標(biāo)題: Titlebook: Cosmic Rays in the Heliosphere; Volume Resulting fro L. A. Fisk,J. R. Jokipii,K.-P. Wenzel Book 1998 Springer Science+Business Media Dordre [打印本頁] 作者: Fatuous 時間: 2025-3-21 20:01
書目名稱Cosmic Rays in the Heliosphere影響因子(影響力)
書目名稱Cosmic Rays in the Heliosphere影響因子(影響力)學(xué)科排名
書目名稱Cosmic Rays in the Heliosphere網(wǎng)絡(luò)公開度
書目名稱Cosmic Rays in the Heliosphere網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Cosmic Rays in the Heliosphere被引頻次
書目名稱Cosmic Rays in the Heliosphere被引頻次學(xué)科排名
書目名稱Cosmic Rays in the Heliosphere年度引用
書目名稱Cosmic Rays in the Heliosphere年度引用學(xué)科排名
書目名稱Cosmic Rays in the Heliosphere讀者反饋
書目名稱Cosmic Rays in the Heliosphere讀者反饋學(xué)科排名
作者: DOSE 時間: 2025-3-21 23:58 作者: 索賠 時間: 2025-3-22 01:52
Three-Dimensional Solar Modulation of Cosmic Rays and Anomalous Components in the Inner Heliospherehe first comprehensive exploration of modulation as a function of latitude from 80° S to 80° N heliographic latitude. Among the principal findings for the inner heliosphere are: a) the cosmic ray intensity depends only weakly on heliographic latitude; b) for the nuclear components, and especially fo作者: majestic 時間: 2025-3-22 07:23 作者: 解決 時間: 2025-3-22 12:23
Anomalous Cosmic Rays and Solar Modulationdinal and radial gradients of these particles exhibit a 22-year periodicity in concert with the reversal of the Sun’s magnetic field. The power-law index of the low energy portion of the energy spectrum of ACRs at the shock in 1996 appears to be ≤ ?1.3, suggesting that the strength of the solar wind作者: 坦白 時間: 2025-3-22 16:52
Cosmic Ray Electronsgative slope, which may in some way be related to electrons released from the magnetosphere of the planet Jupiter. If there is such a relationship, its nature is not established, and alternative explanations for the upturn exist. At higher energies, electrons are predominantly negatively charged, an作者: 坦白 時間: 2025-3-22 18:11
The Solar Wind — Inner Heliospheremission to the many low latitude inner heliosphere missions that preceded it. The two major omissions are the high latitude solar wind at solar maximum, which will he measured during the second Ulysses polar passages. and the solar wind near the Sun. which could he analyzed by a Solar Probe mission.作者: FRAUD 時間: 2025-3-22 21:29 作者: indifferent 時間: 2025-3-23 04:00
Magnetic Fields in the Inner Heliosphereake place in the solar wind. The division between the inner and outer regions of the heliosphere is the result of dynamic processes which form large scale structures with increasing heliocentric distance. The structure of the HMF is normally described in the reference frame based on Parker’s geometr作者: 積習(xí)難改 時間: 2025-3-23 09:26
Voyager Observations of the Magnetic Field in the Distant Heliospherend negative magnetic polarities are observed, and by the unipolar regions above and below the sector zone. Distinct corotating streams and interactions regions are found primarily in the sector zone during the declining phase of the solar cycle. Within a few AU, the streams and interaction regions a作者: Engaging 時間: 2025-3-23 09:48
The Theory of Anomalous Cosmic Raystion or the solar wind, and are subsequently accelerated to very high energies, greater than 1 GeV. Current thinking has the hulk of the acceleration to very-high energies taking place, by the mechanism of diffusive shock acceleration, at the termination shock of the solar wind. Detailed two-dimensi作者: 點燃 時間: 2025-3-23 16:19
Modeling of 3-D Corotating Cosmic-Ray Structures in the Heliospherecurrent sheet and Corotating Interaction Regions (CIRs). We find that present models can qualitatively account for the observed extension of recurrent 26-day cosmic-ray variations to high heliospheric latitudes if perpendicular diffusion is significant. The recurrent enhancement of low-energy (MeV) 作者: Scleroderma 時間: 2025-3-23 20:29 作者: 搖曳 時間: 2025-3-24 00:00
The Inner Heliosphere — Outer Heliosphere Comparison for Cosmic Ray Modulation 1996 at the end of solar cycle 22. These data come from the IMP spacecraft in the inner heliosphere and the Voyager and Pioneer spacecraft in the outer heliosphere. In the inner heliosphere, the cosmic ray intensities at all energies in 1996 have recovered to almost the same maximum values they had作者: resilience 時間: 2025-3-24 02:59
A Brief History of Recurrent Solar Modulation of the Galactic Cosmic Rays (1937–1990)that was believed to have its origin in recurrent variations of the geomagnetic field. However, with the introduction of neutron monitor analysis of the nucleonic component, it was shown in the 1940s and 1950s that this cosmic ray intensity variation arose from interplanetary dynamical phenomena. Be作者: 前奏曲 時間: 2025-3-24 08:52 作者: intangibility 時間: 2025-3-24 13:51 作者: 典型 時間: 2025-3-24 15:34
Recurrent Solar Modulation of the Galactic Cosmic Rays and the Anomalous Nuclear Component in Three nteraction region shocks. Also included are some unpublished measurements that will need to he taken into account in any model for the 26-day modulation phenomena. This report is a brief summary of the principal results from the solar wind, magnetic field and charged particle investigations, and their alternate interpretations.作者: Ferritin 時間: 2025-3-24 19:30
Cosmic Ray Electronsd it is probable that the difference in net charge sign from that of nuclei is responsible for many of the observed differences in the behavior of electrons and nuclei under modulation. A consistent picture of the cosmic positron abundance and its time variation may be emerging from the world dataset.作者: 枕墊 時間: 2025-3-25 02:47
1385-7525 the state of the field. Such is the case for the study of the behavior of cosmic rays in the heliosphere. We are just passing through solar minimum conditions, when the heliosphere has a well-ordered and relatively simple configuration. We have been fortunate to have an array of spacecraft - unprece作者: 大猩猩 時間: 2025-3-25 04:44
Structured On-the-Job Training Modulesm, which will he measured during the second Ulysses polar passages. and the solar wind near the Sun. which could he analyzed by a Solar Probe mission. Here, existing knowledge of the global solar wind in the inner heliosphere is summarized in the context of the new results from Ulysses.作者: ICLE 時間: 2025-3-25 10:59
Work Analysis Roles and Process magnetic field is enhanced in such regions, they are important for the study of modulation of cosmic rays. Unfortunately, direct observation of the enhanced magnetic field from Voyager 2 has been made difficult by spacecraft-associated noise since 1989.作者: Directed 時間: 2025-3-25 12:35 作者: concentrate 時間: 2025-3-25 15:59 作者: Cultivate 時間: 2025-3-25 22:06 作者: 易受刺激 時間: 2025-3-26 00:45
Conducting a Competency Analysis evidence that ACR oxygen is primarily multiply charged above ~ 20 MeV/nuc and primarily singly-charged below ti 16 MeV/nuc. The location of the termination shock was at ~ 65 AU in 1987 and ~ 85 AU in 1994.作者: Temporal-Lobe 時間: 2025-3-26 05:45 作者: defuse 時間: 2025-3-26 08:27
Anomalous Cosmic Rays and Solar Modulation evidence that ACR oxygen is primarily multiply charged above ~ 20 MeV/nuc and primarily singly-charged below ti 16 MeV/nuc. The location of the termination shock was at ~ 65 AU in 1987 and ~ 85 AU in 1994.作者: 等級的上升 時間: 2025-3-26 14:41 作者: 影響帶來 時間: 2025-3-26 19:17
The Solar Wind — Inner Heliospherem, which will he measured during the second Ulysses polar passages. and the solar wind near the Sun. which could he analyzed by a Solar Probe mission. Here, existing knowledge of the global solar wind in the inner heliosphere is summarized in the context of the new results from Ulysses.作者: 消瘦 時間: 2025-3-26 22:58
Voyager 2 Solar Wind Observations in the Outer Heliosphere magnetic field is enhanced in such regions, they are important for the study of modulation of cosmic rays. Unfortunately, direct observation of the enhanced magnetic field from Voyager 2 has been made difficult by spacecraft-associated noise since 1989.作者: 一加就噴出 時間: 2025-3-27 04:30 作者: ascetic 時間: 2025-3-27 07:26
Corotating Particle Events into the context of current heliospheric magnetic field models. The energetic particle signatures of CIRs throughout the regions of the heliosphere covered by the deep-space missions are reviewed. The CIRs accelerate these particles and at the saine time modulate both the high energy galactic cosmic rays and the anomalous cosmic rays.作者: 冬眠 時間: 2025-3-27 09:41
Work Analysis Roles and Processnteraction region shocks. Also included are some unpublished measurements that will need to he taken into account in any model for the 26-day modulation phenomena. This report is a brief summary of the principal results from the solar wind, magnetic field and charged particle investigations, and their alternate interpretations.作者: 側(cè)面左右 時間: 2025-3-27 17:13 作者: Hiatal-Hernia 時間: 2025-3-27 19:25 作者: DEBT 時間: 2025-3-27 22:24 作者: 種子 時間: 2025-3-28 04:02
The Theory of Anomalous Cosmic Rayscent improvements to this picture include the observation of multiply charged cosmic rays and the suggestion that some “preacceleration” of the initially ionized particles occurs in the inner heliosphere.作者: Infelicity 時間: 2025-3-28 07:19
The Modulation of Galactic Cosmic Rays in the Heliosphere: Theory and Modelsdicted. In the process the sophistication of models based on solving Parker’s equation has increased by orders of magnitude. A short review of the global modulation.of cosmic rays is given from a theoretical and modelling point of view.作者: 序曲 時間: 2025-3-28 11:37 作者: 倒轉(zhuǎn) 時間: 2025-3-28 15:46
Three-Dimensional Solar Modulation of Cosmic Rays and Anomalous Components in the Inner Heliospheretures in the solar wind and magnetic field; e) the surface of symmetry of the modulation in 1994–95 was offset about 10. south of the heliographic equator; f) the intensity of electrons and of low energy (< ~100 MeV) protons showed essentially no dependence on heliographic latitude.作者: Obedient 時間: 2025-3-28 22:28
Cosmic-Ray Modulation in the Heliospheree energy spectra of anomalous cosmic rays as a function of heliocentric distance..From solar minimum to solar maximum the long term modulation is principally a combination of two solar related phenomena, the cumulative effect of long-lived global merged interaction regions (GMIRs) and gradient and c作者: 心神不寧 時間: 2025-3-29 00:34 作者: NAV 時間: 2025-3-29 05:18 作者: 討厭 時間: 2025-3-29 09:13 作者: Suppository 時間: 2025-3-29 15:22 作者: 聽寫 時間: 2025-3-29 17:59 作者: Contracture 時間: 2025-3-29 23:04
https://doi.org/10.1007/978-3-319-94367-1e energy spectra of anomalous cosmic rays as a function of heliocentric distance..From solar minimum to solar maximum the long term modulation is principally a combination of two solar related phenomena, the cumulative effect of long-lived global merged interaction regions (GMIRs) and gradient and c作者: 產(chǎn)生 時間: 2025-3-30 01:43
Human Resource Development and Work Analysiso mid-latitudes; the polar regions of the heliosphere are dominated by uniform fast solar wind streams and large amplitude, long wavelength, mostly transverse magnetic fluctuations. Coronal Mass Ejections (CMEs) introduce transient variability into the large scale heliospheric structure and may domi作者: Alopecia-Areata 時間: 2025-3-30 05:24
National Occupational Standardsthe magnetic field and solar wind particles and largely controls the dynamical processes. During 1983 and 1994, corotating streams and corotating interaction regions were observed at 1 AU. Merged interaction regions were observed at ≈15 AU in 1983, but not at ≈45 AU during 1994. This result suggests作者: debouch 時間: 2025-3-30 11:04
Structured On-the-Job Training Modulest the same radius of 42 AU in 1987 and for anomalous cosmic rays this ratio is only 0.1–0.2. This suggests a dramatically different entry of particles into the heliosphere in the two cycles for both types of particles as well as significantly different particle flow characteristics in the outer heli作者: abduction 時間: 2025-3-30 16:02
Historiography of African Market Womenis occurs is unclear. Despite the apparent success of the theory, there is no single choice for the parameters which describe cosmic ray behavior, which can account for all of the observed temporal and spatial variations, spectra, and electron vs. ion behavior.作者: Pantry 時間: 2025-3-30 18:42 作者: 吊胃口 時間: 2025-3-30 22:24
Cosmic Rays in the Heliosphere978-94-017-1189-0Series ISSN 1385-7525 作者: Provenance 時間: 2025-3-31 03:10
https://doi.org/10.1007/978-3-319-94367-1y of the supersonic solar wind flow, the cause of these variations became apparent: the cosmic rays, in transit from the interstellar medium into the heliosphere must propagate upstream against the solar wind flow, which will reduced the cosmic ray flux and cause it to vary. That is, the cosmic-ray flux is modulated by the solar wind.作者: 啪心兒跳動 時間: 2025-3-31 08:27 作者: 吃掉 時間: 2025-3-31 10:58
Introductiony of the supersonic solar wind flow, the cause of these variations became apparent: the cosmic rays, in transit from the interstellar medium into the heliosphere must propagate upstream against the solar wind flow, which will reduced the cosmic ray flux and cause it to vary. That is, the cosmic-ray flux is modulated by the solar wind.作者: 偽造者 時間: 2025-3-31 13:40 作者: Coronary-Spasm 時間: 2025-3-31 19:34
Work Analysis Roles and Processl change dramatically models to account for the physical phenomena underlying the 26-day modulation of galactic cosmic rays and anomalous nuclear components and their propagation modes. These new findings also relate to the propagation of low energy nucleons and electrons accelerated by corotating i作者: 蠟燭 時間: 2025-4-1 00:40
Margaret Oliphant, Women and Money,he first comprehensive exploration of modulation as a function of latitude from 80° S to 80° N heliographic latitude. Among the principal findings for the inner heliosphere are: a) the cosmic ray intensity depends only weakly on heliographic latitude; b) for the nuclear components, and especially fo作者: cornucopia 時間: 2025-4-1 02:54
https://doi.org/10.1007/978-3-319-94367-1 rays over a period of time that now exceeds 25 years and extends to heliocentric distances beyond 65 AU. These data, when compared over consecutive 11 year solar cycles, clearly establishes the existence of a 22-year cosmic ray modulation cycle that is dominated by the 11-year solar activity cycle 作者: 貪心 時間: 2025-4-1 06:56
Conducting a Competency Analysisdinal and radial gradients of these particles exhibit a 22-year periodicity in concert with the reversal of the Sun’s magnetic field. The power-law index of the low energy portion of the energy spectrum of ACRs at the shock in 1996 appears to be ≤ ?1.3, suggesting that the strength of the solar wind作者: 彎腰 時間: 2025-4-1 11:33 作者: 條約 時間: 2025-4-1 15:14
Structured On-the-Job Training Modulesmission to the many low latitude inner heliosphere missions that preceded it. The two major omissions are the high latitude solar wind at solar maximum, which will he measured during the second Ulysses polar passages. and the solar wind near the Sun. which could he analyzed by a Solar Probe mission.
