標題: Titlebook: Advances in Space Environment Research; Volume I A. C.-L. Chian,I. H. Cairns,Y. Yan Book 2003 Springer Science+Business Media Dordrecht 200 [打印本頁] 作者: 短暫 時間: 2025-3-21 16:15
書目名稱Advances in Space Environment Research影響因子(影響力)
書目名稱Advances in Space Environment Research影響因子(影響力)學科排名
書目名稱Advances in Space Environment Research網(wǎng)絡(luò)公開度
書目名稱Advances in Space Environment Research網(wǎng)絡(luò)公開度學科排名
書目名稱Advances in Space Environment Research被引頻次
書目名稱Advances in Space Environment Research被引頻次學科排名
書目名稱Advances in Space Environment Research年度引用
書目名稱Advances in Space Environment Research年度引用學科排名
書目名稱Advances in Space Environment Research讀者反饋
書目名稱Advances in Space Environment Research讀者反饋學科排名
作者: Adherent 時間: 2025-3-21 21:44
A Class of TVD Type Combined Numerical Scheme for MHD Equations with a Survey about Numerical MethodVD) type for magnetohydrodynamic equations in spherical coordinates is proposed by taking into account convergence, stability and resolution. This new MHD model is established by solving the fluid equations of MHD system with a modified Lax-Friedrichs scheme and the magnetic induction equations with作者: SEED 時間: 2025-3-22 04:10 作者: MOCK 時間: 2025-3-22 05:34
Computer Simulations of Solar Plasmas Important is the magnetic geometry determined by the magnetic feld lines lying on magnetic surfaces where also the flows are concentrated..Yet, transfer of methods and results obtained in tokamak research to solar coronal plasma dynamics immediately runs into severe problems with trans‘sonic’ (surp作者: 繁榮中國 時間: 2025-3-22 09:44
The Progress of the Taiwan Oscillation Network Projectse maps and the subsurface wave-speed perturbation suffers from the poor vertical resolution of acoustic imaging. Recently an inversion method has been developed to invert the measured phase travel time perturbation to estimate the distribution of wave-speed perturbation based on the ray approximati作者: FEAS 時間: 2025-3-22 15:29 作者: 言外之意 時間: 2025-3-22 18:58 作者: NEX 時間: 2025-3-22 21:42 作者: 自作多情 時間: 2025-3-23 05:15 作者: 適宜 時間: 2025-3-23 06:35
New Insights on Geomagnetic Storms from Model Simulations Using Multi-Spacecraft Dataesent recent model simulations of the stormtime ring current energization due to the enhanced large-scale convection electric field, which show the transition from an asymmetric to a symmetric ring current during the storm and challenge the standard theories of (a) substorm-driven, and (b) symmetric作者: Opponent 時間: 2025-3-23 11:01
Shang-Hong Lai,Vincent Lepetit,Yoichi Satoonent of the electric field penetrated into the magnetosphere are determined by the quarter square of the magnetic Reynolds number. In final, a dynamic model of the magnetospheric magnetic field is constructed. This model can describe the magnetosphere in the course of the severe magnetic storm. The作者: NUDGE 時間: 2025-3-23 16:30 作者: Assignment 時間: 2025-3-23 18:45
Changjae Oh,Bumsub Ham,Kwanghoon Sohnf a more complete understanding of the physics involved? The paper examines the phenomenology of the events, briefly reviews the results of neural network prediction techniques and discusses the conjecture that the underlying physical processes might be related to self-organised criticality and turb作者: 打折 時間: 2025-3-24 00:37
Deep Supervised Hashing with Triplet Labels Important is the magnetic geometry determined by the magnetic feld lines lying on magnetic surfaces where also the flows are concentrated..Yet, transfer of methods and results obtained in tokamak research to solar coronal plasma dynamics immediately runs into severe problems with trans‘sonic’ (surp作者: Iniquitous 時間: 2025-3-24 02:58
Chu-Song Chen,Jiwen Lu,Kai-Kuang Mase maps and the subsurface wave-speed perturbation suffers from the poor vertical resolution of acoustic imaging. Recently an inversion method has been developed to invert the measured phase travel time perturbation to estimate the distribution of wave-speed perturbation based on the ray approximati作者: 玩忽職守 時間: 2025-3-24 10:22 作者: Noctambulant 時間: 2025-3-24 13:18
Oliver Wasenmüller,Didier Strickerx temporal profiles during the flare process so as to understand the energy release and particle accelerations. It is proposed that the rope instability may have triggered the flare event, and reconnection may occur during this process. The drifting pulsation structure in the decimetric frequency ra作者: 絆住 時間: 2025-3-24 17:36
Ching-Hua Weng,Ying-Hsiu Lai,Shang-Hong Laid it is expected to consider non-constant-alpha force-free field model. As the recent result indicates that the plasma beta is sandwich-ed distributed above the solar surface (Gary, 2001), care must be taken in modeling the coronal field correctly. As the reconstruction of solar coronal magnetic fie作者: 奴才 時間: 2025-3-24 21:44 作者: 討厭 時間: 2025-3-25 02:30
Debluring Low-Resolution Imagesesent recent model simulations of the stormtime ring current energization due to the enhanced large-scale convection electric field, which show the transition from an asymmetric to a symmetric ring current during the storm and challenge the standard theories of (a) substorm-driven, and (b) symmetric作者: adequate-intake 時間: 2025-3-25 03:56 作者: hedonic 時間: 2025-3-25 10:07
Modelling of the Electromagnetic Field in the Interplanetary Space and in the Earth’s Magnetospheresolar wind plasma plays a key role in the forming of the interplanetary magnetic field (IMF) component normal to the ecliptic plane. This component is mostly important for the magnetospheric dynamics which is controlled by the solar wind electric field. A simple analytical solution for the problem o作者: Offstage 時間: 2025-3-25 14:04 作者: infatuation 時間: 2025-3-25 17:46 作者: 暫時休息 時間: 2025-3-25 21:58
A Class of TVD Type Combined Numerical Scheme for MHD Equations with a Survey about Numerical Method This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic field (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere. This role comes as no surprise to numerical modelers that participat作者: 萬靈丹 時間: 2025-3-26 02:23 作者: 寒冷 時間: 2025-3-26 06:53 作者: Ophthalmoscope 時間: 2025-3-26 12:20 作者: Lipohypertrophy 時間: 2025-3-26 15:45 作者: 橡子 時間: 2025-3-26 19:55
Variations of the Magnetic Fields in Large Solar Flaressolar flares of 14 July 2000 and 24 November 2000. We show that rapid variations of the line-of-sight magnetic field occured on a time scale of a few minutes during the flare explosions. The reversibility/irreversibility of the magnetic field of both active regions is a very good tool for understand作者: Subdue 時間: 2025-3-26 22:50 作者: Audiometry 時間: 2025-3-27 04:54
Magnetic Reconnection Phenomena in Interplanetary SpaceE3, Wind, etc. We discover that the observational evidence of the magnetic reconnection may be found in the various solar wind structures, such as at the boundary of magnetic cloud, near the current sheet, and small-scale turbulence structures, etc. We have developed a third order accuracy upwind co作者: 太空 時間: 2025-3-27 07:28 作者: ULCER 時間: 2025-3-27 12:30 作者: Archipelago 時間: 2025-3-27 14:53 作者: 刪減 時間: 2025-3-27 21:16
Recent Developments in Magnetospheric Diagnostics Using ULF Wavesd inexpensively monitored from the ground using networks of magnetometers. The most robust measurable quantity provided by magnetometer networks is signal phase and this paper emphasizes the usefulness of this parameter in a variety of ULF wave diagnostic processes ranging from equatorial to high la作者: insurgent 時間: 2025-3-28 01:40
New Insights on Geomagnetic Storms from Model Simulations Using Multi-Spacecraft Dataest to ’space weather’ programs. We thus discuss the dynamical coupling of the solar wind to the Earth’s magnetosphere during several geomagnetic storms using our ring current-atmosphere interactions model and coordinated space-borne data sets. Our model calculates the temporal and spatial evolution作者: 皺痕 時間: 2025-3-28 02:10
Type II Solar Radio Bursts: Theory and Space Weather Implicationsterms of space weather events. The theory is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances.作者: 牌帶來 時間: 2025-3-28 07:54
Variations of the Magnetic Fields in Large Solar Flaresing how the magnetic energy is released in these flares. The observed sharp increase of the magnetic energy density at the time of maximum of the solar flare could involve an unknown component which deposited supplementary energy into the system.作者: folliculitis 時間: 2025-3-28 10:55 作者: 鋼筆記下懲罰 時間: 2025-3-28 18:08 作者: BUCK 時間: 2025-3-28 18:57
Song-Tao Wang,Zhen Zhou,Han-Bing Qu,Bin Literms of space weather events. The theory is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances.作者: 情感 時間: 2025-3-29 02:27
Qing Rao,Lars Krüger,Klaus Dietmayering how the magnetic energy is released in these flares. The observed sharp increase of the magnetic energy density at the time of maximum of the solar flare could involve an unknown component which deposited supplementary energy into the system.作者: ciliary-body 時間: 2025-3-29 05:12 作者: 激怒 時間: 2025-3-29 08:10
um (WSEF2002) and the High Performance Computing in Space Environment Research (HPC2002), organized by the World Institute for Space Environment Research (WISER) from 22 July to 2 August 2002 in Adelaide, Australia. .The articles in this volume review the state-of-the-art of the theoretical, computa作者: 閑逛 時間: 2025-3-29 13:32
Object Boundary Guided Semantic Segmentationl processes are discussed in the framework of the plasmoid ejection model of eruptive solar flares. On the other hand, it is shown that these radio bursts can be considered as radio signatures of eruptive solar flares and thus used for the prediction of heliospheric effects.作者: 羽毛長成 時間: 2025-3-29 18:19 作者: obnoxious 時間: 2025-3-29 21:21 作者: freight 時間: 2025-3-30 02:49 作者: 收養(yǎng) 時間: 2025-3-30 07:24 作者: 低位的人或事 時間: 2025-3-30 10:25 作者: Accrue 時間: 2025-3-30 16:18 作者: 拋物線 時間: 2025-3-30 19:38
Folker Wientapper,Arjan Kuijpere of solar magnetic fields provide information on the magnetic fields in the solar interior. Here we review some of results in helioseismology on the magnetic fields in the solar convection zone. We will also discuss a recent result on the magnetic fields at the base of the convection zone.作者: Perineum 時間: 2025-3-30 20:55 作者: stress-test 時間: 2025-3-31 04:15
Chu-Song Chen,Jiwen Lu,Kai-Kuang Mad inexpensively monitored from the ground using networks of magnetometers. The most robust measurable quantity provided by magnetometer networks is signal phase and this paper emphasizes the usefulness of this parameter in a variety of ULF wave diagnostic processes ranging from equatorial to high latitudes.作者: FLAT 時間: 2025-3-31 05:58
https://doi.org/10.1007/978-94-007-1069-6Corona; Heliosphere; Planet; Solar flare; Solar wind; Sun; astrophysics; solar作者: 租約 時間: 2025-3-31 10:35
978-94-010-3781-5Springer Science+Business Media Dordrecht 2003作者: Mammal 時間: 2025-3-31 15:53 作者: 乏味 時間: 2025-3-31 19:00 作者: 許可 時間: 2025-4-1 01:29 作者: 設(shè)施 時間: 2025-4-1 04:51 作者: MEAN 時間: 2025-4-1 08:02
