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Titlebook: Neural Network Parallel Computing; Yoshiyasu Takefuji Book 1992 Springer Science+Business Media New York 1992 VLSI.communication.computer.

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發(fā)表于 2025-3-23 12:55:58 | 只看該作者
Yoshiyasu Takefujient heights in the solar atmosphere, with longer wavelengths referring to higher heights above the photosphere. This review focuses on a few topics related to the physics of the Sun–Earth system. Section 2 summarizes the general context of radio wave propagation and radio emissions. The limits of th
12#
發(fā)表于 2025-3-23 16:22:49 | 只看該作者
Yoshiyasu Takefuji and quantitative information on the physical processes involved in the production of non-thermal electrons and ions has been taken from the wealth of hard X-ray (HXR) and gamma-ray (GR) observations performed over the last fifteen years. This review intends to summarize statistical, temporal and sp
13#
發(fā)表于 2025-3-23 18:08:06 | 只看該作者
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發(fā)表于 2025-3-24 00:19:50 | 只看該作者
Yoshiyasu Takefujiintillation (IPS) or Thomson scattering observations. The tomography program iteratively changes this global model to least-squares fit the data. Both a corotating and time-dependent model can be reconstructed. The short time intervals of the time-dependent modeling (to shorter than 1 day) force the
15#
發(fā)表于 2025-3-24 03:33:14 | 只看該作者
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發(fā)表于 2025-3-24 07:46:41 | 只看該作者
17#
發(fā)表于 2025-3-24 14:11:17 | 只看該作者
Yoshiyasu Takefujients a thorough, step-by-step introduction to solar and stellar dynamos. Looking first at the ultimate origin of cosmic seed magnetic fields, the antagonists of field amplification are next considered: resistive decay, flux expulsion, and flows ruled out by anti-dynamo theorems. Two kinematic flows
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發(fā)表于 2025-3-24 16:03:28 | 只看該作者
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