標(biāo)題: Titlebook: Energy Conversion and Particle Acceleration in the Solar Corona; Karl-Ludwig Klein Book 2003 Springer-Verlag Berlin Heidelberg 2003 Chromo [打印本頁(yè)] 作者: sustained 時(shí)間: 2025-3-21 18:18
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona影響因子(影響力)
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona被引頻次
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona被引頻次學(xué)科排名
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona年度引用
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona年度引用學(xué)科排名
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona讀者反饋
書(shū)目名稱(chēng)Energy Conversion and Particle Acceleration in the Solar Corona讀者反饋學(xué)科排名
作者: 生銹 時(shí)間: 2025-3-21 21:24 作者: 不可思議 時(shí)間: 2025-3-22 01:48 作者: 展覽 時(shí)間: 2025-3-22 05:43 作者: gentle 時(shí)間: 2025-3-22 12:20 作者: abject 時(shí)間: 2025-3-22 14:44 作者: abject 時(shí)間: 2025-3-22 20:30 作者: 令人心醉 時(shí)間: 2025-3-22 23:59
Soft Computing for Biological Systems magnetic field representations are briefly reviewed. The extension to 3-D opens new aspects, some of which are sketched inthis paper: Inparticular two-loop interactions, two-ribbon flare geometry, and the plasmoid formationina current sheet are considered. It is shown that alternative onset process作者: 多嘴多舌 時(shí)間: 2025-3-23 03:02 作者: 不公開(kāi) 時(shí)間: 2025-3-23 08:34 作者: SLAY 時(shí)間: 2025-3-23 10:20 作者: 猛然一拉 時(shí)間: 2025-3-23 14:11 作者: 讓步 時(shí)間: 2025-3-23 19:47 作者: 遭遇 時(shí)間: 2025-3-24 00:50 作者: 為敵 時(shí)間: 2025-3-24 05:02 作者: evaculate 時(shí)間: 2025-3-24 07:59
https://doi.org/10.1007/978-3-030-55704-1 In this paper, recent results on the solar origin of 1-300 keV electrons and 0.1-6 MeV protons are reviewed. The main findings are that one class of electron events escaping into interplanetary space are related to the impulsive phase of the flare (radio type III burst related events), but there is作者: PACT 時(shí)間: 2025-3-24 14:43
https://doi.org/10.1007/978-3-030-51610-9 heliosphere, processes in the solar corona associated with flares and coronal mass ejections (CMEs) are the most energetic natural particle accelerators, sometimes accelerating electrons and ions to relativistic energies. The observation of these particles offers the unique opportunity to study fun作者: 殺死 時(shí)間: 2025-3-24 16:35 作者: –DOX 時(shí)間: 2025-3-24 22:48 作者: Hemoptysis 時(shí)間: 2025-3-25 00:07
https://doi.org/10.1007/978-94-007-0585-2ch was focused on radio observations and related modeling. Progress reached in the following areas is summarized: (1) diagnostics of coronal magnetic fields and the morphology of the field in flares and filament eruptions; (2) evidence of magnetic reconnection and MHD turbulence in radio emissions; 作者: 小步舞 時(shí)間: 2025-3-25 07:24
Fluorescence Photobleaching Recovery,submm) - infrared (IR) range of wavelengths. We describe the new solar dedicated submillimeter wave telescope which began operations at El Leoncito in the Argentina Andes: the SST project. It consists of focal plane arrays of two 405 GHz and four 212 GHz radiometers placed in a 1.5-m radome-enclosed作者: 編輯才信任 時(shí)間: 2025-3-25 10:50
Soft Computing for Biological Systemsalities of mainphase are emphasized. Especially the secondary plasmoid formation is considered and its fate discussed stressing the 3-D aspect of the process and the effect of line-tying. Finally, complex events composed of several distinct, but causally related energy release processes are describe作者: Tonometry 時(shí)間: 2025-3-25 12:46
Soft Computing in Case Based Reasoninghe electrons. Less known are radio emissions from trapped electrons driving loss-cone unstable waves. This is the interpretation usually given to decimetric type IV emission. These types of coherent radio emission give clues on the geometry and plasma parameters near the acceleration region..More sp作者: 使無(wú)效 時(shí)間: 2025-3-25 19:24
Yukinori Suzuki,Seppo Ovaska,Yasuhiko Dotevestigation. While energetic electrons may be generated by the runaway effect in the diffusion region, any super-Alfvénic ions seem to be due to some mechanism not related directly to the reconnection process.作者: 木質(zhì) 時(shí)間: 2025-3-25 22:07 作者: DEFT 時(shí)間: 2025-3-26 01:54
Single Event Soft Error Mechanisms,resolved HXR observations (RHESSI) made simultaneously with a high-cadence detection of selected optical lines, one should be able to diagnose the properties of particle beams, provided that the response of the lower atmospheric layers to beam pulses is strong enough.作者: 粗糙濫制 時(shí)間: 2025-3-26 04:33 作者: 去掉 時(shí)間: 2025-3-26 10:27 作者: 急性 時(shí)間: 2025-3-26 15:58 作者: 浮雕 時(shí)間: 2025-3-26 19:29
Magnetic 3-D Configurations of Energy Release in Solar Flaresalities of mainphase are emphasized. Especially the secondary plasmoid formation is considered and its fate discussed stressing the 3-D aspect of the process and the effect of line-tying. Finally, complex events composed of several distinct, but causally related energy release processes are describe作者: 牲畜欄 時(shí)間: 2025-3-26 21:24
Radio Diagnostics of Flare Energy Releasehe electrons. Less known are radio emissions from trapped electrons driving loss-cone unstable waves. This is the interpretation usually given to decimetric type IV emission. These types of coherent radio emission give clues on the geometry and plasma parameters near the acceleration region..More sp作者: 共棲 時(shí)間: 2025-3-27 02:38
How Well Do We Understand Magnetic Reconnection?vestigation. While energetic electrons may be generated by the runaway effect in the diffusion region, any super-Alfvénic ions seem to be due to some mechanism not related directly to the reconnection process.作者: NIB 時(shí)間: 2025-3-27 09:19
What Can Be Learned About Competing Acceleration Models from Multiwavelength Observations?es of 100 ms or less, even after particle transport effects have been considered. Millimeter wave observations also reveal spatial fragmentation. Together with distributions of overall event size, such fragmentation suggests a scale-invariant energy release process, such as would occur in a state of作者: genuine 時(shí)間: 2025-3-27 12:27
Transport of Energy from the Corona to the Chromosphere During Flaresresolved HXR observations (RHESSI) made simultaneously with a high-cadence detection of selected optical lines, one should be able to diagnose the properties of particle beams, provided that the response of the lower atmospheric layers to beam pulses is strong enough.作者: 表示問(wèn) 時(shí)間: 2025-3-27 16:17
Acceleration and Propagation of Solar Energetic Particleslar atmosphere. The comparison of interacting and escaping particles can provide valuable information about the question whether there is one dominant energization process in solar events, or whether particles are accelerated in multiple processes or sites. Equally important, the study of the propag作者: 轉(zhuǎn)向 時(shí)間: 2025-3-27 19:32 作者: 厚顏無(wú)恥 時(shí)間: 2025-3-28 00:41 作者: ECG769 時(shí)間: 2025-3-28 04:25
Energy Conversion and Particle Acceleration in the Solar Corona作者: gastritis 時(shí)間: 2025-3-28 08:18 作者: FLORA 時(shí)間: 2025-3-28 13:07 作者: 領(lǐng)帶 時(shí)間: 2025-3-28 18:31 作者: 一起平行 時(shí)間: 2025-3-28 20:00
0075-8450 he current theoretical and experimental status in the field. Paying attention to both the details and the broader picture, this book addresses both the experienced researcher as well as non-specialist researchers from related areas and postgraduate students..978-3-642-05546-1978-3-540-36242-5Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: jocular 時(shí)間: 2025-3-29 02:02 作者: GEM 時(shí)間: 2025-3-29 05:02 作者: Between 時(shí)間: 2025-3-29 11:04
Theoretical Models of Magnetic Configurations Relevant to Energy Release the results mostly obtained by the BEM and compare the reconstructed 3D coronal magnetic structures with Hα, soft X-ray, UV/EUV images and/or radio observations so as to understand the triggering and energy release processes in these flare events.作者: deficiency 時(shí)間: 2025-3-29 12:53
Signature of Energy Release and Particle Acceleration Observed by the Nobeyama Radioheliographthat flares start in a small loop and also shown that hot plasmas and high-energy electrons are fed into a nearby larger loop from the small one. Based on these and other observations, it is proposed that “high-beta disruption” is the cause of solar flare phenomena.作者: aqueduct 時(shí)間: 2025-3-29 18:58
0075-8450 in the Sun‘s interior creates its hot corona and a wealth of dynamical phenomena such as flares and mass ejections. Based on recent significant progress in understanding magnetic reconnection and a wealth of new observations of energetic particle signatures from the sun, the present volume reviews t作者: Monolithic 時(shí)間: 2025-3-29 19:43
https://doi.org/10.1007/978-1-4614-5348-2eractions between plasmas and magnetic fields. The manner in which magnetically stored energy is converted to other forms, and prominently to energetic particle populations, is clearly of central importance for coronal physics.作者: 細(xì)查 時(shí)間: 2025-3-30 03:40
Janos Abonyi,Janos Madar,Ferenc Szeifertfield and flow variations. To these one can apply conservation laws and verify whether boundaries, like the magnetopause, have a normal magnetic field component, i.e., are rotational discontinuities. In the magnetotail the magnetic field structure can be deduced from the temporal variation of the magnetic field during high speed flow events.作者: HILAR 時(shí)間: 2025-3-30 04:52 作者: Decimate 時(shí)間: 2025-3-30 09:12
https://doi.org/10.1007/978-94-007-0585-2ion events, as evidenced by the 2000 July 14 (“Bastille Day”) flare; (5) radio imaging of CMEs and filament eruptions; (6) the relationship of coronal and interplanetary shock waves to flares, CMEs, and other coronal waves; and (7) the origin of solar energetic particles.作者: Daily-Value 時(shí)間: 2025-3-30 12:26
Introductioneractions between plasmas and magnetic fields. The manner in which magnetically stored energy is converted to other forms, and prominently to energetic particle populations, is clearly of central importance for coronal physics.作者: Motilin 時(shí)間: 2025-3-30 20:00 作者: Subdue 時(shí)間: 2025-3-30 22:57
On the Origin of Solar Energetic Particle Events events, low energy protons (<6 MeV) are released roughly an hour later than the electrons and are most likely accelerated at the shock fronts of coronal mass ejections. The remaining third of proton events show a puzzling velocity dispersion that could be explained by a non-simultaneous release of protons at different energy.作者: 不可磨滅 時(shí)間: 2025-3-31 04:10 作者: 袋鼠 時(shí)間: 2025-3-31 05:46 作者: 隱士 時(shí)間: 2025-3-31 10:55
