標(biāo)題: Titlebook: Solar Flare Magnetic Fields and Plasmas; Yuhong Fan,George Fisher Book 2012 Springer Science+Business Media New York 2012 Coronal Mass Eje [打印本頁(yè)] 作者: magnify 時(shí)間: 2025-3-21 18:26
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas影響因子(影響力)
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas被引頻次
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas被引頻次學(xué)科排名
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas年度引用
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas年度引用學(xué)科排名
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas讀者反饋
書(shū)目名稱(chēng)Solar Flare Magnetic Fields and Plasmas讀者反饋學(xué)科排名
作者: 營(yíng)養(yǎng) 時(shí)間: 2025-3-21 20:50 作者: 泥土謙卑 時(shí)間: 2025-3-22 03:35 作者: 運(yùn)動(dòng)吧 時(shí)間: 2025-3-22 05:35 作者: 追逐 時(shí)間: 2025-3-22 11:23
W. P. Abbett,G. H. Fishertnis, dass jede Arbeitsteilung mit einer Vermehrung von Kommunikationskanalen einhergehen muss, mündet zwangsl?ufig in die Forderung ein, dass sich die medizinische Informatik mehr als bisher auf dem Gebiet der medizinischen Organisation im Bereich der Stationen, der Ambulanzen und Verwaltungseinhei作者: 異端邪說(shuō)2 時(shí)間: 2025-3-22 16:15 作者: 昏暗 時(shí)間: 2025-3-22 21:06
P. Heinzel,E. H. Avrettausinformationssysteme, PACS, Datenschutz, ICD, DRG, Computer-based-Training) und der Bioinformatik (z.B. Sequenzanalyse, Gen-Datenbanken, Proteomics, Genomics, Genexpressionsanalyse) anschaulich dargestellt.978-3-540-42568-7978-3-642-55883-2Series ISSN 0937-7433 Series E-ISSN 2512-5214 作者: musicologist 時(shí)間: 2025-3-22 21:35 作者: Aids209 時(shí)間: 2025-3-23 03:25 作者: ABIDE 時(shí)間: 2025-3-23 08:36
Modeling and Interpreting the Effects of Spatial Resolution on Solar Magnetic Field Maps,closer to the line of sight. Further-derived quantities such as vertical current density show variations even in areas of high average magnetic fill fraction. In short, unresolved maps fail to represent the distribution of the underlying unresolved fields, and the “post-facto” methods generally do n作者: 興奮過(guò)度 時(shí)間: 2025-3-23 11:14
Magnetic Connectivity Between Active Regions 10987, 10988, and 10989 by Means of Nonlinear Force-Frevolution of the magnetic field over the period of three days and found no major changes in topologies, as there was no major eruption event. From this study we have concluded that active regions are much more connected magnetically than the electric current.作者: 不能逃避 時(shí)間: 2025-3-23 15:41 作者: 鈍劍 時(shí)間: 2025-3-23 19:21
Can We Determine Electric Fields and Poynting Fluxes from Vector Magnetograms and Doppler Measuremeherefore the Poynting flux of electromagnetic energy in the solar photosphere. Reliable, accurate maps of the Poynting flux are essential for quantitative studies of the buildup of magnetic energy before flares and coronal mass ejections.作者: 字謎游戲 時(shí)間: 2025-3-24 01:03
Predictions of Energy and Helicity in Four Major Eruptive Solar Flares,e predicted free energies lie between the observed energies and the estimated total flare luminosities. The direction of the leading edge of the MC’s poloidal field is aligned with the poloidal field of the flux rope in the AR rather than the global dipole field. These findings compel us to believe 作者: Ingenuity 時(shí)間: 2025-3-24 06:17
Book 2012Richard C. (Dick) Canfield.? Dick has been making profound contributions to these areas of research over a long and productive scientific career.? Many of the articles in this topical issue were first presented as talks during this workshop and represent substantial original work.? The workshop was 作者: impaction 時(shí)間: 2025-3-24 08:04 作者: 索賠 時(shí)間: 2025-3-24 14:31 作者: 吊胃口 時(shí)間: 2025-3-24 15:51
H. S. Hudson,L. Fletcher,G. H. Fisher,W. P. Abbett,A. Russellls eine checklistenartige übersicht der Anforderungen gegeben...Anschlie?end werden die Einsatzm?glichkeiten von Medizinischen Informationssystemen an Beispielen aufgezeigt und ein überblick zum Vorgehen bei der Auswahl und Einführung gegeben...978-3-540-20425-1978-3-540-26855-0作者: 效果 時(shí)間: 2025-3-24 19:59 作者: critic 時(shí)間: 2025-3-25 02:59 作者: Comprise 時(shí)間: 2025-3-25 04:53
S. Régnierls eine checklistenartige übersicht der Anforderungen gegeben...Anschlie?end werden die Einsatzm?glichkeiten von Medizinischen Informationssystemen an Beispielen aufgezeigt und ein überblick zum Vorgehen bei der Auswahl und Einführung gegeben...978-3-540-20425-1978-3-540-26855-0作者: 使服水土 時(shí)間: 2025-3-25 09:01 作者: oxidant 時(shí)間: 2025-3-25 11:59 作者: Affluence 時(shí)間: 2025-3-25 16:10 作者: Institution 時(shí)間: 2025-3-25 21:32 作者: 思鄉(xiāng)病 時(shí)間: 2025-3-26 00:23
uring solar flares.Includes unique new observations of stellThis volume is devoted to the dynamics and diagnostics of solar magnetic fields and plasmas in the Sun’s atmosphere. Five broad areas of current research in Solar Physics are presented: (1) New techniques for incorporating radiation transfe作者: 畸形 時(shí)間: 2025-3-26 05:05 作者: ENNUI 時(shí)間: 2025-3-26 11:05 作者: Implicit 時(shí)間: 2025-3-26 14:19
Optical-to-Radio Continua in Solar Flares,hmark for further modeling and for planning new observations, especially with the ALMA instrument. Finally, we demonstrate how these continua are formed and show a close correspondence between their brightness temperature and the kinetic-temperature structure of the flaring atmosphere.作者: dagger 時(shí)間: 2025-3-26 17:08 作者: PSA-velocity 時(shí)間: 2025-3-26 23:45
Book 2012rch in Solar Physics are presented: (1) New techniques for incorporating radiation transfer effects into three-dimensional magnetohydrodynamic models of the solar interior and atmosphere, (2) The connection between observed radiation processes occurring during flares and the underlying flare energy 作者: 腫塊 時(shí)間: 2025-3-27 01:39 作者: mydriatic 時(shí)間: 2025-3-27 05:29
Radiative Cooling in MHD Models of the Quiet Sun Convection Zone and Corona,ow corona. We discuss an efficient, simplified approximation to the physics of optically thick radiative transport through the surface layers, and investigate the effects of convective turbulence on the magnetic structure of the Sun’s atmosphere in an initially unipolar (open field) region. We find 作者: 機(jī)警 時(shí)間: 2025-3-27 11:50 作者: nonplus 時(shí)間: 2025-3-27 17:35
Optical-to-Radio Continua in Solar Flares, flare models F2 and FLA, we synthesize the thermal continua from optical to mm–radio domains and compare their intensities with quiet-Sun values computed from a recent model C7. In this way, the far-infrared and sub-mm/mm continua are studied for the first time, and we present our results as a benc作者: Finasteride 時(shí)間: 2025-3-27 19:43
The Evolution of Sunspot Magnetic Fields Associated with a Solar Flare, understood, although there is evidence that flaring is related to changes in the topology or complexity of an active-region’s magnetic field. Here, the evolution of the magnetic field in active region NOAA 10953 was examined using ./SOT-SP data over a period of 12 hours leading up to and after a GO作者: Bucket 時(shí)間: 2025-3-27 23:55 作者: Allege 時(shí)間: 2025-3-28 05:36 作者: 吸引人的花招 時(shí)間: 2025-3-28 10:12
Modeling and Interpreting the Effects of Spatial Resolution on Solar Magnetic Field Maps,ment comparisons. The investigation first uses synthetic data, and the results are confirmed with ./SpectroPolarimeter data. Four methods are examined, one which manipulates the Stokes spectra to simulate spatial-resolution degradation, and three “post-facto” methods where the magnetic field maps ar作者: vanquish 時(shí)間: 2025-3-28 13:33 作者: vasculitis 時(shí)間: 2025-3-28 15:47 作者: 很像弓] 時(shí)間: 2025-3-28 22:04
Can We Determine Electric Fields and Poynting Fluxes from Vector Magnetograms and Doppler Measureme us to use Faraday’s law to find an approximate solution for the electric field in the photosphere, using a Poloidal–Toroidal Decomposition (PTD) of the magnetic field and its partial time derivative. Without additional information, however, the electric field found from this technique is under-dete作者: 小臼 時(shí)間: 2025-3-29 00:49
Predictions of Energy and Helicity in Four Major Eruptive Solar Flares,e eruptive solar flares and relate them to observations. We use the three-dimensional . model (Longcope, ., .., 91) and observations of pre-flare photospheric magnetic field and flare ribbons to derive values of reconnected magnetic flux, flare energy, flux rope helicity, and orientation of the flux作者: Microgram 時(shí)間: 2025-3-29 05:23 作者: travail 時(shí)間: 2025-3-29 11:13 作者: 用不完 時(shí)間: 2025-3-29 11:49
A. F. Kowalski,S. L. Hawley,J. A. Holtzman,J. P. Wisniewski,E. J. Hiltong.Viele instruktive Graphiken, umfassender Index.Includes suDas Buch bietet sowohl Medizinern und Biologen als auch Informatikern einen umfassenden und verst?ndlichen Einstieg in die Medizinische Informatik und Bioinformatik. Die Darstellung der Themen ist abgestimmt auf die Studieninhalte dieser ne作者: 爆米花 時(shí)間: 2025-3-29 17:04
P. Heinzel,E. H. Avrettg.Viele instruktive Graphiken, umfassender Index.Includes suDas Buch bietet sowohl Medizinern und Biologen als auch Informatikern einen umfassenden und verst?ndlichen Einstieg in die Medizinische Informatik und Bioinformatik. Die Darstellung der Themen ist abgestimmt auf die Studieninhalte dieser ne作者: 豐滿有漂亮 時(shí)間: 2025-3-29 23:30
