標題: Titlebook: Eruptions on the Sun; Boris Filippov Book 2024 The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature [打印本頁] 作者: Washington 時間: 2025-3-21 19:25
書目名稱Eruptions on the Sun影響因子(影響力)
書目名稱Eruptions on the Sun影響因子(影響力)學科排名
書目名稱Eruptions on the Sun網(wǎng)絡(luò)公開度
書目名稱Eruptions on the Sun網(wǎng)絡(luò)公開度學科排名
書目名稱Eruptions on the Sun被引頻次
書目名稱Eruptions on the Sun被引頻次學科排名
書目名稱Eruptions on the Sun年度引用
書目名稱Eruptions on the Sun年度引用學科排名
書目名稱Eruptions on the Sun讀者反饋
書目名稱Eruptions on the Sun讀者反饋學科排名
作者: BLOT 時間: 2025-3-21 20:37 作者: GRAIN 時間: 2025-3-22 01:56 作者: 心胸狹窄 時間: 2025-3-22 05:48
https://doi.org/10.1007/978-3-642-76344-1cribed. More attention is paid to the solar atmosphere, where solar activity phenomena are rape and developed. Some instruments for observations of the Sun, especially the upper layers of the solar atmosphere, which are impossible from the ground level, are listed, as well as space missions dedicate作者: insular 時間: 2025-3-22 08:48
https://doi.org/10.1057/9781137360823itting of spectral lines in the early twentieth century. After the invention of the photoelectric solar magnetograph in the mid-twentieth century, it became clear that magnetic fields are present almost everywhere in the photosphere, but they are distributed very unevenly. The strongest fields are o作者: conception 時間: 2025-3-22 15:33 作者: conception 時間: 2025-3-22 20:24 作者: 暖昧關(guān)系 時間: 2025-3-23 00:17 作者: anticipate 時間: 2025-3-23 03:34 作者: Solace 時間: 2025-3-23 07:02
https://doi.org/10.1007/978-3-642-92045-5ial equilibrium of prominences, different parameters must be achieved for an eruption to begin. In sheared arcade models, there should be a significant increase in shear. In flux-rope models, there is a critical value of twist at which kink instability occurs. The catastrophic loss of equilibrium an作者: strdulate 時間: 2025-3-23 10:13
https://doi.org/10.1007/978-3-642-92044-8ons. The most numerous and ubiquitous are spicules—thin elongated structures in the solar chromosphere. Surges are larger-scale ejections than spicules, but occur much less frequently. They are usually associated with small, changing satellite sunspots. Larger-scale X-ray jets are associated with su作者: 用手捏 時間: 2025-3-23 15:42
https://doi.org/10.1007/978-3-642-99731-0raditionally, solar flares were considered as a sudden, rapid increase in the brightness of a small area of the solar surface in white light, X-ray or EUV, lasting from a few to tens minutes. In a more general sense, solar flares are now assumed as the sudden release of magnetic energy in the solar 作者: 斑駁 時間: 2025-3-23 18:32
https://doi.org/10.1007/978-3-662-42554-1a with a magnetic field within them that escape from the solar atmosphere and propagate through the heliosphere. Arriving at the Earth, the CME shakes the terrestrial magnetosphere, initiating geomagnetic storms and sometimes causing disruption to many of the achievements of the industrial and infor作者: negligence 時間: 2025-3-24 00:06
Mitteilungen über Forschungsarbeiten This chapter provides a brief overview of the characteristics of the solar wind and its manifestations in the heliosphere. There are?two types of solar wind: a slow wind with a speed of about 350?km?s. and a fast wind with speeds of 500–800?km?s.. The fast wind originates in those parts of the coro作者: Resign 時間: 2025-3-24 04:58
https://doi.org/10.1007/978-3-031-58177-9Coronal Mass Ejections; Solar Flares; Prominences; Solar Eruptive Events; Space Weather作者: OTHER 時間: 2025-3-24 10:27
978-3-031-58179-3The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl作者: nominal 時間: 2025-3-24 12:07 作者: receptors 時間: 2025-3-24 16:01
Boris FilippovProvides a comprehensive review of solar eruptive phenomena.Discusses solar observations in tandem with the relevant physics.Offers possible ways for a more reliable forecast of space weather作者: Blatant 時間: 2025-3-24 22:15
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/f/image/320715.jpg作者: SKIFF 時間: 2025-3-24 23:10 作者: Cardioversion 時間: 2025-3-25 05:39
https://doi.org/10.1007/978-1-84996-426-5l global technological infrastructure, mostly of a negative nature. Thus, space weather, which reflects the state of the electromagnetic environment in near-Earth space, is becoming of great importance for humanity.作者: FILLY 時間: 2025-3-25 09:59 作者: countenance 時間: 2025-3-25 13:34
https://doi.org/10.1007/978-3-642-92045-5t. This characteristic of the field is described by the decay index, which has critical values dependent on some properties of the model. The results of critical decay-index estimations in observed eruptive events are presented.作者: FAST 時間: 2025-3-25 15:49 作者: 思考 時間: 2025-3-25 22:07
https://doi.org/10.1007/978-3-642-99731-0The energy released during a flare is most likely stored in the corona in the form of coronal electric currents long before the flare begins. The “standard flare model” was developed in the late 1970s. It includes an eruptive flux rope and a current sheet beneath it, where magnetic reconnection occurs, converting magnetic energy into other forms.作者: 是限制 時間: 2025-3-26 03:28 作者: 高腳酒杯 時間: 2025-3-26 07:38 作者: onlooker 時間: 2025-3-26 09:10 作者: HERE 時間: 2025-3-26 14:58
Solar Jets,ke phenomena are observed in white light using space-born coronagraphs. Modeling of jets is usually associated with magnetic configurations that include a null point, near which magnetic reconnection is possible and plasma flows can be redirected.作者: 斷斷續(xù)續(xù) 時間: 2025-3-26 17:02
Solar Flares,The energy released during a flare is most likely stored in the corona in the form of coronal electric currents long before the flare begins. The “standard flare model” was developed in the late 1970s. It includes an eruptive flux rope and a current sheet beneath it, where magnetic reconnection occurs, converting magnetic energy into other forms.作者: 水土 時間: 2025-3-26 23:43 作者: heartburn 時間: 2025-3-27 03:42 作者: 音樂學者 時間: 2025-3-27 05:45 作者: FLAX 時間: 2025-3-27 11:56 作者: Semblance 時間: 2025-3-27 15:36 作者: Rodent 時間: 2025-3-27 19:03
https://doi.org/10.1007/978-3-658-11623-1 controlled by the magnetic field. All present day prominence models are based on one or other magnetic configuration that creates the magnetic skeleton of the prominence. Other conspicuous plasma structures observed in the corona are coronal cavities, coronal streamers, and polar plumes. Their properties are also briefly discussed.作者: Axillary 時間: 2025-3-27 22:42
https://doi.org/10.1007/978-3-662-11517-6on. The cause of prominence eruptions seems to be in properties of the prominence equilibrium, the possibility of developing instabilities. The structure of the coronal magnetic field not only determines the height of the onset of eruption, but also guides the direction of the motion of eruptive prominences.作者: 新手 時間: 2025-3-28 04:17
Equilibrium Plasma Structures in the Solar Atmosphere, controlled by the magnetic field. All present day prominence models are based on one or other magnetic configuration that creates the magnetic skeleton of the prominence. Other conspicuous plasma structures observed in the corona are coronal cavities, coronal streamers, and polar plumes. Their properties are also briefly discussed.作者: Glower 時間: 2025-3-28 08:07 作者: 難管 時間: 2025-3-28 10:57
Introduction,gnetic field, which is the source of solar activity. Some manifestations of the solar activity affect the Earth’s environment and cause disturbances in the terrestrial magnetic field, geomagnetic storms. Solar flares and coronal mass ejections are hazardous for satellites, space stations, and astron作者: 小步舞 時間: 2025-3-28 15:20
General Characteristics of the Sun,cribed. More attention is paid to the solar atmosphere, where solar activity phenomena are rape and developed. Some instruments for observations of the Sun, especially the upper layers of the solar atmosphere, which are impossible from the ground level, are listed, as well as space missions dedicate作者: 警告 時間: 2025-3-28 19:20
Magnetic Fields on the Sun,itting of spectral lines in the early twentieth century. After the invention of the photoelectric solar magnetograph in the mid-twentieth century, it became clear that magnetic fields are present almost everywhere in the photosphere, but they are distributed very unevenly. The strongest fields are o作者: 妨礙議事 時間: 2025-3-29 02:47
Equilibrium Plasma Structures in the Solar Atmosphere,magnetic field for a long time. Solar prominences were discovered long ago during total eclipse observations. Their types, properties, and magnetic structure are described. The location of prominences on the solar disk and their internal fine structure suggest that prominence plasma is supported and作者: fodlder 時間: 2025-3-29 04:09
Intimate Relationship Between Plasma Structures and Magnetic Fields in the Solar Atmosphere,on and internal structure of coronal plasma formations. Prominences are elongated along large-scale polarity inversion lines of the photospheric magnetic field (neutral lines). It is shown that the prominence material is concentrated close to the magnetic neutral surface or the surface passing throu作者: 公理 時間: 2025-3-29 07:58
Peculiarities of Filament Visual Interaction on the Solar Disk,ity inversion lines changing their positions. The interaction between filaments depends on their internal properties, which are determined by the filament chirality, or the sign of the helicity of the filament magnetic field. In quadrupolar magnetic configurations, filaments with the same chirality 作者: Medicare 時間: 2025-3-29 12:06
Eruption of Prominences,ltogether. Rapidly rising prominences are called eruptive prominences. The general properties of eruptive prominences and their kinematics are considered. In most cases, there is no convincing evidence of the presence of an external source of excitation of the prominence than could lead to an erupti作者: 名字 時間: 2025-3-29 18:44 作者: 范例 時間: 2025-3-29 19:44
Solar Jets,ons. The most numerous and ubiquitous are spicules—thin elongated structures in the solar chromosphere. Surges are larger-scale ejections than spicules, but occur much less frequently. They are usually associated with small, changing satellite sunspots. Larger-scale X-ray jets are associated with su作者: compose 時間: 2025-3-30 01:32
Solar Flares,raditionally, solar flares were considered as a sudden, rapid increase in the brightness of a small area of the solar surface in white light, X-ray or EUV, lasting from a few to tens minutes. In a more general sense, solar flares are now assumed as the sudden release of magnetic energy in the solar 作者: ELATE 時間: 2025-3-30 07:26
Coronal Mass Ejections,a with a magnetic field within them that escape from the solar atmosphere and propagate through the heliosphere. Arriving at the Earth, the CME shakes the terrestrial magnetosphere, initiating geomagnetic storms and sometimes causing disruption to many of the achievements of the industrial and infor
