作者: 思想靈活 時(shí)間: 2025-3-21 20:58
https://doi.org/10.1007/978-94-017-1179-1Corona; Heliosphere; Planet; Solar wind; solar作者: Exclude 時(shí)間: 2025-3-22 01:17 作者: intention 時(shí)間: 2025-3-22 04:38
across, carved out of the interstellar medium by the flow of gas. The solar wind flow can be quite complex, as for example during sunspot maximum, or relatively simple, as during sunspot minimum. Prior to and near sunspot minimum, the solar wind and heliosphere are observed to take on a relatively s作者: extract 時(shí)間: 2025-3-22 09:47
Northern Ireland: Wellbeing as a Vision,e solar wind, and is now generally believed to mark the boundary between solar wind which was originally slow when it left the Sun and solar wind which was originally fast. This paper summarises some important facts and open questions about the origin and nature of the boundary between fast and slow作者: 秘密會議 時(shí)間: 2025-3-22 13:50 作者: 秘密會議 時(shí)間: 2025-3-22 19:26 作者: aquatic 時(shí)間: 2025-3-23 01:14 作者: frugal 時(shí)間: 2025-3-23 02:40 作者: 我悲傷 時(shí)間: 2025-3-23 08:58
Vodafone Acquisition of Mannesmann,n various astrophysical settings. The heliosphere offers the best chance to study these poorly understood processes experimentally. We examine ion injection and pre-acceleration using measurements of the bulk and suprathermal solar wind, and pickup ions. Our most puzzling observation is that high-ve作者: 駁船 時(shí)間: 2025-3-23 12:27
nsport equation for energetic particles we discuss diffusive acceleration at the corotating shocks, stochastic acceleration within the interaction region, and the injection and acceleration of pickup ions at the corotating shocks.作者: libertine 時(shí)間: 2025-3-23 13:54 作者: excursion 時(shí)間: 2025-3-23 18:13
r conditions in the changing heliosphere. During the last four years, concentrated around the solar minimum period of solar cycle 22, the exploration of the solar polar regions by the joint ESA/NASA mission Ulysses revealed the three-dimensional behavior of cosmic rays in the inner and middle helios作者: Oversee 時(shí)間: 2025-3-23 22:16
Bulat Nasrulin,Muhammad Muzammal,Qiang Qustreams. Dynamic interaction of solar wind streams is a general feature of the heliospheric medium; when the sources of the solar wind streams are relatively stable, the interaction regions form a pattern which corotates with the Sun. The regions of origin of the high speed solar wind streams have b作者: sperse 時(shí)間: 2025-3-24 06:02
Bulat Nasrulin,Muhammad Muzammal,Qiang Quic particles. This report summarizes current understanding of those features and patterns, discusses how they can vary from case to case and with distance from the Sun and possible causes of those variations, presents an analytical model of the morphological features found in earlier qualitative mod作者: 為寵愛 時(shí)間: 2025-3-24 09:50
Xuechao Yang,Xun Yi,Surya Nepal,Fengling Han in early 1995, Ulysses observed a weaker CIR from early 1996 to mid-1997 in the northern hemisphere as it traveled back to the ecliptic at the orbit of Jupiter. These two CIRs are the observational basis of the investigation into the latitudinal structure of CIRs. The first CIR was caused by an ext作者: Apoptosis 時(shí)間: 2025-3-24 13:23 作者: 辯論 時(shí)間: 2025-3-24 17:09 作者: 牽連 時(shí)間: 2025-3-24 20:07 作者: 樹木中 時(shí)間: 2025-3-25 02:24
Bandar Alghamdi,Yue Xu,Jason Watsonon, and acceleration of particles associated with Corotating Interaction Regions (CIRs) is reviewed. This includes diffusive or first-order Fermi acceleration at oblique shocks, adiabatic deceleration in the solar wind, stochastic acceleration in Alfvén waves and oblique propagating magnetosonic wav作者: Angiogenesis 時(shí)間: 2025-3-25 06:42
Corotating Interaction Regions978-94-017-1179-1Series ISSN 1385-7525 作者: 颶風(fēng) 時(shí)間: 2025-3-25 07:37
Northern Ireland: Wellbeing as a Vision,s in plasma, magnetic field, and particles become more complex as observations are made at greater and greater distances. Pickup ions from charge exchange undoubtedly play an important role in the structure, but the full details are not yet understood.作者: ALTER 時(shí)間: 2025-3-25 15:35
nsport equation for energetic particles we discuss diffusive acceleration at the corotating shocks, stochastic acceleration within the interaction region, and the injection and acceleration of pickup ions at the corotating shocks.作者: apropos 時(shí)間: 2025-3-25 17:38 作者: ciliary-body 時(shí)間: 2025-3-26 00:02
Injection and Acceleration Processes in Corotating Interaction Regions: Theoretical Conceptsnsport equation for energetic particles we discuss diffusive acceleration at the corotating shocks, stochastic acceleration within the interaction region, and the injection and acceleration of pickup ions at the corotating shocks.作者: maintenance 時(shí)間: 2025-3-26 01:06 作者: LAVA 時(shí)間: 2025-3-26 05:33
Northern Ireland: Wellbeing as a Vision,h was originally fast. This paper summarises some important facts and open questions about the origin and nature of the boundary between fast and slow solar wind near the Sun, the evolution of stream interfaces with heliocentric distance in the inner heliosphere, and their relationship.作者: 粘土 時(shí)間: 2025-3-26 11:44
ffusion, or, in a recent model for the heliospheric magnetic field, by direct magnetic connection. The commonalties and differences of these two mechanisms are considered, and the need for future observations and modeling efforts are discussed.作者: 商業(yè)上 時(shí)間: 2025-3-26 14:39 作者: 傾聽 時(shí)間: 2025-3-26 20:21 作者: 小蟲 時(shí)間: 2025-3-26 23:15
Bandar Alghamdi,Yue Xu,Jason Watsonleration at oblique shocks, adiabatic deceleration in the solar wind, stochastic acceleration in Alfvén waves and oblique propagating magnetosonic waves, and shock surfing as possible injection mechanism to discriminate pickup ions from solar wind ions.作者: 卷發(fā) 時(shí)間: 2025-3-27 04:39 作者: enmesh 時(shí)間: 2025-3-27 07:13 作者: GNAW 時(shí)間: 2025-3-27 12:16 作者: graphy 時(shí)間: 2025-3-27 13:41
Origin, Injection, and Acceleration of CIR Particles: Observationse of heliolatitudes. With this more complete observational picture established, this review is the basis to consider the status of theoretical models on origin, injection, and acceleration of CIR particles reported by Scholer, Mann . (1999) in this volume.作者: GROSS 時(shí)間: 2025-3-27 17:51
Origin, Injection, and Acceleration of CIR Particles: Theoryleration at oblique shocks, adiabatic deceleration in the solar wind, stochastic acceleration in Alfvén waves and oblique propagating magnetosonic waves, and shock surfing as possible injection mechanism to discriminate pickup ions from solar wind ions.作者: 四海為家的人 時(shí)間: 2025-3-28 00:42 作者: 美麗的寫 時(shí)間: 2025-3-28 04:24
Acquisitions by Royal Dutch Shell, acceleration process. This paper summarizes properties of energetic particles in CIRs as known through the early 1990s, prior to the launch of the Ulysses, and WIND spacecraft, whose new results are presented in Kunow, Lee .. (1999) in this volume.作者: mastoid-bone 時(shí)間: 2025-3-28 07:08
Yumeng Fu,Wei Wang,Hao Fu,Wu Yang,Dan Yin in global cosmic ray modulation. We also discuss some outstanding questions related to the origin of non-dispersive quasi-periodic particle enhancements associated with CIRs and their successors in the outer heliosphere.作者: 獨(dú)特性 時(shí)間: 2025-3-28 11:35
Ildar Nurgaliev,Muhammad Muzammal,Qiang Quties .. latitude do not support enhanced latitude transport. This chapter contains a summary of the interaction between observations and models for the effects of CIRs, and its impact on the understanding of the physics of modulation.作者: 冒號 時(shí)間: 2025-3-28 18:13 作者: 沒有希望 時(shí)間: 2025-3-28 20:35 作者: 鄙視讀作 時(shí)間: 2025-3-28 23:05 作者: Insul島 時(shí)間: 2025-3-29 06:23 作者: 符合你規(guī)定 時(shí)間: 2025-3-29 10:25 作者: Agronomy 時(shí)間: 2025-3-29 11:25 作者: 推遲 時(shí)間: 2025-3-29 15:37
Solar Origin and Interplanetary Evolution of Stream Interfacese solar wind, and is now generally believed to mark the boundary between solar wind which was originally slow when it left the Sun and solar wind which was originally fast. This paper summarises some important facts and open questions about the origin and nature of the boundary between fast and slow作者: BYRE 時(shí)間: 2025-3-29 20:21
Formation and Evolution of Corotating Interaction Regions and Their Three Dimensional Structureifferent speeds to become radially aligned. Compressive interaction regions are produced where high-speed wind runs into slower plasma ahead. When the flow pattern emanating from the Sun is roughly time-stationary these compression regions form spirals in the solar equatorial plane that corotate wit作者: Aesthete 時(shí)間: 2025-3-30 01:19 作者: 召集 時(shí)間: 2025-3-30 05:02 作者: Initiative 時(shí)間: 2025-3-30 08:22
CIR Associated Energetic Particles in the Inner and Middle Heliospheretive (>100%/AU) radial intensity gradients. Their appearance at 1 AU is associated with the appearance of fast, recurrent solar wind streams. At several AU, CIR energetic particles are accelerated at shocks which propagate away from the interface of fast and slow solar wind streams. CIR energy spect作者: 驚惶 時(shí)間: 2025-3-30 15:40 作者: 斷斷續(xù)續(xù) 時(shí)間: 2025-3-30 20:09
Injection and Acceleration Processes in Corotating Interaction Regions: Theoretical Conceptsnsport equation for energetic particles we discuss diffusive acceleration at the corotating shocks, stochastic acceleration within the interaction region, and the injection and acceleration of pickup ions at the corotating shocks.作者: Colonoscopy 時(shí)間: 2025-3-30 21:42 作者: 附錄 時(shí)間: 2025-3-31 01:00
Modulation of Galactic Cosmic Rays at Solar Minimumr conditions in the changing heliosphere. During the last four years, concentrated around the solar minimum period of solar cycle 22, the exploration of the solar polar regions by the joint ESA/NASA mission Ulysses revealed the three-dimensional behavior of cosmic rays in the inner and middle helios作者: modifier 時(shí)間: 2025-3-31 06:21
The Solar Origin of Corotating Interaction Regions and their Formation in the Inner Heliospherestreams. Dynamic interaction of solar wind streams is a general feature of the heliospheric medium; when the sources of the solar wind streams are relatively stable, the interaction regions form a pattern which corotates with the Sun. The regions of origin of the high speed solar wind streams have b作者: 監(jiān)禁 時(shí)間: 2025-3-31 09:32 作者: PRISE 時(shí)間: 2025-3-31 16:56 作者: Assemble 時(shí)間: 2025-3-31 17:30
Corotating Interaction Regions in the Outer Heliospherere convected to greater heliocentric distances. A progression of different types of structure are observed at increasing distance from the Sun. Similar structures are observed at similar heliocentric distance at different portions of the solar cycle. CIRs and their successors are associated with man
