Titlebook: Solar and Stellar Flares; Proceedings of the 1 Bernhard M. Haisch,Marcello Rodonò Conference proceedings 1989 Kluwer Academic Publishers 19

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嫌恶

Solar Flare Spectral Diagnosis: Present and Future,tensity of soft X-ray lines increases, line profiles show large non-thermal broadenings and strong blue-asymmetries..There have been important contributions in the understanding of the formation of the flare high-temperature plasma, as an effect of the hydrodynamic response of the solar atmosphere t

BURSA

Electron Acceleration in Solar Flares,duration events are consistent with diffusive shock acceleration taking place high in the corona. Electron spectra of short-duration flares are well reproduced by the distribution functions derived from a model assuming simultaneous second-order Fermi acceleration and Coulomb losses operating in clo

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Hyperalgesia

Conference proceedings 1989 solar-stellar articles in the journal Solar Physics. In addition, 115 very exciting posters were also displayed and a companion volume containing many of these is available as a publication of the Catania Astrophysical Observatory. We dedicate this book to the Solar Maximum Mission and to the Flare

shrill

ication of solar-stellar articles in the journal Solar Physics. In addition, 115 very exciting posters were also displayed and a companion volume containing many of these is available as a publication of the Catania Astrophysical Observatory. We dedicate this book to the Solar Maximum Mission and to the Flare978-94-010-6948-9978-94-009-1017-1

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CLIFF

Models of Flaring Loops,vebands, as observed by recent satellite observatories. We find that the predictions of flare loop models are in fact in excellent agreement with these observations, reinforcing both the notion of the loop as a fundamental component of solar flares and the belief that electron acceleration is an integral part of the flare energy release process.

crumble

Preflare Activity,e the variety of preflare activity. Multiple structures are now believed to participate in the energy release. Dynamic global coupling of the magnetic fields between a flaring site and the rest of an activity complex is seen from the data to be an important aspect of preflare activity.

contrast-medium

Solar Flares: The Impulsive Phase,n our understanding of the impulsive phase. New instrumentation planned for observations during the present Cycle 22 will provide a concerted attack on the impulsive phase as part of the Max ’91 program.