標(biāo)題: Titlebook: Comic Rays in Interplanetary Magnetics Fields; I. N. Toptygin Book 1985 D. Reidel Publishing Company, Dordrecht, Holland 1985 Corona.Plane [打印本頁] 作者: 葉子 時(shí)間: 2025-3-21 16:28
書目名稱Comic Rays in Interplanetary Magnetics Fields影響因子(影響力)
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書目名稱Comic Rays in Interplanetary Magnetics Fields被引頻次
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書目名稱Comic Rays in Interplanetary Magnetics Fields讀者反饋
書目名稱Comic Rays in Interplanetary Magnetics Fields讀者反饋學(xué)科排名
作者: Dysarthria 時(shí)間: 2025-3-21 21:01 作者: 數(shù)量 時(shí)間: 2025-3-22 01:32
Book 1985tudy of cosmic ray spectra, time variations, abundances, gradients, and anisotropy provides a wealth of data on physical conditions in the regions of cosmic ray generation as well as in the media through which cosmic rays propagate. Astrophysical aspects of cosmic ray physics have been considered in作者: 抒情短詩 時(shí)間: 2025-3-22 06:31 作者: 蝕刻 時(shí)間: 2025-3-22 12:35 作者: 減震 時(shí)間: 2025-3-22 13:51
Mariacristina Rossi,Eva M. Sierminskaions and measurements on the Earth could not be compared with those obtained on spacecraft. Hence, the period of time prior to the beginning of direct observations in space may be naturally called the pre-history of cosmic physics.作者: 減震 時(shí)間: 2025-3-22 19:21 作者: Adulate 時(shí)間: 2025-3-23 01:09
Modulation of Galactic Cosmic Rays,. The nature of particles with lower energy is not entirely clear. According to estimates by Hayakawa (1969), particles of solar origin produce 10% of the total cosmic ray intensity in the solar system. The fraction of solar particles is likely to increase with decreasing energy.作者: graphy 時(shí)間: 2025-3-23 04:26 作者: Ceremony 時(shí)間: 2025-3-23 08:17 作者: Harridan 時(shí)間: 2025-3-23 12:19
https://doi.org/10.1007/978-3-319-92345-1ntury (e.g., see Brandt, 1970; for review). The continuous character of the solar wind was experimentally proved by Biermann (1951, 1952) by an investigation of the behaviour of comet tails. This result was also confirmed indirectly by observations of the modulation effects of galactic cosmic rays and by data on geomagnetic activity and aurorae.作者: 善于 時(shí)間: 2025-3-23 16:03 作者: Finasteride 時(shí)間: 2025-3-23 19:59 作者: opprobrious 時(shí)間: 2025-3-24 00:09
Theory of Fast Particle Motion in Interplanetary Magnetic Fields, 10. K). With increasing energy, the mean free path increases as energy squared in the non-relativistic energy range. The mean free path of cosmic rays with respect to nuclear collisions is even larger.作者: Exuberance 時(shí)間: 2025-3-24 03:21
Geophysics and Astrophysics Monographshttp://image.papertrans.cn/c/image/238896.jpg作者: Conscientious 時(shí)間: 2025-3-24 09:35 作者: 我不怕犧牲 時(shí)間: 2025-3-24 12:35 作者: Lamina 時(shí)間: 2025-3-24 15:52 作者: conscribe 時(shí)間: 2025-3-24 21:06 作者: inferno 時(shí)間: 2025-3-25 00:34
Mariacristina Rossi,Eva M. Sierminskases of particle energy variations have been considered, such as adiabatic deceleration in expanding streams of magnetic inhomogeneities (§8,1, 12, 13) and in large-scale magnetic fields frozen into the plasma (§8.4), as well as the Fermi acceleration by large-scale regular plasma motions (§8.3). Thi作者: Demonstrate 時(shí)間: 2025-3-25 06:17
Homeownership and Wealth Accumulation,of solar wind plasma particles. The energy of the most energetic particles detected in extensive atmospheric showers exceeds 10. eV. In this enormous energy range it is impossible to determine the exact critical energy which separates solar and galactic cosmic rays. However, since particles with T >作者: 掙扎 時(shí)間: 2025-3-25 08:18 作者: 易發(fā)怒 時(shí)間: 2025-3-25 14:46
https://doi.org/10.1007/978-94-009-5257-7Corona; Planet; Solar flare; Solar wind; solar作者: 骨 時(shí)間: 2025-3-25 17:15 作者: 泛濫 時(shí)間: 2025-3-25 22:00
Propagation of Energetic Solar Particles,article propagation in interplanetary space. The data presented are only basic and not totally complete. More detailed data may be found in the monograph by Dorman and Miroshnichenko (1968), and in the review by Dorman (1978).作者: 艱苦地移動 時(shí)間: 2025-3-26 04:09
Physical Properties of the Interplanetary Medium,circumsolar space. This is a more or less continuous plasma flow which is generated in the upper corona of the Sun and carries magnetic fields of solar origin. The first indications of the existence of some corpuscular flow, directed from the Sun, in interplanetary space were obtained in the last ce作者: 跳動 時(shí)間: 2025-3-26 07:35 作者: fabricate 時(shí)間: 2025-3-26 12:07 作者: 背心 時(shí)間: 2025-3-26 15:54
Particle Acceleration Processes in Interplanetary Space,ses of particle energy variations have been considered, such as adiabatic deceleration in expanding streams of magnetic inhomogeneities (§8,1, 12, 13) and in large-scale magnetic fields frozen into the plasma (§8.4), as well as the Fermi acceleration by large-scale regular plasma motions (§8.3). Thi作者: bile648 時(shí)間: 2025-3-26 18:39 作者: 人造 時(shí)間: 2025-3-27 00:43
Concluding Remarks,7. Although various physical phenomena in this field had been studied long before that time, the amount and quality of the data obtained from observations and measurements on the Earth could not be compared with those obtained on spacecraft. Hence, the period of time prior to the beginning of direct作者: 尋找 時(shí)間: 2025-3-27 01:42 作者: 混亂生活 時(shí)間: 2025-3-27 08:07 作者: 根除 時(shí)間: 2025-3-27 10:58 作者: 俗艷 時(shí)間: 2025-3-27 15:48 作者: Toxoid-Vaccines 時(shí)間: 2025-3-27 18:55 作者: 土產(chǎn) 時(shí)間: 2025-3-28 00:33
Angela Smith,Sheila Quaidtill open. First, contrast US will hardly replace CT or MR imaging for preoperative assessment of patients with liver tumors, as these techniques still offer a more comprehensive assessment of the liver parenchyma, which is mandatory to properly plan any kind of surgical or interventional procedure.作者: compel 時(shí)間: 2025-3-28 05:23
