標(biāo)題: Titlebook: Magnetospheric Imaging — The Image Prime Mission; J. L. Burch Book 2003 Springer Science+Business Media Dordrecht 2003 Heliosphere.Planet. [打印本頁(yè)] 作者: EVOKE 時(shí)間: 2025-3-21 17:50
書目名稱Magnetospheric Imaging — The Image Prime Mission影響因子(影響力)
書目名稱Magnetospheric Imaging — The Image Prime Mission影響因子(影響力)學(xué)科排名
書目名稱Magnetospheric Imaging — The Image Prime Mission網(wǎng)絡(luò)公開(kāi)度
書目名稱Magnetospheric Imaging — The Image Prime Mission網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書目名稱Magnetospheric Imaging — The Image Prime Mission被引頻次
書目名稱Magnetospheric Imaging — The Image Prime Mission被引頻次學(xué)科排名
書目名稱Magnetospheric Imaging — The Image Prime Mission年度引用
書目名稱Magnetospheric Imaging — The Image Prime Mission年度引用學(xué)科排名
書目名稱Magnetospheric Imaging — The Image Prime Mission讀者反饋
書目名稱Magnetospheric Imaging — The Image Prime Mission讀者反饋學(xué)科排名
作者: abracadabra 時(shí)間: 2025-3-22 00:17 作者: inclusive 時(shí)間: 2025-3-22 02:03
Quantifying Global Plasmaspheric Images with , Observations,ellites are combined to understand plasmaspheric behavior and to quantify the global images. A brief review of the understanding of the plasmasphere as learned from in situ observations prior to the launch of IMAGE is given to place the results presented here into context.作者: 一美元 時(shí)間: 2025-3-22 07:07
https://doi.org/10.1007/978-94-010-0027-7Heliosphere; Planet; Solar wind; magnetic field; solar作者: LAITY 時(shí)間: 2025-3-22 12:45 作者: 希望 時(shí)間: 2025-3-22 16:07
Extreme Ultraviolet Imager Observations of the Structure and Dynamics of the Plasmasphere,nance line. The images reveal the details of a highly structured and dynamic entity. Comparing EUV images and selected . observations has helped to validate the remote sensing measurements. The brightness in the EUV images is heavily weighted by the He. density near the plane of the magnetic equator作者: Genetics 時(shí)間: 2025-3-22 17:46
Quantifying Global Plasmaspheric Images with , Observations,ellites are combined to understand plasmaspheric behavior and to quantify the global images. A brief review of the understanding of the plasmasphere as learned from in situ observations prior to the launch of IMAGE is given to place the results presented here into context.作者: 杠桿 時(shí)間: 2025-3-22 22:47 作者: 失眠癥 時(shí)間: 2025-3-23 01:31 作者: Alveoli 時(shí)間: 2025-3-23 09:16 作者: 樹(shù)上結(jié)蜜糖 時(shí)間: 2025-3-23 13:26 作者: 偉大 時(shí)間: 2025-3-23 17:06
The Role and Contributions of Energetic Neutral Atom (ENA) Imaging in Magnetospheric Substorm Resea as observation and quantification of injected particle drift as a function of energy, observation of dynamics in the tail that are directly related to the effects of imposed (growth phase) and induced (expansion phase) electric fields on the plasma, the prompt extraction of oxygen from the ionosphe作者: 污點(diǎn) 時(shí)間: 2025-3-23 18:08
An Overview of Results from RPI on IMAGE,ic radio sounder, relaxation sounder, and a passive plasma wave instrument. The RPI is a highly flexible instrument that can be programmed to perform these types of measurements at times when IMAGE is located in key regions of the magnetosphere. RPI is the first radio sounder ever flown to large rad作者: 慷慨不好 時(shí)間: 2025-3-23 22:36
Global Imaging of Proton and Electron Aurorae in the Far Ultraviolet,er. These provide simultaneous global images, which can be interpreted in terms of the precipitating particle types (protons and electrons) and their energies. IMAGE FUV is the first space-borne global imager that can provide instantaneous global images of the proton precipitation. At times a bright作者: 發(fā)怨言 時(shí)間: 2025-3-24 02:46 作者: Congruous 時(shí)間: 2025-3-24 09:42
Cusp Dynamics and Ionospheric Outflow,al oval is dynamically coupled to the magnetosphere are through the injection of magnetosheath plasma into the magnetospheric cusps and through the ejection of ionospheric plasma into the magnetosphere. The ionospheric footpoints of the Earth’s magnetospheric cusps are relatively narrow regions in i作者: Oligarchy 時(shí)間: 2025-3-24 12:14 作者: contrast-medium 時(shí)間: 2025-3-24 15:24
Heliosphere-Geosphere Interactions Using Low Energy Neutral Atom Imaging,, with the goal of greatly enhanced temporal resolution of an otherwise familiar phenomenon. During ground test and calibration, the LENA imager was found to respond to neutral atoms with energies well above its nominal energy range of 10–750 eV, up to at least 3–4 keV, owing to sputtering interacti作者: 神圣將軍 時(shí)間: 2025-3-24 19:42 作者: 反話 時(shí)間: 2025-3-25 00:39
J. L. Burchtructural equation model by latent factors in 1970, causal modelling by means of latent variables has become the standard in the social and behavioural sciences. Indeed, the central va- ables that social and behavioural theories deal with, can hardly ever be identi?ed as observed variables. Statisti作者: 舞蹈編排 時(shí)間: 2025-3-25 06:13
B. R. Sandel,J. Goldstein,D. L. Gallagher,M. Spasojevicw how this methodology is implemented in practice with curreSince Charles Spearman published his seminal paper on factor analysis in 1904 and Karl Joresk ¨ og replaced the observed variables in an econometric structural equation model by latent factors in 1970, causal modelling by means of latent va作者: 征服 時(shí)間: 2025-3-25 08:34 作者: 健談 時(shí)間: 2025-3-25 12:01
Donald G. Mitchell,Pontus C:Son Brandt,Edmond C. Roelof,Douglas C. Hamilton,Kyle C. Retterer,Steven tructural equation model by latent factors in 1970, causal modelling by means of latent variables has become the standard in the social and behavioural sciences. Indeed, the central va- ables that social and behavioural theories deal with, can hardly ever be identi?ed as observed variables. Statisti作者: Compatriot 時(shí)間: 2025-3-25 18:04
M.-C. Fok,T. E. Moore,G. R. Wilson,J. D. Perez,X. X. Zhang,P. C:Son Brandt,D. G. Mitchell,E. C. Roeltructural equation model by latent factors in 1970, causal modelling by means of latent variables has become the standard in the social and behavioural sciences. Indeed, the central va- ables that social and behavioural theories deal with, can hardly ever be identi?ed as observed variables. Statisti作者: 收集 時(shí)間: 2025-3-25 20:46 作者: anchor 時(shí)間: 2025-3-26 04:11
D. N. Bakerw how this methodology is implemented in practice with curreSince Charles Spearman published his seminal paper on factor analysis in 1904 and Karl Joresk ¨ og replaced the observed variables in an econometric structural equation model by latent factors in 1970, causal modelling by means of latent va作者: HEED 時(shí)間: 2025-3-26 05:24
C. J. Pollock,P. C:Son-Brandt,J. L. Burch,M. G. Henderson,J.-M. Jahn,D. J. Mccomas,S. B. Mende,D. G.tructural equation model by latent factors in 1970, causal modelling by means of latent variables has become the standard in the social and behavioural sciences. Indeed, the central va- ables that social and behavioural theories deal with, can hardly ever be identi?ed as observed variables. Statisti作者: HALO 時(shí)間: 2025-3-26 11:38 作者: puzzle 時(shí)間: 2025-3-26 13:50
Extreme Ultraviolet Imager Observations of the Structure and Dynamics of the Plasmasphere,understanding the ways that electric fields in the inner magnetosphere affect the large and meso-scale distribution of plasma, and their study can elucidate the mechanisms by which the solar wind and interplanetary magnetic field couple to the inner magnetosphere.作者: 癡呆 時(shí)間: 2025-3-26 19:39
Global Imaging of O+ from IMAGE/HENA, the ring current increases during the storm main phase. Our observations suggest that the responsible injection mechanism is mass-dependent and scatters the pitch angles. This leads us to favor a non-adiabatic mechanism proposed by (Delcourt, 2002).作者: 音樂(lè)等 時(shí)間: 2025-3-26 20:59 作者: 放肆的我 時(shí)間: 2025-3-27 03:28
ging of the Earth‘s magnetosphere. IMAGE was launched from Vandenberg AFB into an elliptical polar orbit by a Delta II launch vehicle on March 25, 2000. The two-year prime sci- entific mission of IMAGE began on May 25, 2000 after instrument commissioning was successfully completed. IMAGE has now bee作者: BILE 時(shí)間: 2025-3-27 06:21
lysis. The number of publications based on longitudinal data has increased immensely. Papers with causal claims based on cross-sectional data only experience rejection just for that reason.978-3-642-42572-1978-3-642-11760-2作者: Conflagration 時(shí)間: 2025-3-27 09:47 作者: 出價(jià) 時(shí)間: 2025-3-27 16:16 作者: Institution 時(shí)間: 2025-3-27 17:57 作者: bromide 時(shí)間: 2025-3-27 23:36
S. B. Mende,H. U. Frey,T. J. Immel,J.-C. Gerard,B. Hubert,S. A. Fuselier作者: 斥責(zé) 時(shí)間: 2025-3-28 05:05 作者: 文字 時(shí)間: 2025-3-28 08:16 作者: 矛盾心理 時(shí)間: 2025-3-28 10:28 作者: 討厭 時(shí)間: 2025-3-28 15:52
T. E. Moore,M. R. Collier,M.-C. Fok,S. A. Fuselier,H. Khan,W. Lennartsson,D. G. Simpson,G. R. Wilson作者: 認(rèn)為 時(shí)間: 2025-3-28 20:00 作者: EWE 時(shí)間: 2025-3-29 01:56
M. B. Moldwin,B. R. Sandel,M. F. Thomsen,R. C. Elphics as, for example, on human development and voting behaviour have become available for analysis. The number of publications based on longitudinal data has increased immensely. Papers with causal claims based on cross-sectional data only experience rejection just for that reason.作者: hemophilia 時(shí)間: 2025-3-29 06:03
Donald G. Mitchell,Pontus C:Son Brandt,Edmond C. Roelof,Douglas C. Hamilton,Kyle C. Retterer,Steven s as, for example, on human development and voting behaviour have become available for analysis. The number of publications based on longitudinal data has increased immensely. Papers with causal claims based on cross-sectional data only experience rejection just for that reason.作者: inconceivable 時(shí)間: 2025-3-29 10:40 作者: 孵卵器 時(shí)間: 2025-3-29 13:58 作者: Presbycusis 時(shí)間: 2025-3-29 18:01
The First Two Years of IMAGE,Detached subauroral proton arcs have been found to appear in the afternoon sector following south-north and east-west rotations of the IMF. Low-energy neutral atom imaging has shown global-scale ionospheric outflow to be an immediate response to solar-wind pressure pulses. Such imaging has also prov作者: HUSH 時(shí)間: 2025-3-29 22:31
Global ENA IMAGE Simulations,elop image inversion methods to extract ion information from ENA images. Simulation studies have successfully reproduced and explained energetic ion drift dynamics, the transition from open to closed drift paths, and the magnetosheath response to extreme solar wind conditions. On the other hand, HEN作者: 暗語(yǔ) 時(shí)間: 2025-3-30 00:23 作者: 騎師 時(shí)間: 2025-3-30 04:15
Telescopic and Microscopic Views of the Magnetosphere: Multispacecraft Observations,d initiated a powerful geomagnetic storm (minimum Dst ~ ?360 nT). The CLUSTER set of four spacecraft were located in the midnight sector of the magnetosphere near perigee (r~4 R.) at ~0635 UT and observed a dispersionless injection of energetic (E ≥ 20 keV) electrons in association with a large magn作者: 排出 時(shí)間: 2025-3-30 09:06
An Overview of Results from RPI on IMAGE,r cap and the plasmasphere under a variety of geomagnetic conditions. New results from RPI show that the plasmasphere refills in slightly greater than a day at L values of 2.8 and that ion heating is probably playing a major role in the overall density distribution along the field-line. In addition,作者: 原始 時(shí)間: 2025-3-30 12:47
Global Imaging of Proton and Electron Aurorae in the Far Ultraviolet,is well correlated with the solar wind dynamic pressure and it was found that the direct entry of solar wind particles could account for the intensity of the observed spot without the need for any additional acceleration. Another discovery was the observation of dayside subauroral proton arcs. These
