標(biāo)題: Titlebook: Coronal Magnetic Energy Releases; Proceedings of the C Arnold O. Benz,Albrecht Krüger Conference proceedings 1995 Springer-Verlag Berlin He [打印本頁] 作者: Washington 時(shí)間: 2025-3-21 17:48
書目名稱Coronal Magnetic Energy Releases影響因子(影響力)
書目名稱Coronal Magnetic Energy Releases影響因子(影響力)學(xué)科排名
書目名稱Coronal Magnetic Energy Releases網(wǎng)絡(luò)公開度
書目名稱Coronal Magnetic Energy Releases網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Coronal Magnetic Energy Releases被引頻次
書目名稱Coronal Magnetic Energy Releases被引頻次學(xué)科排名
書目名稱Coronal Magnetic Energy Releases年度引用
書目名稱Coronal Magnetic Energy Releases年度引用學(xué)科排名
書目名稱Coronal Magnetic Energy Releases讀者反饋
書目名稱Coronal Magnetic Energy Releases讀者反饋學(xué)科排名
作者: pancreas 時(shí)間: 2025-3-21 20:28
Imaging, stereoscopy, and tomography of the solar corona in soft X-rays and radio,accurate measurements of geometric parameters (position, altitude, rotation rate), but also the deconvolution of physical parameters (density, temperature, magnetic field) along the line-of-sight, which is most feasible with simultaneous observations in complementary wavelengths, e.g. in soft X-rays, EUV, and radio.作者: Genistein 時(shí)間: 2025-3-22 04:27
Long-duration non thermal energy release in flares and outside flares,ursts, storm continua and noise storms. The energy budget of suprathermal particles is estimated, possible acceleration sites are investigated, and similarities and differences between impulsive flares, gradual events and noise storms are discussed.作者: chemoprevention 時(shí)間: 2025-3-22 05:07
Coupled magnetohydrodynamic and kinetic development of current sheets in the solar corona,energy release, (4) the acceleration of particles in such an environment. The dynamical current sheet model naturally explains fragmentary energy release, and it may lead to a better understanding of particle acceleration and of the cross-field propagation of the flare disturbance.作者: MEET 時(shí)間: 2025-3-22 10:18
EIT: The extreme ultraviolet imaging telescope,ive temperature diagnostic in the range 6.10. to 3.10.K. This SOHO instrument will thus probe the coronal plasma on a global scale, as well as the underlying cooler and turbulent atmosphere. The EIT‘s characteristics and performances are presented, and prospects for coordinated observations with ground-based radio observatories are outlined.作者: 潛移默化 時(shí)間: 2025-3-22 13:36
Summary and Implications for Future Researched on the scenario of self organised criticality, reproduces many of the known flare characteristics. The same model is used to provide a large number of nanoflares, which can heat the corona. We also show that this complex, inhomogeneous active region, is an efficient accelerator and reproduce the observed dm spikes and type III bursts.作者: 潛移默化 時(shí)間: 2025-3-22 20:50 作者: acheon 時(shí)間: 2025-3-22 21:26 作者: PSA-velocity 時(shí)間: 2025-3-23 01:54 作者: Rodent 時(shí)間: 2025-3-23 05:49 作者: 只有 時(shí)間: 2025-3-23 10:54
Wavelet Theory and Its Applicationsting process of active, rapidly rotating stars. However, the required cadence of flares has not (yet) been found. The link between stellar coronal heating and magnetic energy release is not clear as long as the various flare-like phenomena in the solar corona are not better understood.作者: Indecisive 時(shí)間: 2025-3-23 17:31
Gender Segregation in the Workplaceal images, a much faster operation. Ordering the archive by its content, which facilitates searching and comparing tasks, is investigated using self-organizing maps. Such a map conserves the topological order of the input space. This property may be used to automatically distinguish dissimilar emission types.作者: Alpha-Cells 時(shí)間: 2025-3-23 18:16
Gender Segregation in the Workplaceedium has been carried out at Cambridge since March 1990. The method will be described and some typical disturbances observed during this period will be shown. The results provide new insights into the nature of coronal magnetic energy releases responsible for the most powerful interplanetary shocks.作者: 序曲 時(shí)間: 2025-3-24 00:47
A. Lempicki,A. J. Wojtowicz,C. Brecher temperature range from 10.to 2 × 10... SUMER will be flown on the ESA/NASA spacecraft Solar and Heliospheric Observatory (SOHO) to be launched in September 1995. SOHO will be positioned near the first Lagrangean point (L1) of the Sun-Earth system.作者: 有權(quán) 時(shí)間: 2025-3-24 03:06
Flares and coronal heating in the sun and stars,ting process of active, rapidly rotating stars. However, the required cadence of flares has not (yet) been found. The link between stellar coronal heating and magnetic energy release is not clear as long as the various flare-like phenomena in the solar corona are not better understood.作者: 奴才 時(shí)間: 2025-3-24 10:25 作者: resistant 時(shí)間: 2025-3-24 12:53
Interplanetary scintillation imaging of disturbances in the solar wind,edium has been carried out at Cambridge since March 1990. The method will be described and some typical disturbances observed during this period will be shown. The results provide new insights into the nature of coronal magnetic energy releases responsible for the most powerful interplanetary shocks.作者: 熒光 時(shí)間: 2025-3-24 15:31
,SUMER — Solar Ultraviolet Measurements of Emitted Radiation, temperature range from 10.to 2 × 10... SUMER will be flown on the ESA/NASA spacecraft Solar and Heliospheric Observatory (SOHO) to be launched in September 1995. SOHO will be positioned near the first Lagrangean point (L1) of the Sun-Earth system.作者: 惡心 時(shí)間: 2025-3-24 20:04 作者: nuclear-tests 時(shí)間: 2025-3-25 01:45 作者: 沖擊力 時(shí)間: 2025-3-25 06:32 作者: Mortal 時(shí)間: 2025-3-25 08:47
Numerical simulations of shock electron acceleration in solar physics, mainly based on full particle electrostatic and electromagnetic codes. Such codes are appropriate to follow the overall dynamics of the shock itself and to identify the different sources of acceleration and heating of particles in a self-consistent way.作者: CLIFF 時(shí)間: 2025-3-25 11:42 作者: 稀釋前 時(shí)間: 2025-3-25 16:31
0075-8450 of magnetic energy releases. The experimental data from groundbased methods of radio astronomy as well as from satellites are also discussed. The book addresses researchers in astrophysics, and planetary science but should also be accessible to graduate students.978-3-662-14002-4978-3-540-49189-7Ser作者: thrombus 時(shí)間: 2025-3-25 21:53
https://doi.org/10.1007/978-1-4615-3584-3accurate measurements of geometric parameters (position, altitude, rotation rate), but also the deconvolution of physical parameters (density, temperature, magnetic field) along the line-of-sight, which is most feasible with simultaneous observations in complementary wavelengths, e.g. in soft X-rays, EUV, and radio.作者: TAIN 時(shí)間: 2025-3-26 04:05 作者: Carbon-Monoxide 時(shí)間: 2025-3-26 08:10 作者: Felicitous 時(shí)間: 2025-3-26 10:08
Performance of Natural I/O Applications,ive temperature diagnostic in the range 6.10. to 3.10.K. This SOHO instrument will thus probe the coronal plasma on a global scale, as well as the underlying cooler and turbulent atmosphere. The EIT‘s characteristics and performances are presented, and prospects for coordinated observations with ground-based radio observatories are outlined.作者: conscience 時(shí)間: 2025-3-26 15:46 作者: LUMEN 時(shí)間: 2025-3-26 20:32
Imaging, stereoscopy, and tomography of the solar corona in soft X-rays and radio,e three-dimensional (3D) reconstruction techniques, such as stereoscopy and tomography. The 3D reconstruction of coronal structures involves not only accurate measurements of geometric parameters (position, altitude, rotation rate), but also the deconvolution of physical parameters (density, tempera作者: Flawless 時(shí)間: 2025-3-26 22:09
Initial results from the Nobeyama Radiobeliograph,observations, which contain a last part of the maximum phase of the solar cycle 22, it was possible to obtain almost every aspect of solar activity at 17 GHz. They include two X-class flares, tens of M-class flares, hundreds of flares from the very initial phase through the late decay phase, or from作者: phlegm 時(shí)間: 2025-3-27 04:12 作者: LITHE 時(shí)間: 2025-3-27 07:45 作者: intolerance 時(shí)間: 2025-3-27 12:00 作者: 無情 時(shí)間: 2025-3-27 16:45 作者: 昏暗 時(shí)間: 2025-3-27 19:01 作者: predict 時(shí)間: 2025-3-28 00:05 作者: cravat 時(shí)間: 2025-3-28 03:40
Non-linear data analysis and statistical techniques in solar radio astronomy, from turbulence theory is an appropriate method to find out some scaling behavior of fluctuations in time. More generally, the wavelet analysis, which is some generalization of the power spectrum, exhibits information on the location as well as the size of hidden characteristic features. Applying b作者: Grandstand 時(shí)間: 2025-3-28 08:45 作者: 血友病 時(shí)間: 2025-3-28 10:50 作者: thrombosis 時(shí)間: 2025-3-28 15:03 作者: 怕失去錢 時(shí)間: 2025-3-28 19:49
Surprises in the radio signatures of CMEs,nding of these phenomena considerably. Imaging observations of metric radio emissions along with coronagraph observations have been used to obtain these results. We consider the following: (i) Why slow CMEs are associated with metric type IV radio emission contrary to the earlier belief, (ii) Why sh作者: adroit 時(shí)間: 2025-3-29 02:46
The SOHO mission,rplanetary space. It is currently scheduled for launch in 1995. In this paper a mission overview is given, comprising scientific objectives, payload, spacecraft, operations, and data and ground system.作者: 完整 時(shí)間: 2025-3-29 05:05
,SUMER — Solar Ultraviolet Measurements of Emitted Radiation,ructures and events associated with solar magnetic activity in the chromosphere, the transition zone and the corona. Specifically, SUMER will measure profiles and intensities of extreme ultraviolet (EUV) lines emitted in the solar atmosphere ranging from the upper chromosphere to the lower corona; d作者: Stagger 時(shí)間: 2025-3-29 10:35 作者: 血統(tǒng) 時(shí)間: 2025-3-29 12:27 作者: 節(jié)約 時(shí)間: 2025-3-29 16:50 作者: mastopexy 時(shí)間: 2025-3-29 22:40 作者: 浪蕩子 時(shí)間: 2025-3-30 02:07 作者: 虛假 時(shí)間: 2025-3-30 05:59 作者: 厚顏無恥 時(shí)間: 2025-3-30 11:22 作者: Venules 時(shí)間: 2025-3-30 13:19
Wavelet Theory and Its Applicationsagnetic energy. Several solar phenomena from bright points to coronal mass ejections are attributed to free magnetic energy apparently available in the corona. The possibility that magnetic energy release is the dominant energy input into the corona is discussed for the Sun with special emphasis on 作者: acrobat 時(shí)間: 2025-3-30 19:00
https://doi.org/10.1007/978-1-4615-3584-3e three-dimensional (3D) reconstruction techniques, such as stereoscopy and tomography. The 3D reconstruction of coronal structures involves not only accurate measurements of geometric parameters (position, altitude, rotation rate), but also the deconvolution of physical parameters (density, tempera作者: 獨(dú)白 時(shí)間: 2025-3-30 20:45
Women, Work-Related Stress, and Smokingobservations, which contain a last part of the maximum phase of the solar cycle 22, it was possible to obtain almost every aspect of solar activity at 17 GHz. They include two X-class flares, tens of M-class flares, hundreds of flares from the very initial phase through the late decay phase, or from作者: impale 時(shí)間: 2025-3-31 04:40
Summary and Implications for Future ResearchX-ray and microwave emission: gradual hard X-ray and associated radio emission from centimetric to hectometric waves, Moving Type IV bursts, Type II bursts, storm continua and noise storms. The energy budget of suprathermal particles is estimated, possible acceleration sites are investigated, and si作者: Cumbersome 時(shí)間: 2025-3-31 06:06
Women, Work-Related Stress, and Smoking and in the one case for which we have simultaneous soft and hard X-ray images, they also show compact sources coincident with the radio source. One of the bursts is barely detected in soft X-rays, yet has a moderate 17 GHz flux,.作者: Precursor 時(shí)間: 2025-3-31 09:46 作者: Spartan 時(shí)間: 2025-3-31 14:33
Summary and Implications for Future Researchtion of magnetohydrodynamic (i.e., tearing and coalescence) and kinetic currentdriven instabilities, (3) the resulting spatial and temporal scales of energy release, (4) the acceleration of particles in such an environment. The dynamical current sheet model naturally explains fragmentary energy rele作者: 阻擋 時(shí)間: 2025-3-31 19:30
Summary and Implications for Future Researchzone. Random movements of the feet of the fibers in the photosphere and emergence of new magnetic flux from the convection zone are responsible for the formation of neutral sheets and magnetic discontinuities inside the active region, which are the sites for magnetic dissipation. A simple model, bas作者: 淡紫色花 時(shí)間: 2025-4-1 00:24
Dissolved Oxygen and Redox Potential,zed compact objects accretion can be modified by repeated magnetic energy storage and release. Further also in the absence of a central magnetosphere, such as around galactic and extragalactic black holes, magnetic flaring activity is possible in a corona on both sides of the disk..Moreover strong o作者: 使殘廢 時(shí)間: 2025-4-1 05:45 作者: STRIA 時(shí)間: 2025-4-1 08:23
Gender Segregation in the Workplacety along the line of sight. Routine daily observations of interplanetary scintillation (IPS) on about 1000 sources can be used to construct whole-sky maps showing the two-dimensional projection of large scale features of enhanced, or reduced density such as corotating streams or compression zones fo作者: 凈禮 時(shí)間: 2025-4-1 10:10 作者: Synovial-Fluid 時(shí)間: 2025-4-1 14:53
Hosts for Solid-State Luminescent Systems,ation are not been fully understood yet. A two-step mechanism is often invoked including (i) the formation of electrons streams by shock waves and (ii) the excitation of radio emission by these streams. In the present report, we will focuss mainly on step (i) through results of numerical simulations
