Titlebook: Cool Stars, Stellar Systems, and the Sun; Proceedings of the F Jeffrey L. Linsky,Robert E. Stencel Conference proceedings 1987 Springer-Ver

饰带

The dynamics of solar magnetic flux tubes subjected to resonant foot point shaking,endent development of waves in thin magnetic flux tubes generated by this purely transverse foot point shaking. The resulting magnetic field and velocity variations, the pressure and temperature fluctuations generated by nonlinear coupling to the longitudinal wave mode, as well as the expected resonance effects are discussed.

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A VLA survey of dMe flare stars,cm, two bands centered at 4535 and 4985 MHz are observed. Results so far, based on a total observing time of about one hour each during July 1986 have yielded detections from 9 of the 27 stellar systems in the program.

intrude

Fulsome

Dae-Hee Seo,Deok-Gyu Lee,Im-Yeong Leeo concerning the escape of the radiation through the strongly absorbing second harmonic layer. It is suggested that stellar bursts are likely to consist of narrowband drifting structures, and that observations to test this suggestion are desirable.

Entrancing

Introduction

畸形

Control Objectives and Strategies,function of the magnetic field strength. We also present wave flux calculations for magnetic flux tubes embedded in the solar convective zone; the main result is that the longitudinal tube wave fluxes are at least 2 orders of magnitude too low to play a significant role in the heating of the solar chromosphere.

Asymptomatic

鞠躬

百灵鸟

MHD wave energy fluxes for late-type dwarfs,free atmosphere, and do not vary enough for a given spectral type in order to explain observed UV and X-ray fluxes. Thus, our results show that MHD energy fluxes obtained if stellar surface magnetic fields are uniform cannot explain the observed stellar coronal emissions.