標(biāo)題: Titlebook: Genesis and Propagation of Cosmic Rays; Maurice M. Shapiro (Director of the School, Co-Dir Book 1988 D. Reidel Publishing Company, Dordrec [打印本頁] 作者: Jackson 時間: 2025-3-21 18:29
書目名稱Genesis and Propagation of Cosmic Rays影響因子(影響力)
書目名稱Genesis and Propagation of Cosmic Rays影響因子(影響力)學(xué)科排名
書目名稱Genesis and Propagation of Cosmic Rays網(wǎng)絡(luò)公開度
書目名稱Genesis and Propagation of Cosmic Rays網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Genesis and Propagation of Cosmic Rays被引頻次
書目名稱Genesis and Propagation of Cosmic Rays被引頻次學(xué)科排名
書目名稱Genesis and Propagation of Cosmic Rays年度引用
書目名稱Genesis and Propagation of Cosmic Rays年度引用學(xué)科排名
書目名稱Genesis and Propagation of Cosmic Rays讀者反饋
書目名稱Genesis and Propagation of Cosmic Rays讀者反饋學(xué)科排名
作者: 啪心兒跳動 時間: 2025-3-21 21:53
Stars and Cosmic Rays,e review our current knowledge on “solarlike activity” and its relation with stellar parameters at various locations of the Hertzsprung-Russell diagram. This “solar-stellar connection” emphasizes the role of solar studies in helping to understand the pre-acceleration states of the history of galactic cosmic rays.作者: TERRA 時間: 2025-3-22 03:35
Conditions for Acceleration of Super-High Energy Cosmic Rays in Active Galactic Nuclei,a low impedance element (ambient conducting medium). Beam particles can be accelerated to 10. provided that the beam channel medium behaves like an inductive circuit with high impedance. But even if these conditions are satisfied, a major difficulty the model faces is the large energy loss caused by photomeson reactions.作者: 詞匯記憶方法 時間: 2025-3-22 06:02
Cosmic Ray Bombardment of Solids in Space,ant role played in giant molecular clouds by cosmic rays for the production of molecular hydrogen, the cornerstone of interstellar chemistry. A method to obtain suitable information on the almost unknown spectrum of low energy cosmic rays outside the heliosphere is also presented.作者: DEAWL 時間: 2025-3-22 12:16
Current Issues in Macroeconomics sky area. Events with energy above 5×10. eV are largely of extragalactic origin. Several particles arrive preferentialy from the general direction of the local supercluster. There is also an excess of particles coming from the Galactic South Pole direction, which is not understood.作者: invade 時間: 2025-3-22 15:36
Current Issues in Maritime Economicse review our current knowledge on “solarlike activity” and its relation with stellar parameters at various locations of the Hertzsprung-Russell diagram. This “solar-stellar connection” emphasizes the role of solar studies in helping to understand the pre-acceleration states of the history of galactic cosmic rays.作者: invade 時間: 2025-3-22 18:21 作者: 混合 時間: 2025-3-22 22:21
Elling Prediction in Ocular Pursuit,ant role played in giant molecular clouds by cosmic rays for the production of molecular hydrogen, the cornerstone of interstellar chemistry. A method to obtain suitable information on the almost unknown spectrum of low energy cosmic rays outside the heliosphere is also presented.作者: 模仿 時間: 2025-3-23 04:12
Enrico G. Beltrametti,Bas C. Fraassenhese results are then compared with the measured properties of the e. component of cosmic rays in the solar neighborhood. It is found that even though this component of the cosmic rays is a rather minor one in terms of either number or energetics, it is the component which appears best explained by known phenomena at the present time.作者: Mendacious 時間: 2025-3-23 09:09 作者: 表臉 時間: 2025-3-24 01:04 作者: 殺菌劑 時間: 2025-3-24 04:41
Stars and Cosmic Rays,th cool stars: protons, antiprotons, γ-rays, neutrinos, but also X-rays (> keV) and nuclear γ-ray lines. In spite of these differences, common features between hot and cool stars as regards their connection with cosmic rays are singled out.作者: debase 時間: 2025-3-24 08:46 作者: Calculus 時間: 2025-3-24 12:54
Hadron and Muon Components in Photon Shower at 1015 eV, muons (Eμ > 500 GeV) in events generated by primary photons of very high energy. The calculated lateral distributions of muons with Eμ > 5 G and Eμ > 2 GeV in gamma-initiated showers predict a ? 8 ÷ 10 times lower density of the muon flux in comparison with the one in showers from primary protons or nuclei.作者: 率直 時間: 2025-3-24 15:30
,Monopoles, Muons, Neutrinos, and Cygnus X?3,y data, in coincidence with the underground detector, since July of 1985. We describe the initial surface-underground data, and discuss the experiments to search for magnetic monopoles at the level of the Parker limit, neutrinos, and high energy cosmic ray air showers with these instruments and with a new atmospheric Cerenkov detector.作者: infatuation 時間: 2025-3-24 21:40 作者: Androgen 時間: 2025-3-25 00:25 作者: craven 時間: 2025-3-25 04:51
Current Issues in Macroeconomics. Measurements from Haverah Park (northern hemisphere) and Sydney (southern hemisphere) are consistent in energy spectrum and anisotropy in the common sky area. Events with energy above 5×10. eV are largely of extragalactic origin. Several particles arrive preferentialy from the general direction of作者: hypnotic 時間: 2025-3-25 08:51
Current Issues in Maritime Economics bulk of the cosmic-ray nuclei originate in F to M stars appears to be independently supported by studies of stellar outer atmospheres and activity. We review our current knowledge on “solarlike activity” and its relation with stellar parameters at various locations of the Hertzsprung-Russell diagra作者: alcohol-abuse 時間: 2025-3-25 14:20
Current Issues in Microeconomicsouds: they excite giant HII regions, inside which they create large wind cavities. The possibility of particle acceleration by wind shocks then allows to introduce the concept of thick cosmic-ray sources. The high-energy particles generated by such sources are very different from those associated wi作者: Foment 時間: 2025-3-25 19:12
,Nursing education — a luxury or necessity?, the origin of the excess of .Ne in the galactic cosmic rays (GCR) is correct, then other detectable anomalies in the GCR should occur. Wolf-Rayet stars make interesting amounts of .A1 (Dearborn and Blake 1985) which may account, at least in part, for the gamma-ray observations of Mahoney et al. (19作者: 水獺 時間: 2025-3-25 23:11 作者: 辭職 時間: 2025-3-26 02:31 作者: STANT 時間: 2025-3-26 06:23 作者: 盡責(zé) 時間: 2025-3-26 12:05
Psychiatric Aspects of Suicide in BudapestThe current system might resemble an electrical circuit with a voltage source (black hole and accretion disc) coupled to a load (cosmic-ray beam) and a low impedance element (ambient conducting medium). Beam particles can be accelerated to 10. provided that the beam channel medium behaves like an in作者: Postmenopause 時間: 2025-3-26 14:03
https://doi.org/10.1007/978-1-349-15220-9ium that is stable against Parker type instabilities. Equilibrium configurations considered in the past were found to be unstable as a consequence of simplifying assumptions, which are inconsistent with recent observations.作者: 拍翅 時間: 2025-3-26 18:09
Carleton J. Phillips,Bernard Tandlerht produced by the cascade particles in the earth’s atmosphere can be received at ground. For energies greater than 10. eV the particles of the cascade can be measured by detector arrays. The flux sensitivities of typical installations are presented.作者: Vo2-Max 時間: 2025-3-26 23:00 作者: Paraplegia 時間: 2025-3-27 02:41 作者: flourish 時間: 2025-3-27 08:39
Elling Prediction in Ocular Pursuit,ffects induced in frozen gases by impinging ions because they constitute the solid base for any reliable astrophysical application. We show the important role played in giant molecular clouds by cosmic rays for the production of molecular hydrogen, the cornerstone of interstellar chemistry. A method作者: 和平主義者 時間: 2025-3-27 09:36
978-94-010-8286-0D. Reidel Publishing Company, Dordrecht, Holland 1988作者: 幼稚 時間: 2025-3-27 14:33 作者: HALO 時間: 2025-3-27 18:42 作者: 一小塊 時間: 2025-3-28 01:55
An Assessment of Software Sneak Analysision. Young, bright shell remnants generally have spectral indices α larger than the 0.5 expected from basic shock acceleration theory. Fainter, older shell remnants have a wide range of α. Evidence on whether or not particle acceleration is continuing in SNRs is also discussed.作者: 成份 時間: 2025-3-28 02:52
Developments in Plant and Soil Sciencesl aspect of the possible acceleration mechanism. This investigation is made on the basis of the vacuum field of an orthogonal rotator. Effects of special relativity and classical radiation theory are taken into account. Results are discussed in terms of the “critical surface” and “acceleration boundary”.作者: Ischemic-Stroke 時間: 2025-3-28 07:41 作者: Decimate 時間: 2025-3-28 11:18 作者: 白楊魚 時間: 2025-3-28 17:39
Particle Acceleration in Galactic Supernova Remnants,ion. Young, bright shell remnants generally have spectral indices α larger than the 0.5 expected from basic shock acceleration theory. Fainter, older shell remnants have a wide range of α. Evidence on whether or not particle acceleration is continuing in SNRs is also discussed.作者: 哭得清醒了 時間: 2025-3-28 21:12 作者: anesthesia 時間: 2025-3-28 23:40 作者: placebo 時間: 2025-3-29 06:54
VHE and UHE Gamma Ray Observations by Ground Based Detectors,ht produced by the cascade particles in the earth’s atmosphere can be received at ground. For energies greater than 10. eV the particles of the cascade can be measured by detector arrays. The flux sensitivities of typical installations are presented.作者: Friction 時間: 2025-3-29 10:37
https://doi.org/10.1007/978-94-009-4025-3active galactic nuclei; astronomy; astrophysics; cosmic ray; earth; heliosphere; observatory; radio astrono作者: 使聲音降低 時間: 2025-3-29 14:02 作者: FAST 時間: 2025-3-29 18:13
Living-Donor Liver Transplantation in TaiwanThe quartet of isotopes of hydrogen(H) and helium(He) are the four most abundant species in the arriving cosmic radiation. In this paper, a brief summary of the spectra snd propagation of these species is given. The reader is referred to Beatty (1986) for a more detailed discussion.作者: 閑逛 時間: 2025-3-29 21:03
Preference Revelation and Public Goods,Recent γ-ray studies of the distribution of cosmic rays throughout the Galaxy are discussed based on the observations obtained with the .-2 .-B satellites. For reasons addressed in this paper the picture arising from recent analyses of both data bases differs from the one generally advocated in the past.作者: 殘酷的地方 時間: 2025-3-30 02:00 作者: Etymology 時間: 2025-3-30 04:32
An Overview of Cosmic Ray Research: Composition, Acceleration and Propagation,An overview of Cosmic Ray Research and its relation to other areas of High Energy Astrophysics is presented. Particular attention is paid to providing a summary of current results on the composition, acceleration and propagation of the cosmic radiation — topics which will be discussed in greater detail in other papers in this volume.作者: Regurgitation 時間: 2025-3-30 09:09
Galactic Cosmic Ray Hydrogen and Helium,The quartet of isotopes of hydrogen(H) and helium(He) are the four most abundant species in the arriving cosmic radiation. In this paper, a brief summary of the spectra snd propagation of these species is given. The reader is referred to Beatty (1986) for a more detailed discussion.作者: micronized 時間: 2025-3-30 16:00
Gamma-Ray Views on the Galactic Cosmic-Ray Distribution,Recent γ-ray studies of the distribution of cosmic rays throughout the Galaxy are discussed based on the observations obtained with the .-2 .-B satellites. For reasons addressed in this paper the picture arising from recent analyses of both data bases differs from the one generally advocated in the past.作者: 積云 時間: 2025-3-30 16:59 作者: 恩惠 時間: 2025-3-30 22:16 作者: Palpitation 時間: 2025-3-31 03:25
Current Issues in International Tradeyear is about 10. with a mean energy near 10. eV. The above huge power output and number of particles accelerated is likely to be provided by shock waves of expanding supernova remnants ploughing into stellar wind zones. After acceleration, cosmic rays are confined for about 10. years in the Galacti作者: Obedient 時間: 2025-3-31 07:46
Current Issues in Labour Economicscement, we see that the cosmic ray source is not dominated by the r-process up through the 50’s as evidenced by the Sr/Rb ratio and by the abundance of Sn and Ba. In addition the actinides are not greatly enhanced, ruling out freshly synthesized r-process production as the primary source of the heav作者: Encoding 時間: 2025-3-31 11:33 作者: 富足女人 時間: 2025-3-31 14:55 作者: Prostaglandins 時間: 2025-3-31 19:17 作者: harangue 時間: 2025-4-1 00:54 作者: excursion 時間: 2025-4-1 02:06 作者: 附錄 時間: 2025-4-1 09:21 作者: 水槽 時間: 2025-4-1 11:14
Stars and Cosmic Rays,ouds: they excite giant HII regions, inside which they create large wind cavities. The possibility of particle acceleration by wind shocks then allows to introduce the concept of thick cosmic-ray sources. The high-energy particles generated by such sources are very different from those associated wi作者: Vaginismus 時間: 2025-4-1 17:41 作者: 輕觸 時間: 2025-4-1 19:29
Radio Astronomy and Cosmic Rays,possibly, or even probably, originates in supernovae and/or supernova remnants. Therefore in consideration of this electronic component, we review the general history and observed properties of supernovae with concentration on the more recent results or radio supernovae, the observed properties of s作者: 充足 時間: 2025-4-1 22:42
Particle Acceleration in Galactic Supernova Remnants,ion. Young, bright shell remnants generally have spectral indices α larger than the 0.5 expected from basic shock acceleration theory. Fainter, older shell remnants have a wide range of α. Evidence on whether or not particle acceleration is continuing in SNRs is also discussed.作者: Debark 時間: 2025-4-2 04:23 作者: paradigm 時間: 2025-4-2 08:04
Conditions for Acceleration of Super-High Energy Cosmic Rays in Active Galactic Nuclei,The current system might resemble an electrical circuit with a voltage source (black hole and accretion disc) coupled to a load (cosmic-ray beam) and a low impedance element (ambient conducting medium). Beam particles can be accelerated to 10. provided that the beam channel medium behaves like an in作者: 圣歌 時間: 2025-4-2 13:16
