標(biāo)題: Titlebook: Cosmic Rays and Earth; Proceedings of an IS J. W. Bieber,E. Eroshenko,R. Kallenbach Conference proceedings 2000 Springer Science+Business M [打印本頁(yè)] 作者: commotion 時(shí)間: 2025-3-21 18:31
書(shū)目名稱Cosmic Rays and Earth影響因子(影響力)
書(shū)目名稱Cosmic Rays and Earth影響因子(影響力)學(xué)科排名
書(shū)目名稱Cosmic Rays and Earth網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Cosmic Rays and Earth網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Cosmic Rays and Earth被引頻次
書(shū)目名稱Cosmic Rays and Earth被引頻次學(xué)科排名
書(shū)目名稱Cosmic Rays and Earth年度引用
書(shū)目名稱Cosmic Rays and Earth年度引用學(xué)科排名
書(shū)目名稱Cosmic Rays and Earth讀者反饋
書(shū)目名稱Cosmic Rays and Earth讀者反饋學(xué)科排名
作者: Medicaid 時(shí)間: 2025-3-21 22:59 作者: 無(wú)思維能力 時(shí)間: 2025-3-22 01:40 作者: Panacea 時(shí)間: 2025-3-22 05:15
erplanetary medium. Such regions, and the shocks which they may generate, have pronounced effects on cosmic ray densities both locally and at some distance away. These energetic particle effects can often be used to identify CMEs in the interplanetary medium, where they are usually called ‘ejecta’. 作者: 中國(guó)紀(jì)念碑 時(shí)間: 2025-3-22 09:18
g topics are discussed: observations of the cosmic ray modulation at the Earth and main characteristics of the accumulated experimental data; manifestations of the solar magnetic cycle in cosmic rays; the effect of hysteresis and its relation to the size of the heliosphere; the rigidity spectrum of 作者: gustation 時(shí)間: 2025-3-22 14:40
erates its own detectors and offers the opportunity to extend the cosmic-ray records over much longer time scales. Two different types of ‘natural detectors’ can be distinguished. The first is based on long lived radionuclides that are produced by cosmic-ray interactions in the atmosphere and subseq作者: gustation 時(shí)間: 2025-3-22 18:02
ntal problems of modern astrophysics. It is the aim of this paper to review new developments in the understanding of mechanisms involved in the scattering of charged particles by magnetic field fluctuations. Special emphasis is given to a comparison of transport parameters determined from the modeli作者: Axillary 時(shí)間: 2025-3-23 00:12
ons, initiated in the solar atmosphere, affect galactic cosmic rays. In some cases their influence on the cosmic ray intensity results in data signatures that can possibly be used to predict geomagnetic storm onsets. Case studies illustrating the complexity of the cosmic ray effects and related geom作者: 精確 時(shí)間: 2025-3-23 05:21
ship between the two, it is expected and found that the Earth’s temperature follows more closely decade variations in cosmic ray flux than other solar activity parameters. If the relationship is real the state of the Heliosphere affects the Earth’s climate.作者: 修改 時(shí)間: 2025-3-23 07:22 作者: 佛刊 時(shí)間: 2025-3-23 12:59
itors, muon telescope systems use coincidence techniques to obtain directional information about the arriving particle. Neutron monitor observations require simple corrections for pressure variations to compensate for the varying mass of atmospheric absorber over a site. In contrast, muon observatio作者: VAN 時(shí)間: 2025-3-23 14:15
Transferring Tests Across Web Applicationsability of cosmic radiation data from the early years to the present time. Information on the worldwide network of neutron monitor stations and the availability of these cosmic radiation records is included.作者: happiness 時(shí)間: 2025-3-23 20:19 作者: 損壞 時(shí)間: 2025-3-23 22:17
Andrea Gallidabino,Cesare Pautassosent about half of these are still active. Many of the original questions about the production of atmospheric secondaries, geomagnetic effects, and neutron monitor response in general, have been settled satisfactorily. Due to their long-term reliability and automated data acquisition, the remaining 作者: legitimate 時(shí)間: 2025-3-24 05:25
Form Filling Based on Constraint Solvingem is that the trajectory-tracing process involves using mathematical equations that have ‘no solution in closed form’. This difficulty has forced researchers to use the ‘brute force’ technique of numerical integration of many individual trajectories to ascertain the behavior of trajectory families 作者: HILAR 時(shí)間: 2025-3-24 09:55
Andrea Gallidabino,Cesare Pautassoy cosmic rays. Simpson (1948) discovered that the latitude variation of the secondary hadronic component was considerably larger than the muon component suggesting the response of a neutron monitor is more sensitive to lower energies in the primary spectrum. The different methods of determining the 作者: GRIPE 時(shí)間: 2025-3-24 12:49 作者: Gingivitis 時(shí)間: 2025-3-24 15:32
Cosmic Rays and Earth978-94-017-1187-6Series ISSN 1385-7525 作者: BAIL 時(shí)間: 2025-3-24 22:21
site of solar flares that are responsible for .-ray, .-ray and neutron emission and particles accelerated at high coronal altitudes and in interplanetary space by travelling disturbances such as coronal mass ejections. Special emphasis is placed on those particles directly or indirectly associated with neutron monitor signals.作者: Efflorescent 時(shí)間: 2025-3-25 03:02 作者: CRACY 時(shí)間: 2025-3-25 04:55
Transferring Tests Across Web Applicationsability of cosmic radiation data from the early years to the present time. Information on the worldwide network of neutron monitor stations and the availability of these cosmic radiation records is included.作者: 牢騷 時(shí)間: 2025-3-25 09:48 作者: 重畫(huà)只能放棄 時(shí)間: 2025-3-25 13:55 作者: 離開(kāi)可分裂 時(shí)間: 2025-3-25 18:49
Fifty Years of Cosmic Radiation Dataability of cosmic radiation data from the early years to the present time. Information on the worldwide network of neutron monitor stations and the availability of these cosmic radiation records is included.作者: 嚴(yán)厲譴責(zé) 時(shí)間: 2025-3-25 20:39
https://doi.org/10.1007/978-94-017-1187-6Neutron; atmosphere; cosmic ray; earth; geophysics; heliosphere; space weather作者: 歹徒 時(shí)間: 2025-3-26 01:37 作者: 不可侵犯 時(shí)間: 2025-3-26 08:19 作者: GROG 時(shí)間: 2025-3-26 09:09 作者: GUILT 時(shí)間: 2025-3-26 13:11 作者: SPALL 時(shí)間: 2025-3-26 17:36
m then on integrate the production of cosmogenic nuclides over the whole exposure time. The analysis of .Be in polar ice cores and .C in tree rings clearly reveals solar and geomagnetic modulation of the cosmic-ray flux on different time scales ranging from decades (11-year Schwabe cycle) to millennia.作者: 睨視 時(shí)間: 2025-3-26 22:53 作者: Aphorism 時(shí)間: 2025-3-27 03:44
Coronal Mass Ejections and Forbush Decreasessummarize the characteristics of CMEs, their effects on particles and the present understanding of the mechanisms involved which cause the particle effects. The role of CMEs in long term modulation will also be discussed.作者: Autobiography 時(shí)間: 2025-3-27 09:14 作者: 禮節(jié) 時(shí)間: 2025-3-27 11:51 作者: Lucubrate 時(shí)間: 2025-3-27 14:11 作者: accessory 時(shí)間: 2025-3-27 20:21 作者: essential-fats 時(shí)間: 2025-3-28 00:31
Cosmic Rays and Earth — A Summaryine temporal and spatial variations in our space environment. The resulting datasets represent the longest continuous, high time resolution series of particle radiation measurement in space science. At present, the neutron monitor network is complemented by spacecraft instrumentation to study solar-terrestrial correlated phenomena.作者: 宿醉 時(shí)間: 2025-3-28 04:29 作者: 藝術(shù) 時(shí)間: 2025-3-28 10:19 作者: linear 時(shí)間: 2025-3-28 13:19
The Cosmic Ray Nucleonic Component: The Invention and Scientific Uses of the Neutron Monitorplications were:.With the world-wide distribution of neutron monitor stations that are presently operating (~ 50) many novel investigations are still to be carried out, especially in collaborations with spacecraft experiments.作者: abduction 時(shí)間: 2025-3-28 15:51
Conference proceedings 2000ontribu- tions of all participants. Following a general summary of the workshop prepared by the editors, the volume leads off with a keynote article by Professor John Simpson describing his invention of the neutron monitor in 1948 and the early scientific discoveries made with this instrument.作者: EWE 時(shí)間: 2025-3-28 20:28 作者: 單挑 時(shí)間: 2025-3-28 22:57
osphere and describes models and software that have been developed that provide quantitative information about the cosmic radiation exposure at flight altitudes. The discussion is extended to include the cosmic radiation exposure to manned spacecraft.作者: Infraction 時(shí)間: 2025-3-29 06:39 作者: Range-Of-Motion 時(shí)間: 2025-3-29 08:31 作者: Mangle 時(shí)間: 2025-3-29 12:53
The Cosmic Ray Nucleonic Component: The Invention and Scientific Uses of the Neutron Monitoreonic component cascade in the atmosphere had a huge geomagnetic latitude dependence. For example, between 0° and 60° this dependence was a ~ 200–400% effect — depending on altitude — thus opening the opportunity to measure the intensity changes in the arriving cosmic-ray nuclei down to ~ 1–2 GeV nu作者: adhesive 時(shí)間: 2025-3-29 18:42 作者: 取消 時(shí)間: 2025-3-29 20:57
Coronal Mass Ejections and Forbush Decreaseserplanetary medium. Such regions, and the shocks which they may generate, have pronounced effects on cosmic ray densities both locally and at some distance away. These energetic particle effects can often be used to identify CMEs in the interplanetary medium, where they are usually called ‘ejecta’. 作者: cutlery 時(shí)間: 2025-3-30 00:24 作者: 模仿 時(shí)間: 2025-3-30 04:52 作者: 變化無(wú)常 時(shí)間: 2025-3-30 09:40
Particle Scattering by Magnetic Fieldsntal problems of modern astrophysics. It is the aim of this paper to review new developments in the understanding of mechanisms involved in the scattering of charged particles by magnetic field fluctuations. Special emphasis is given to a comparison of transport parameters determined from the modeli作者: RODE 時(shí)間: 2025-3-30 13:16 作者: MENT 時(shí)間: 2025-3-30 18:28 作者: 敵手 時(shí)間: 2025-3-30 22:59
Cosmic Ray Implications for Human Healthches the Earth and its environment is a function of solar cycle, altitude and latitude. The possible effect of naturally occurring cosmic radiation on airplane crews and space flight personal is a subject of current study. This paper discusses the variables controlling the cosmic ray flux in the atm作者: itinerary 時(shí)間: 2025-3-31 03:29 作者: Rheumatologist 時(shí)間: 2025-3-31 08:24
Fifty Years of Cosmic Radiation Dataability of cosmic radiation data from the early years to the present time. Information on the worldwide network of neutron monitor stations and the availability of these cosmic radiation records is included.作者: allergy 時(shí)間: 2025-3-31 12:11
Integration of Neutron Monitor Data with Spacecraft Observations: A Historical Perspectivetions of the Sun as a transient source of high energy particles and laid the foundation of our early concepts of a heliosphere. The first major impact of the arrival of the Space Age in 1957 on our understanding of cosmic rays came from spacecraft operating beyond the confines of our magnetosphere. 作者: 牌帶來(lái) 時(shí)間: 2025-3-31 15:23 作者: evince 時(shí)間: 2025-3-31 20:29
Magnetospheric Models and Trajectory Computationsem is that the trajectory-tracing process involves using mathematical equations that have ‘no solution in closed form’. This difficulty has forced researchers to use the ‘brute force’ technique of numerical integration of many individual trajectories to ascertain the behavior of trajectory families 作者: 摘要 時(shí)間: 2025-4-1 01:07 作者: unstable-angina 時(shí)間: 2025-4-1 03:59 作者: Liability 時(shí)間: 2025-4-1 09:05 作者: Fermentation 時(shí)間: 2025-4-1 11:42 作者: foodstuff 時(shí)間: 2025-4-1 17:43
Integration of Neutron Monitor Data with Spacecraft Observations: A Historical Perspectiventerpreting many of these new results..With the launch of IMP 6 in 1971, followed by a number of other spacecraft, long-term monitoring of low and medium energy galactic and anomalous cosmic rays and solar and interplanetary energetic particles, and the interplanetary medium were available on a cont作者: 樹(shù)上結(jié)蜜糖 時(shí)間: 2025-4-1 21:36
Design and Co-Ordination of Multi-Station International Neutron Monitor Networksn even distribution in longitude, at high altitude and near the equator. Steps have already been taken to improve the network with these goals in mind, and to standardize methods. This contribution describes some of these steps and suggests further strategies to achieve the most optimal network.作者: 自傳 時(shí)間: 2025-4-2 00:50
Magnetospheric Models and Trajectory Computationsion in space of various cosmic ray anisotropies. Unfortunately, cutoff rigidities are not simple parameters due to the chaotic behavior of the cosmic-ray trajectories in the cosmic ray penumbral region. As the computational problem becomes more manageable, there is still the issue of the accuracy of作者: Seminar 時(shí)間: 2025-4-2 04:02
