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Titlebook: Informatics in Control, Automation and Robotics; Selected Papers from Joaquim Filipe,Juan Andrade Cetto,Jean-Louis Ferri Book 2009 Springer

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樓主: hexagon
21#
發(fā)表于 2025-3-25 04:24:25 | 只看該作者
radio emission is indicative of high energy, nonthermal processes: acceleration of electrons to some 10‘s of keV or, in some circumstances, several MeV or more. These electrons then emit radio waves by the incoherent processes of gyroresonance and gyrosynchrotron radiation, and the coherent process
22#
發(fā)表于 2025-3-25 07:39:19 | 只看該作者
Patrick Millot radio emission is indicative of high energy, nonthermal processes: acceleration of electrons to some 10‘s of keV or, in some circumstances, several MeV or more. These electrons then emit radio waves by the incoherent processes of gyroresonance and gyrosynchrotron radiation, and the coherent process
23#
發(fā)表于 2025-3-25 14:57:24 | 只看該作者
24#
發(fā)表于 2025-3-25 18:41:45 | 只看該作者
25#
發(fā)表于 2025-3-25 20:44:47 | 只看該作者
26#
發(fā)表于 2025-3-26 00:49:42 | 只看該作者
Boris Kryzhanovsky,Vladimir Kryzhanovsky,Andrey Mikaelianncluding the Orion, Taurus-Auriga, ρ Ophiuchi and Chamaeleon clouds obtained with the Einstein X-ray Observatory have revealed more than 150 X-ray luminous PMS stars to date. Some are classical strong emission line T Tauri stars while others are late-type PMS stars with weak or absent lines. The sof
27#
發(fā)表于 2025-3-26 06:37:48 | 只看該作者
Nicolas Jouandeauncluding the Orion, Taurus-Auriga, ρ Ophiuchi and Chamaeleon clouds obtained with the Einstein X-ray Observatory have revealed more than 150 X-ray luminous PMS stars to date. Some are classical strong emission line T Tauri stars while others are late-type PMS stars with weak or absent lines. The sof
28#
發(fā)表于 2025-3-26 10:40:01 | 只看該作者
29#
發(fā)表于 2025-3-26 13:44:49 | 只看該作者
30#
發(fā)表于 2025-3-26 19:38:43 | 只看該作者
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