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

Initiative

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

惊惶

断断续续

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.

Colonoscopy

附录

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

modifier

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

监禁

PRISE

Assemble

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