找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

Titlebook: Genesis and Propagation of Cosmic Rays; Maurice M. Shapiro (Director of the School, Co-Dir Book 1988 D. Reidel Publishing Company, Dordrec

[復制鏈接]
樓主: Jackson
61#
發(fā)表于 2025-4-1 02:06:19 | 只看該作者
62#
發(fā)表于 2025-4-1 09:21:45 | 只看該作者
63#
發(fā)表于 2025-4-1 11:14:42 | 只看該作者
Stars and Cosmic Rays,ouds: they excite giant HII regions, inside which they create large wind cavities. The possibility of particle acceleration by wind shocks then allows to introduce the concept of thick cosmic-ray sources. The high-energy particles generated by such sources are very different from those associated wi
64#
發(fā)表于 2025-4-1 17:41:47 | 只看該作者
65#
發(fā)表于 2025-4-1 19:29:16 | 只看該作者
Radio Astronomy and Cosmic Rays,possibly, or even probably, originates in supernovae and/or supernova remnants. Therefore in consideration of this electronic component, we review the general history and observed properties of supernovae with concentration on the more recent results or radio supernovae, the observed properties of s
66#
發(fā)表于 2025-4-1 22:42:44 | 只看該作者
Particle Acceleration in Galactic Supernova Remnants,ion. Young, bright shell remnants generally have spectral indices α larger than the 0.5 expected from basic shock acceleration theory. Fainter, older shell remnants have a wide range of α. Evidence on whether or not particle acceleration is continuing in SNRs is also discussed.
67#
發(fā)表于 2025-4-2 04:23:22 | 只看該作者
68#
發(fā)表于 2025-4-2 08:04:27 | 只看該作者
Conditions for Acceleration of Super-High Energy Cosmic Rays in Active Galactic Nuclei,The current system might resemble an electrical circuit with a voltage source (black hole and accretion disc) coupled to a load (cosmic-ray beam) and a low impedance element (ambient conducting medium). Beam particles can be accelerated to 10. provided that the beam channel medium behaves like an in
69#
發(fā)表于 2025-4-2 13:16:57 | 只看該作者
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學 Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學 Yale Uni. Stanford Uni.
QQ|Archiver|手機版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-8 04:51
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復 返回頂部 返回列表
成武县| 田林县| 鸡泽县| 江油市| 惠来县| 来安县| 巴林右旗| 涿鹿县| 苍梧县| 科技| 三都| 新民市| 武义县| 长沙市| 竹溪县| 延津县| 镇平县| 金寨县| 利津县| 德清县| 曲阳县| 清涧县| 阳西县| 全南县| 长治县| 重庆市| 仁寿县| 曲沃县| 大埔县| 辽源市| 沅陵县| 定安县| 永胜县| 万全县| 虹口区| 县级市| 永和县| 承德市| 吉木萨尔县| 饶阳县| 望都县|