標(biāo)題: Titlebook: Recent Advances in the Understanding of Solar Flares; Proceedings of the U S. R. Kane,Y. Uchida,H. S. Hudson Conference proceedings 1983 Sp [打印本頁(yè)] 作者: stripper 時(shí)間: 2025-3-21 17:15
書(shū)目名稱Recent Advances in the Understanding of Solar Flares影響因子(影響力)
書(shū)目名稱Recent Advances in the Understanding of Solar Flares影響因子(影響力)學(xué)科排名
書(shū)目名稱Recent Advances in the Understanding of Solar Flares網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Recent Advances in the Understanding of Solar Flares網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Recent Advances in the Understanding of Solar Flares被引頻次
書(shū)目名稱Recent Advances in the Understanding of Solar Flares被引頻次學(xué)科排名
書(shū)目名稱Recent Advances in the Understanding of Solar Flares年度引用
書(shū)目名稱Recent Advances in the Understanding of Solar Flares年度引用學(xué)科排名
書(shū)目名稱Recent Advances in the Understanding of Solar Flares讀者反饋
書(shū)目名稱Recent Advances in the Understanding of Solar Flares讀者反饋學(xué)科排名
作者: fluoroscopy 時(shí)間: 2025-3-21 22:29
Solar Flare X-ray Spectra from the P78-1 Spacecraftdiagnostics used in interpreting the spectra are summarized, and the origin of the thermal soft X-ray emitting plasma is discussed in light of the P78-1 results, earlier data, and numerical simulations of magnetic flux tubes heated to solar flare temperatures.作者: 服從 時(shí)間: 2025-3-22 00:25
Energetic Electrons as an Energy Transport Mechanism in Solar Flaresrticular through the diagnostics of both the Fe Kα feature and optically thin transition region lines such as OV. Finally, we discuss the relative roles of electron and proton heating in γ-ray flare events.作者: 創(chuàng)作 時(shí)間: 2025-3-22 06:49 作者: 哺乳動(dòng)物 時(shí)間: 2025-3-22 11:49
Solar Instruments on the P78-1 Spacecraftuilt by the Aerospace Corporation and the Naval Research Laboratory. The hard X-ray spectrometers were built by the Aerospace Corporation and the white light coronagraph was supplied by the Naval Research Laboratory. Most of these instruments are still returning data.作者: 運(yùn)氣 時(shí)間: 2025-3-22 13:58
Magnetic Theories of Solar Flaresm, or emerging flux. The second type is thought to be the result of an eruptive MHD instability that is either spontaneous or triggered from outside. After the eruption the magnetic field lines that have been blown open reconnect back down in a way that has now been simulated numerically.作者: majestic 時(shí)間: 2025-3-22 20:55
Non-Thermal and Non-Equilibrium Effects in Soft X-ray Flare Spectra-state. A search of suitable complex flares with multiple impulsive features has shown indications of soft X-ray line intensity anomalies, consistent with the presence of a non-thermal electron component.作者: 頌揚(yáng)本人 時(shí)間: 2025-3-22 22:08
Transport and Containment of Plasma, Particles and Energy within Flaresture at the time of a flare and a complex and changing magnetic topology during the course of a flare. The rocket data are examined for constraints on flare cooling, within the context of simple loop models. These results form a basis for comments on the limitations of simple loop models for flares.作者: Annotate 時(shí)間: 2025-3-23 05:18
Thermal Evolution of Flare Plasmaursts is confirmed by the observation of an electron temperature increase at the time interval of hard X-ray spikes and a quantitative comparison between thermal energy content and hard X-ray energy input. Non-thermal electrons of 10 keV < E < 30 keV energy may play an important role in pre- and post-burst phases.作者: Deduct 時(shí)間: 2025-3-23 09:17
Upper Limits on the Total Radiant Energy of Solar Flarespulsive emission; for a gradual component, about 4 x 10. ergs total radiant energy. The limits lie about an order of magnitude higher than the total radiant energy estimated from the various known emission components, suggesting that no heretofore unknown dominant component of flare radiation exists.作者: Abbreviate 時(shí)間: 2025-3-23 12:48
ld in Tokyo October 5-8, 1982. The meeting was sponsored jointly by the Japan Society for the Promotion of Science and the u.S. National Science Foundation. The principal aim of the meeting was to obtain the most up-to-date physical picture of solar flares by bringing together results from the recen作者: 槍支 時(shí)間: 2025-3-23 17:12
Conference proceedings 1983o October 5-8, 1982. The meeting was sponsored jointly by the Japan Society for the Promotion of Science and the u.S. National Science Foundation. The principal aim of the meeting was to obtain the most up-to-date physical picture of solar flares by bringing together results from the recent observat作者: iodides 時(shí)間: 2025-3-23 19:51 作者: Jogging 時(shí)間: 2025-3-23 23:45 作者: 谷類 時(shí)間: 2025-3-24 04:15 作者: fixed-joint 時(shí)間: 2025-3-24 09:47
Solar Flare X-ray Spectra from the P78-1 Spacecraft such as electron temperature and density, turbulence, mass motions, and state of ionization equilibrium, characteristic of the thermal soft X-ray emitting flare plasma, and the time behavior of these quantities during flares. In addition, a brief description of the instruments is given, the plasma 作者: 考古學(xué) 時(shí)間: 2025-3-24 12:24 作者: critic 時(shí)間: 2025-3-24 15:54
Observation of Chromospheric Evaporation during the Solar Maximum Missions been analysed to study the upward motions of part of the soft X-ray emitting plasma. These motions are inferred from the presence of secondary blue-shifted lines in the Ca XIX and Fe XXV spectral regions during the impulsive phase of disk flares. Limb flares do not show such blue-shifted lines ind作者: Asseverate 時(shí)間: 2025-3-24 19:36
Transport and Containment of Plasma, Particles and Energy within Flaresmary energy release in the corona through the interaction of magnetic structures, particle and plasma transport into more than a single magnetic structure at the time of a flare and a complex and changing magnetic topology during the course of a flare. The rocket data are examined for constraints on作者: PON 時(shí)間: 2025-3-25 00:02
Interpretation of the Soft X-ray Spectra from HinotoriKα emission at the impulsive phase of the hard X-ray burst,,and assess net Kocemission due to the electron impact by eliminating the fluorescence contribution. Second we discuss on the differences in the electron temperatures and emission measures derived respectively from FeXXVI and FeXXV spectra. 作者: grenade 時(shí)間: 2025-3-25 06:34
Thermal Evolution of Flare Plasmaspectral range. The general trend that the thermal plasma observed in soft X-rays is heated by the non-thermal electrons that emit as the hard X-ray bursts is confirmed by the observation of an electron temperature increase at the time interval of hard X-ray spikes and a quantitative comparison betw作者: HUMID 時(shí)間: 2025-3-25 10:36
Conductive Flux in the Chromosphere Derived from Line Linear Polarization Observationdirected towards disk center..This polarization could be due to collisional excitation of hydrogen and SI by energetic electrons beamed in the vertical direction. Direct excitation by a highly energetic beam of electrons of order 10–100 keV.is doubtful. The heat flux in the region connecting the tra作者: 召集 時(shí)間: 2025-3-25 13:50
Upper Limits on the Total Radiant Energy of Solar Flaresn board the Solar Maximum Mission. Typical limits amount to 6 x 10. erg/s for a 32-second integration time, with 5σ statistical significance for an impulsive emission; for a gradual component, about 4 x 10. ergs total radiant energy. The limits lie about an order of magnitude higher than the total r作者: URN 時(shí)間: 2025-3-25 17:03
Energetic Electrons as an Energy Transport Mechanism in Solar Flaresen “thermal” and “nonthermal” origins of these electrons. We discuss diagnostics in hard X-rays, especially those relating to the recent observations of the SMM and HINOTORI satellites. We also briefly address the response of the atmosphere to energy input in the form of high energy electrons, in pa作者: FLEET 時(shí)間: 2025-3-25 23:39 作者: stress-response 時(shí)間: 2025-3-26 02:03 作者: 擦掉 時(shí)間: 2025-3-26 06:33
Recent Advances in the Understanding of Solar FlaresProceedings of the U作者: nitroglycerin 時(shí)間: 2025-3-26 09:40 作者: collagenase 時(shí)間: 2025-3-26 16:14 作者: pulmonary 時(shí)間: 2025-3-26 18:21
Conductive Flux in the Chromosphere Derived from Line Linear Polarization Observationof the conductive heat flux in the high chromosphere. This conductive flux is of the order of magnitude of the total radiation loss in the chromosphere and below, which is also of the order of magnitude of the conductive flux in the transition zone.作者: Isthmus 時(shí)間: 2025-3-26 22:46 作者: fulcrum 時(shí)間: 2025-3-27 01:33
these results in the context of flare theories would be important. Starting with an introductory presentation of the characteristics of the instruments on board the satellites, the sessions of the first day and the beginning of the second dealt mainly with energy transport in flares and with .the formation pr978-94-009-7230-8978-94-009-7228-5作者: ingrate 時(shí)間: 2025-3-27 05:58 作者: Defense 時(shí)間: 2025-3-27 10:40 作者: hazard 時(shí)間: 2025-3-27 17:23
Y. Tanaka have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: 隱語(yǔ) 時(shí)間: 2025-3-27 20:12
K. J. Frost have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: achlorhydria 時(shí)間: 2025-3-27 22:02
G. A. Doschek have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: 噱頭 時(shí)間: 2025-3-28 04:56
have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: concentrate 時(shí)間: 2025-3-28 06:55
have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: SEMI 時(shí)間: 2025-3-28 13:06 作者: CULP 時(shí)間: 2025-3-28 18:36 作者: 擴(kuò)音器 時(shí)間: 2025-3-28 19:14 作者: BARK 時(shí)間: 2025-3-28 23:34
A. H. Gabriel,E. Antonucci,L. Steenman-Clark have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: 擴(kuò)張 時(shí)間: 2025-3-29 03:49
E. Antonucci,B. R. Dennis have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: 中古 時(shí)間: 2025-3-29 10:10 作者: Sarcoma 時(shí)間: 2025-3-29 14:50
K. Tanaka,N. Nitta,K. Akita,T. Watanabe have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: SAGE 時(shí)間: 2025-3-29 16:52
Kyo Akita,Katsuo Tanaka,Tetsuya Watanabe have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: 清真寺 時(shí)間: 2025-3-29 22:50
Tetsuya Watanabe,Katsuo Tanaka,Kyo Akita,Nariaki Nitta have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: abduction 時(shí)間: 2025-3-30 00:54
J.-C. Henoux,G. Chambe,D. Heristchi,M. Semel,B. Woodgate,D. Shine,J. Beckers have made to cancer care and pays tribute to their dedication and drive. It will provide encouragement for all those confronted with difficulties in building their careers, and will give some inspiration for future leaders..978-3-540-23658-0978-3-540-27069-0作者: 舊石器 時(shí)間: 2025-3-30 04:28
H. S. Hudson,R. C. Willsonitutional change to the benefit of the EP. In Chapter 2.2, we identify three mechanisms based on this approach: the logic of appropriateness, communicative action and rhetorical action. Relying on these three mechanisms, we develop a set of strategies of EP empowerment and theorise their conditions 作者: MIRE 時(shí)間: 2025-3-30 10:16
, we argue that, by using certain strategies, the EP has been pushing the EU in the direction of parliamentary democracy. While we cannot see a fully fledged EU-wide parliamentary democracy any time soon, we contend that the EP has, on its own account and cooperating with actors with similar prefere作者: 自愛(ài) 時(shí)間: 2025-3-30 15:04 作者: acrophobia 時(shí)間: 2025-3-30 16:58 作者: Genistein 時(shí)間: 2025-3-30 23:03 作者: Anecdote 時(shí)間: 2025-3-31 03:51 作者: 托人看管 時(shí)間: 2025-3-31 05:57
K. J. Frostver Story and Masterpiece are two key sections of the magazine that have featured in-depth interviews with some of Europe’s most influential oncology leaders – people who have been pioneers of the art and science of oncology over the past 30 years. These interviews comprise a unique collection of st
