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Titlebook: Origin of Cosmic Rays; Giancarlo Setti,Gianfranco Spada,Arnold W. Wolfend Book 1981 International Astronomical Union 1981 active galactic

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樓主: foresight
51#
發(fā)表于 2025-3-30 11:37:28 | 只看該作者
52#
發(fā)表于 2025-3-30 13:14:30 | 只看該作者
Isotopes of Cosmic Ray Elements from Neon to Nickel,from 0.40 to 0.70 amu for A between 20 and 60 amu. This was not adequate to uniquely resolve neighboring mass peaks in many cases, but was adequate to draw a number of conclusions regarding many of the more abundant elements.
53#
發(fā)表于 2025-3-30 17:05:43 | 只看該作者
Book 1981s most workers in the cosmic ray field were interested in the Nuclear Physical aspect of the particle beam and many important dis- coveries were made, notably the identification of the positron, the muon, the pion and the strange particles. More recently however, em- phasis has changed to the Astrop
54#
發(fā)表于 2025-3-30 23:56:57 | 只看該作者
55#
發(fā)表于 2025-3-31 03:46:45 | 只看該作者
56#
發(fā)表于 2025-3-31 06:26:02 | 只看該作者
https://doi.org/10.1007/978-3-662-62050-2les in transit. Brain fluids (CSF and brain interstitial fluid) are secreted, flow through particular routes and then drain back into the venous system; this fluid turnover aids central homeostasis and also affects CNS drug concentration. Several CNS pathologies involve changes in the barrier layers
57#
發(fā)表于 2025-3-31 11:21:18 | 只看該作者
58#
發(fā)表于 2025-3-31 15:26:08 | 只看該作者
59#
發(fā)表于 2025-3-31 21:23:36 | 只看該作者
Preservation of cultural heritage: the design of low-energy archival storagerheben. Für Kritik und Vorschl?ge zur Verbesserung dieses Buches sind wir sehr dank- bar. An dieser Stelle m?chten wir Herrn Dr. R.Amann für seine Beurteilung des Roh- skriptes und Aufforderung zur Ver?ffentlic978-3-662-09750-2
60#
發(fā)表于 2025-4-1 01:27:53 | 只看該作者
,The Anti-de Sitter Proof of Thurston’s Earthquake Theorem,is a (left or right) earthquake. The purpose of these notes is to provide a proof of Thurston’s earthquake theorem, using the bi-invariant geometry of the Lie group ., which is also called Anti-de Sitter three-space. The involved techniques are elementary, and no background knowledge is assumed apart from some two-dimensional hyperbolic geometry.
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