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(fù)制鏈接]
樓主: Jackson
51#
發(fā)表于 2025-3-30 09:09:52 | 只看該作者
Galactic Cosmic Ray Hydrogen and Helium,The quartet of isotopes of hydrogen(H) and helium(He) are the four most abundant species in the arriving cosmic radiation. In this paper, a brief summary of the spectra snd propagation of these species is given. The reader is referred to Beatty (1986) for a more detailed discussion.
52#
發(fā)表于 2025-3-30 16:00:20 | 只看該作者
Gamma-Ray Views on the Galactic Cosmic-Ray Distribution,Recent γ-ray studies of the distribution of cosmic rays throughout the Galaxy are discussed based on the observations obtained with the .-2 .-B satellites. For reasons addressed in this paper the picture arising from recent analyses of both data bases differs from the one generally advocated in the past.
53#
發(fā)表于 2025-3-30 16:59:52 | 只看該作者
54#
發(fā)表于 2025-3-30 22:16:15 | 只看該作者
55#
發(fā)表于 2025-3-31 03:25:46 | 只看該作者
Current Issues in International Tradeyear is about 10. with a mean energy near 10. eV. The above huge power output and number of particles accelerated is likely to be provided by shock waves of expanding supernova remnants ploughing into stellar wind zones. After acceleration, cosmic rays are confined for about 10. years in the Galacti
56#
發(fā)表于 2025-3-31 07:46:15 | 只看該作者
Current Issues in Labour Economicscement, we see that the cosmic ray source is not dominated by the r-process up through the 50’s as evidenced by the Sr/Rb ratio and by the abundance of Sn and Ba. In addition the actinides are not greatly enhanced, ruling out freshly synthesized r-process production as the primary source of the heav
57#
發(fā)表于 2025-3-31 11:33:51 | 只看該作者
58#
發(fā)表于 2025-3-31 14:55:04 | 只看該作者
59#
發(fā)表于 2025-3-31 19:17:27 | 只看該作者
60#
發(fā)表于 2025-4-1 00:54:14 | 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(wù)流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學(xué) 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(xué) 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, 2025-10-7 20:09
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(fù) 返回頂部 返回列表
榆树市| 绥阳县| 迁安市| 张掖市| 张家港市| 库车县| 宁南县| 炉霍县| 广平县| 浮山县| 亚东县| 阳高县| 修水县| 兴国县| 南丹县| 宝坻区| 镇原县| 蒙城县| 安康市| 福安市| 周至县| 株洲县| 恭城| 石城县| 茂名市| 义乌市| 苍溪县| 库车县| 宁晋县| 洪江市| 荣昌县| 北票市| 涡阳县| 海门市| 安吉县| 黑山县| 休宁县| 上思县| 台中市| 原平市| 灵璧县|