitudes, which is presumably connected with the generation of SAR arcs.作者: BRACE 時間: 2025-3-23 09:29
The Assertion-Training Module — Session 11essary to construct the corresponding quantitative models: to write down the physical equations implied by the qualitative ideas, and solve them. Quantitative models, although of necessity greatly simplified and schematic, serve to test whether our qualitative models really behave as we think they do.作者: 使人入神 時間: 2025-3-23 11:44 作者: 施舍 時間: 2025-3-23 14:15 作者: corporate 時間: 2025-3-23 21:43
A Time Series Approach to Option Pricinge try to identify some of the processes that lead to structure in the profiles in the region of closed field lines. We also show that the use of a suitable coordinate system improves our insight into the causes of structure observed on open field lines.作者: 積習已深 時間: 2025-3-23 23:00 作者: Vaginismus 時間: 2025-3-24 05:48
0067-0057 ring the period August 30 through September 10, 1971. One hundred seventy-nine persons from eight- een different countries attended. The authors and the publisher have made a special effort for rapid publication of an up-to-date status of the particles, fields, and processes in the earth‘s magnetosp作者: 向外供接觸 時間: 2025-3-24 09:38 作者: 反饋 時間: 2025-3-24 11:35 作者: 能夠支付 時間: 2025-3-24 17:22 作者: 天然熱噴泉 時間: 2025-3-24 22:44
Entry of Energetic Solar Protons into the Tailily to investigation by trajectory integration methods, and these have been used here in an attempt to link the structure with the interplanetary anisotropy and hence deduce the penetration mechanisms.作者: 獨裁政府 時間: 2025-3-24 23:59
The Interrelationship of Magnetospheric Processesessary to construct the corresponding quantitative models: to write down the physical equations implied by the qualitative ideas, and solve them. Quantitative models, although of necessity greatly simplified and schematic, serve to test whether our qualitative models really behave as we think they do.作者: Eviction 時間: 2025-3-25 07:21 作者: 現暈光 時間: 2025-3-25 10:04 作者: 紋章 時間: 2025-3-25 11:45
Mechanisms for the Injection of Protons into the Magnetospheree try to identify some of the processes that lead to structure in the profiles in the region of closed field lines. We also show that the use of a suitable coordinate system improves our insight into the causes of structure observed on open field lines.作者: babble 時間: 2025-3-25 16:46 作者: 很像弓] 時間: 2025-3-25 21:26 作者: rheumatism 時間: 2025-3-26 03:57
The Interrelationship of Magnetospheric Processesomplicated phenomenon have led to a sequence of theoretical models of constantly increasing sophistication (see, for example, Axford (1969)). Most of these models have been formulated in qualitative terms. But although such qualitative models are very useful, and indeed indispensable, it is also nec作者: Thrombolysis 時間: 2025-3-26 06:27
Magnetic and Electric Waves in Spacexperiments on many different spacecraft and analyzed with an increasing number of different techniques. In this review, we examine a number of the recent observations of waves in space, discussing the role of waves in the various regions and their characteristics, and illustrating some of their tech作者: Hdl348 時間: 2025-3-26 12:05
Magnetospheric Particle Populationseview, the results of measurements presented in the past 2 yr which give new information will be emphasized. The various magnetospheric regions are shown schematically in the noon-midnight meridian plane in Figure 1, and some features in the equatorial plane are shown in Figure 2. Each of these regi作者: finale 時間: 2025-3-26 13:04
Characteristics of Magnetosheath Plasma Observed at Low Altitudes in the Dayside Magnetospheric Cuspometer (SPS). The extent of these particle fluxes in MLT and IN Lat, their variation with magnetic activity, and their pitch angle distribution are given. Comparison between the SPS data and energetic particle data indicates that the boundary between open and closed field lines on the dayside is ass作者: Vertebra 時間: 2025-3-26 20:38 作者: CLEAR 時間: 2025-3-26 23:25 作者: doxazosin 時間: 2025-3-27 02:08 作者: Ondines-curse 時間: 2025-3-27 08:35 作者: 享樂主義者 時間: 2025-3-27 09:30
New Observations of the Proton Population of the Radiation Belt Between 1.5 and 104 Mevesting theoretical concepts has been the incompleteness of the available data. Several surveys of the trapped proton population have been performed previously (Davis and Williamson, 1963; Freden ., 1965; Fillius, 1966; Gabbe and Brown, 1966; Mihalov and White, 1966; Vernov ., 1967; De Forest, 1970; 作者: 送秋波 時間: 2025-3-27 14:37 作者: LAIR 時間: 2025-3-27 18:35 作者: antedate 時間: 2025-3-28 00:33
Electron Intensities over Auroral Arcsm these measurements is that both the auroral arcs occurred at the boundary between two magnetospheric plasmas. This conclusion is based on the fact that some of the observed changes in electron energy spectrum are unlike the changes to be expected on grounds of continuity from a single source plasm作者: Suppository 時間: 2025-3-28 03:28
The Pre-Midnight Asymmetry in the 40 keV Electron Flux Profiles and Its Relation to Magnetospheric Sboundary, often reveal striking asymmetric deviations of the electron flux levels from the average longitudinal or LT distributions. Among these, the most prominent recurrent asymmetric deviation involves an electron flux profile in the dusk-midnight sector which is terminated by a narrow steep spik作者: regale 時間: 2025-3-28 06:26
https://doi.org/10.1007/978-94-010-2896-7Planet; Population; Variation; magnetosphere; solar作者: 單獨 時間: 2025-3-28 12:28 作者: Eulogy 時間: 2025-3-28 16:10
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/e/image/300938.jpg作者: 單調女 時間: 2025-3-28 22:09
https://doi.org/10.1057/9780230346680Not so long ago the region of space that we now call the magnetosphere used to be considered a very simple part of our environment from a physical point of view: essentially a vacuum penetrated by a magnetic field.作者: glomeruli 時間: 2025-3-28 23:39
https://doi.org/10.1007/978-0-387-68120-7Precipitation patterns of electrons on the dayside have been studied for many years using ground based evidence and satellite experiments. This article will summarize some of the more recent work, and attempt to extend and refine our understanding of these regions.作者: Endemic 時間: 2025-3-29 04:43 作者: infatuation 時間: 2025-3-29 09:55 作者: 煩憂 時間: 2025-3-29 14:26
Pitch Angles and Spectra of Particles in the Outer Zone Near NoonPrecipitation patterns of electrons on the dayside have been studied for many years using ground based evidence and satellite experiments. This article will summarize some of the more recent work, and attempt to extend and refine our understanding of these regions.作者: mechanism 時間: 2025-3-29 17:30
Angular Distributions of Precipitating ElectronsFor auroral electrons the angular distribution within the loss cone is probably the most sensitive indicator of the mechanism which causes the precipitation. However, in the energy range of a few keV, which generally contains most of the auroral electron flux, only very limited results have been reported to date.作者: curriculum 時間: 2025-3-29 22:42 作者: 瑣事 時間: 2025-3-30 00:43 作者: 直覺沒有 時間: 2025-3-30 06:25
New Results on Particle Arrival at the Polar Capsid and Sauer, 1967). More recent satellite results have shown that in at least two solar particle events (Evans and Stone, 1969; Van Allen ., 1971) there were indeed large particle intensity differences between north and south polar regions.作者: 畏縮 時間: 2025-3-30 08:33 作者: Bernstein-test 時間: 2025-3-30 15:54
A Theory of Tutelary Relationships971. It concentrates on studies of the bow shock, magnetosheath, magnetopause, polar cusp, convection-driving electric fields, and the composition of trapped particles of charge greater than one. Whenever possible, particle or field observations are related to the overall question of the magnetosphe作者: Adenoma 時間: 2025-3-30 20:24 作者: Catheter 時間: 2025-3-31 00:03
https://doi.org/10.1007/978-1-349-09136-2xperiments on many different spacecraft and analyzed with an increasing number of different techniques. In this review, we examine a number of the recent observations of waves in space, discussing the role of waves in the various regions and their characteristics, and illustrating some of their tech作者: Exposure 時間: 2025-3-31 01:20
,Conclusion: The New York Press, 1914–1917,eview, the results of measurements presented in the past 2 yr which give new information will be emphasized. The various magnetospheric regions are shown schematically in the noon-midnight meridian plane in Figure 1, and some features in the equatorial plane are shown in Figure 2. Each of these regi作者: EXCEL 時間: 2025-3-31 05:37
https://doi.org/10.1007/978-1-349-17237-5ometer (SPS). The extent of these particle fluxes in MLT and IN Lat, their variation with magnetic activity, and their pitch angle distribution are given. Comparison between the SPS data and energetic particle data indicates that the boundary between open and closed field lines on the dayside is ass作者: Kindle 時間: 2025-3-31 10:08
A Time Series Approach to Option Pricingncluding the magnetotail, and should help us to understand the physical processes occurring in the magneto-sphere. Flux profiles of low energy (～ 1 MeV) solar protons over the polar caps have been studied by many workers, beginning with Williams and Bostrom (1967) and Blake . (1968). In this paper w作者: 并入 時間: 2025-3-31 13:42
https://doi.org/10.1007/978-1-137-48257-0.< 10 MeV and electrons of .<1 MeV) and particular attention has been paid to the flux enhancements frequently observed close to the cutoff latitude, characteristic of the particles (e.g., Williams and Bostrom, 1967, 1969; Blake ., 1968; McDiarmid and Burrows, 1969;Bostrom, 1970).作者: Instrumental 時間: 2025-3-31 20:32 作者: 匍匐前進 時間: 2025-3-31 23:15 作者: 法官 時間: 2025-4-1 03:24 作者: 泄露 時間: 2025-4-1 08:21
https://doi.org/10.1007/978-1-4471-3694-1atellites. The protons trapped by the geomagnetic field have been measured by a great number of satellites, starting with the measurements of Davis and Williamson (1963), who measured the protons at low latitudes in the energy range 100 keV to several MeV. Frank (1967) extended the measurements down
