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

克制

Stellar Flare Spectral Diagnotics: Present and Future,ons and ground-based observatories, with new techniques for obtaining high spectral and temporal resolution, are discussed in light of their possible contribution to our understanding of solar and stellar flares.

粉笔

jaundiced

Electron Beam as Origin of White-Light Solar Flares, enhanced white-light emission both at chromospheric and photospheric level, due to Paschen and H. continua emission, respectively. We then obtain white-light contrasts compatible with observations, obviously showing the link between white-light flares and atmospheric bombardment by electron beams.

slow-wave-sleep

Radio Emission from Stellar Flares,sion for the flare process in classic and compact stars. In particular we discuss the possible production of radio flares from interactions between an accretion disk and the magnetic field of the central object.

Presbycusis

Preface,ways: various aspects of solar flares were observed but hardly ever white-light events, whereas on the stellar side optical flaring was virtually the only observable phenomenon. With the first X-ray detections of flares on UV Ceti, YZ CMi, and Proxima Centauri in the mid-1970’s things changed dramat

暂时过来

nonplus

esoteric

GNAW

防水

Electron Acceleration in Solar Flares,pacecraft detected electrons above 10 MeV. Combining our data with those from the ULEWAT spectrometer (MPI Garching and University of Maryland) electron spectra in the range from 0.1 to 100 MeV were obtained. The observed spectral shapes can be divided into two classes. The spectra of the one class