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標題: Titlebook: Origin of Cosmic Rays; Giancarlo Setti,Gianfranco Spada,Arnold W. Wolfend Book 1981 International Astronomical Union 1981 active galactic [打印本頁]

作者: foresight    時間: 2025-3-21 17:52
書目名稱Origin of Cosmic Rays影響因子(影響力)




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作者: Canopy    時間: 2025-3-21 22:46
978-90-277-1272-1International Astronomical Union 1981
作者: 恫嚇    時間: 2025-3-22 01:16

作者: AVOID    時間: 2025-3-22 05:05
International Astronomical Union Symposiahttp://image.papertrans.cn/o/image/704603.jpg
作者: Allure    時間: 2025-3-22 09:18
https://doi.org/10.1007/978-94-009-8475-2active galactic nuclei; astrophysics; cosmic ray; heliosphere; interstellar matter; quasar; star; star form
作者: 不合    時間: 2025-3-22 14:40
The Origin of Cosmic Rays (Introductory Remarks),The field of study, which by tradition is still called ‘the problem of cosmic ray origin’, is now at a watershed, at a turning point. For this reason the time chosen for the present Symposium is especially suited.
作者: Carcinogenesis    時間: 2025-3-22 21:03

作者: 充滿人    時間: 2025-3-22 22:07

作者: 不可思議    時間: 2025-3-23 03:58
CR-39 Plastic Track Detector Experiment for Measurement of Charge Composition of Primary Cosmic Rays of stack assembly was adopted for these modules: one consisting of ‘pure’ CR-39 plastic track detector: the next one, a composite assembly of CR-39 with three layers of 600 micron thick nuclear emulsions: and the last one with CR-39 and Lexan Polycarbonate. The payload was flown successfully in Ju
作者: 強所    時間: 2025-3-23 07:32
Interstellar and Intracluster Tunnels and Acceleration of High-Energy Cosmic Rays,ed by single sources into interstellar space undergo momentum diffusion by stochastic interaction with long wavelength MHD perturbations; small wavelength modes provide pitchangle scatterings. These MHD perturbations, A Ifvèn and fast magnetosonic waves, are generated by the dynamic interaction of s
作者: instate    時間: 2025-3-23 12:22

作者: nugatory    時間: 2025-3-23 14:56

作者: Postmenopause    時間: 2025-3-23 20:47

作者: creatine-kinase    時間: 2025-3-24 00:08
R. J. Protheroe,J. F. Ormes,G. M. Comstockcontinue to focus on these broad discriminations, at which it can do very well, thereby possibly offering the close-to-100% success that most NLP seemingly requires, with the possible exception of very fine questions of target word choice in MT. This proposal can be seen as reorienting WSD to what i
作者: Felicitous    時間: 2025-3-24 05:41
Richard I. Epsteincontinue to focus on these broad discriminations, at which it can do very well, thereby possibly offering the close-to-100% success that most NLP seemingly requires, with the possible exception of very fine questions of target word choice in MT. This proposal can be seen as reorienting WSD to what i
作者: HIKE    時間: 2025-3-24 06:37
Giancarlo Setti,Gianfranco Spada,Arnold W. Wolfend
作者: 創(chuàng)造性    時間: 2025-3-24 13:28
1743-9213 husiasm and this book contains the proceedings of the ensuing Symposium, (styled IUPAP/ IAU Symposium No. 94) which was held in Bologna from 11th - 14th June 19978-90-277-1272-1978-94-009-8475-2Series ISSN 1743-9213 Series E-ISSN 2352-2186
作者: Chauvinistic    時間: 2025-3-24 16:16

作者: 漂浮    時間: 2025-3-24 20:32

作者: 小口啜飲    時間: 2025-3-25 00:15

作者: 省略    時間: 2025-3-25 04:28

作者: stratum-corneum    時間: 2025-3-25 09:51

作者: Alienated    時間: 2025-3-25 12:10

作者: Debrief    時間: 2025-3-25 19:08

作者: graphy    時間: 2025-3-25 23:27
Isotopes of Cosmic Ray Elements from Neon to Nickel,an and Waddington (1975), Young (1979), measures elemental charge from scintillation and Cherenkov signals and mass from Cherenkov and total energy determined from a measure of residual range in nuclear emulsion. The charge resolution obtained ranged from 0.19 to 0.21 charge units between neon and n
作者: Respond    時間: 2025-3-26 04:11
Wolf Rayet Stars and the Origin of the 22Ne Excess in Cosmic Rays,ould be influential in the bulk energization of the local cosmic radiation (Cassé and Paul, 1980). Since wind acceleration is not supposed to accelerate thermal particles, a continuous injection of low energy particles (E ~ 1 to 10 MeV/n) is required. We keep open the possibility that these particle
作者: brachial-plexus    時間: 2025-3-26 04:51
CR-39 Plastic Track Detector Experiment for Measurement of Charge Composition of Primary Cosmic Rayormation concerning their origin, acceleration and interstellar propagation. In recent years solid state nuclear track detectors have been employed extensively to study heavy primary cosmic rays. Plastic track detectors necessarily have large geometric factors for heavy primaries, and a continuous s
作者: dapper    時間: 2025-3-26 10:14
Supernova and Cosmic Rays, astronomy and high energy astrophysics, but the theoretical explanation of SN involves virtually every branch of physics. Supernovae, however, offer more than a challenging physics problem because SN are involved in the origin of most of the heavy elements, are the birthplaces of neutron stars, pul
作者: 過剩    時間: 2025-3-26 13:33
What Can We Learn about Cosmic Rays from the UV, Optical, Radio and X-ray Observations of Supernovaeration of high energy particles. So far only optical information about SNe has been available and from it there is no direct evidence of Cosmic Rays. It is not surprising then that models of Cosmic Ray production are still rich in free parameters. On April 19th 1979 a very bright (~12 mag) SN, labe
作者: 碎石頭    時間: 2025-3-26 18:51

作者: 制度    時間: 2025-3-26 22:32
Diffusion of High Energy Cosmic Rays from the Virgo Cluster,a of Extragalactic sources. The characteristic features to be explained by any origin model are: the flattening of the energy spectrum above 10. eV and the apparent presence of a directional anisotropy which increases systematically with energy.
作者: subordinate    時間: 2025-3-27 01:48

作者: Keshan-disease    時間: 2025-3-27 05:38
Interstellar and Intracluster Tunnels and Acceleration of High-Energy Cosmic Rays,to 10. eV, corresponding to extragalactic processes (Kiràly et al. 1979). However the continuity of the spectrum indicates that the physical mechanisms must be correlated. In the global energetics the spectral range above 10. eV is irrelevant and the bulk of C R energy is actually provided by supern
作者: 前面    時間: 2025-3-27 09:58
Features of the High Energy Electron Spectrum,rger than those obtained by other experimental devices. (Taira et al., 1979, Nishimura et al., 1980). The total exposure is now almost 6 m.-day-str., including the recent exposure at Palestine, Texas in May 1980, and it is now quite possible to extend observations of the electron spectrum into the T
作者: 柏樹    時間: 2025-3-27 14:08

作者: 顧客    時間: 2025-3-27 20:52
Propagation Studies Related to the Origin of Cosmic Rays,f the methods for demodulating the effects of the solar wind on the spectra of particles, we describe an accurate method for correcting for spallation effects on the cosmic-ray nuclei during their transport from the sources subsequent to their acceleration. We present the composition of cosmic rays
作者: 有危險    時間: 2025-3-27 22:23

作者: 勛章    時間: 2025-3-28 04:45
Are Stellar Flares and the Galactic Cosmic Rays Related?,-relativistic, super-thermal particles which are subsequently boosted to cosmic ray energies by some other mechanism, perhaps related to supernovae (eg. Cassé and Goret, 1978). Two-stage models in which the injection and re-acceleration processes are uncorrelated are apparently untenable because the
作者: 史前    時間: 2025-3-28 08:11

作者: Osteoporosis    時間: 2025-3-28 14:22

作者: confide    時間: 2025-3-28 15:14
,The Charge and Isotopic Composition of Z ≥ 10 Nuclei in the Cosmic Ray Source,se as well as the semi empirical parameters used for the unmeasured cross sections is no better than ± 10–15%. As a result the actual source abundances of these nuclei can only be deduced to an accuracy of ± 2–3% of the Fe abundance.
作者: 出汗    時間: 2025-3-28 22:12
Supernova and Cosmic Rays,sars and probably black holes, control the structure of the interstellar medium, may be responsible for the birth of new stars (and possibly our own solar system), and, of greatest concern in this paper, are involved either directly or indirectly in the origin of the galactic cosmic rays.
作者: 誓言    時間: 2025-3-29 02:13
On the Detection of Heavy Primaries Above 1014 eV,dy of hadronic interactions above 10. eV. A recent EAS experiment (Goodman et al., 1979) suggests the possibility that the spectrum becomes increasingly rich in heavy nuclei as the total energy per nucleus approaches 10. eV. Above that energy the overall spectrum steepens and the question of composition is almost completely open.
作者: SSRIS    時間: 2025-3-29 03:59

作者: 投射    時間: 2025-3-29 08:44
Review of Cosmic Rays,should not be surprised that the origin of this radiation and its behavior is likely to involve a variety of different physical phenomena. Also, the spectrum of cosmic rays has two dimensions, one in energy, and one in the species of the particles.
作者: Alienated    時間: 2025-3-29 13:05
Isotopes in Galactic Cosmic Rays,ven three different nucleosynthesis mechanisms are required to account for the species .Fe, .Fe, .Fe. For carbon, nitrogen and oxygen the problem is that the spallation corrections are large compared to the solar system ratios but nevertheless the present upper limits are not in contradiction with the solar system ratios (fig. 1).
作者: notification    時間: 2025-3-29 18:54
What Can We Learn about Cosmic Rays from the UV, Optical, Radio and X-ray Observations of Supernova1979c was followed quite intensively in the optical and UV (with IUE) regions of the spectrum as well as observed at radio and X-ray frequencies. A detailed account of these observations is in press (Panagia et al. 1980). Here we summarize only very briefly the results relevant to the present discussion.
作者: obsession    時間: 2025-3-29 21:35

作者: Panther    時間: 2025-3-30 02:27
Very High Energy Cosmic Rays,ropy appearing to be correlated with features of the spectrum. Detailed interpretation of this information awaits conclusive evidence regarding the composition of these cosmic rays. New results and prospective new results on the composition are described and discussed.
作者: 無目標    時間: 2025-3-30 04:23
Features of the High Energy Electron Spectrum,including the recent exposure at Palestine, Texas in May 1980, and it is now quite possible to extend observations of the electron spectrum into the TeV region with reliable accuracy in the next few years.
作者: Isometric    時間: 2025-3-30 11:37

作者: Odyssey    時間: 2025-3-30 13:14
Isotopes of Cosmic Ray Elements from Neon to Nickel,from 0.40 to 0.70 amu for A between 20 and 60 amu. This was not adequate to uniquely resolve neighboring mass peaks in many cases, but was adequate to draw a number of conclusions regarding many of the more abundant elements.
作者: 收集    時間: 2025-3-30 17:05
Book 1981s most workers in the cosmic ray field were interested in the Nuclear Physical aspect of the particle beam and many important dis- coveries were made, notably the identification of the positron, the muon, the pion and the strange particles. More recently however, em- phasis has changed to the Astrop
作者: 冰雹    時間: 2025-3-30 23:56

作者: 高度贊揚    時間: 2025-3-31 03:46

作者: 有花    時間: 2025-3-31 06:26
https://doi.org/10.1007/978-3-662-62050-2les in transit. Brain fluids (CSF and brain interstitial fluid) are secreted, flow through particular routes and then drain back into the venous system; this fluid turnover aids central homeostasis and also affects CNS drug concentration. Several CNS pathologies involve changes in the barrier layers
作者: jettison    時間: 2025-3-31 11:21

作者: heartburn    時間: 2025-3-31 15:26

作者: seduce    時間: 2025-3-31 21:23
Preservation of cultural heritage: the design of low-energy archival storagerheben. Für Kritik und Vorschl?ge zur Verbesserung dieses Buches sind wir sehr dank- bar. An dieser Stelle m?chten wir Herrn Dr. R.Amann für seine Beurteilung des Roh- skriptes und Aufforderung zur Ver?ffentlic978-3-662-09750-2
作者: 軟膏    時間: 2025-4-1 01:27
,The Anti-de Sitter Proof of Thurston’s Earthquake Theorem,is a (left or right) earthquake. The purpose of these notes is to provide a proof of Thurston’s earthquake theorem, using the bi-invariant geometry of the Lie group ., which is also called Anti-de Sitter three-space. The involved techniques are elementary, and no background knowledge is assumed apart from some two-dimensional hyperbolic geometry.
作者: Brain-Imaging    時間: 2025-4-1 03:06
Vorsorgende Umweltpolitik,das sind Handlungsmaxime, die sich aus der Analyse der Umweltproblematik ergeben. In der allgemeinen politischen Diskussion unserer Tage werden sie dem Konzept des ., dem Leitbild einer dauerhaft sozial- und umweltgerechten Entwicklung, zugeordnet.
作者: HUMP    時間: 2025-4-1 07:10





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