Titlebook: Coronal Physics from Radio and Space Observations; Proceedings of the C Gérard Trottet Conference proceedings 1997 Springer-Verlag Berlin H

管理員

Observations of the 3D distributions of thermal to near-relativistic electrons in the interplanetardistributions . .(. .) often are plateaued or slightly unstable, with ., implying growth rates of . ～0.03 s.. Most of the time, however, the reduced distributions are stable, with negative slopes, suggesting that other competing wave processes such as whistler growth may be stabilizing the beam.

縮影

Carcinogenesis

Prospects for the solar radio telescope,be done with a solar-dedicated radio synthesis telescope, and to discuss the design constraints imposed by the science envisioned. Special attention was also given to nighttime uses for the instrument. We summarize the “strawman” concept for the instrument here.

季雨

0075-8450 nd WIND and spectral and imaging data from SOHO and YOHKOH provide an unprecedented richness of relevant data. For their better understanding, radio observations - also included in this book - play a key role.978-3-662-14120-5978-3-540-68693-4Series ISSN 0075-8450 Series E-ISSN 1616-6361

流浪者

一美元

The Nature of Liquids and Gases,al processes creating enhanced plasma wave turbulence and particle acceleration at shock waves. The ULYSSES, WIND, and SOHO missions together with ground based observations and additional theoretical investigations are an exceptional opportunity to achieve progress in answering the many open questions.

燦爛

Diagnostics of energy release in the X-ray corona,ent results of X-ray bright-points, transient brightenings and jets are reviewed, and diagnostics that result from bulk plasma motions are discussed. Finally, three events are examined in detail and the implications of the observation discussed in relation to flare models.

動作謎

Solar flare radio and hard X-ray observations and the avalanche model,al electrons is fragmented in both space and time. Observations dealing with the extent in heights and spatial scales of the electron acceleration sites are also reviewed. The knowledge of the electron energy spectra deduced at low and high energies from both hard X-ray and centimeter/millimeter obs

北極熊

Radio observations of the quiet sun and their implications on coronal heating,oblem of coronal heating. Radio observations provide powerful diagnostics of the physical conditions in the transition region and the corona. Recent observational and theoretical results are presented and their implications are discussed. The prospects of further observations, in conjunction with ot

adj憂郁的

Energy release in the solar corona,particle events, as well as coronal heating and the solar wind. The basic physics of these phenomena and their relationship to each other remains a vigorous area of inquiry. The . at Mont Evray directed its attention to recent observational and theoretical developments relevant to flares and coronal