Titlebook: Corotating Interaction Regions; Proceedings of an IS A. Balogh,J. T. Gosling,H. Kunow Conference proceedings 1999 Springer Science+Business

驳船

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.

libertine

excursion

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

Oversee

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

sperse

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

为宠爱

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

Apoptosis

辩论

牵连

树木中

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