饰带
发表于 2025-3-30 10:41:49
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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发表于 2025-3-30 14:04:56
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
发表于 2025-3-30 20:23:17
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Fulsome
发表于 2025-3-30 23:24:23
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
发表于 2025-3-31 04:39:55
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Introduction
发表于 2025-3-31 05:09:21
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畸形
发表于 2025-3-31 10:17:24
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
发表于 2025-3-31 17:13:00
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鞠躬
发表于 2025-3-31 20:02:00
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百灵鸟
发表于 2025-4-1 01:29:12
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.