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: Solar and Interplanetary Dynamics; M. Dryer,E. Tandberg-Hanssen Book 1980 International Astronomical Union 1980 Variation.astrophysics.cos

[復制鏈接]
查看: 45971|回復: 71
樓主
發(fā)表于 2025-3-21 17:55:10 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Solar and Interplanetary Dynamics
編輯M. Dryer,E. Tandberg-Hanssen
視頻videohttp://file.papertrans.cn/872/871458/871458.mp4
叢書名稱International Astronomical Union Symposia
圖書封面Titlebook: Solar and Interplanetary Dynamics;  M. Dryer,E. Tandberg-Hanssen Book 1980 International Astronomical Union 1980 Variation.astrophysics.cos
描述Informal discussions in 1977 among a number of scientists asso- ciated with solar and interplanetary physics revealed a need for a dialogue between the two often-divergent groups. It was clear that the latter group was dependent essentially on the sun for its raison d‘etre. On the other hand it was also clear that the former group could benefit in its search for insight vis-a-vis solar activity by looking beyond the shell of the inner corona. Needless to add that the combined solar/interplanetary topic is relevant to astrophysics when one considers stellar winds and binary star flows. It was felt, there- fore, that a symposium was essential to bring together, for the first time, leading solar and interplanetary physicists from the interna- tional community to discuss and record herein their own research. The fundamental physical processes underlying our own capricious star‘s activity can be understood only by the coupling of solar and interplan- etary topics in an intimate observational and theoretical structure. This book, intended for active research scientists and advanced grad- uate students, is an important step in this direction. The background of solar and interplanetary dyn
出版日期Book 1980
關鍵詞Variation; astrophysics; cosmic ray; dynamics; galaxies; heliosphere; planet; solar activity; solar system; s
版次1
doihttps://doi.org/10.1007/978-94-009-9100-2
isbn_softcover978-90-277-1163-2
isbn_ebook978-94-009-9100-2Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightInternational Astronomical Union 1980
The information of publication is updating

書目名稱Solar and Interplanetary Dynamics影響因子(影響力)




書目名稱Solar and Interplanetary Dynamics影響因子(影響力)學科排名




書目名稱Solar and Interplanetary Dynamics網(wǎng)絡公開度




書目名稱Solar and Interplanetary Dynamics網(wǎng)絡公開度學科排名




書目名稱Solar and Interplanetary Dynamics被引頻次




書目名稱Solar and Interplanetary Dynamics被引頻次學科排名




書目名稱Solar and Interplanetary Dynamics年度引用




書目名稱Solar and Interplanetary Dynamics年度引用學科排名




書目名稱Solar and Interplanetary Dynamics讀者反饋




書目名稱Solar and Interplanetary Dynamics讀者反饋學科排名




單選投票, 共有 1 人參與投票
 

0票 0.00%

Perfect with Aesthetics

 

1票 100.00%

Better Implies Difficulty

 

0票 0.00%

Good and Satisfactory

 

0票 0.00%

Adverse Performance

 

0票 0.00%

Disdainful Garbage

您所在的用戶組沒有投票權(quán)限
沙發(fā)
發(fā)表于 2025-3-21 23:28:20 | 只看該作者
A Two-Level Solar Dynamo Based on Solar Activity, Convection, and Differential Rotationhere. It seems natural, therefore, to expect the reconnection aspect of conversion to be located there, where the least work needs to be performed. To transfer the generated flux there, we may add to conversion another spontaneous process: . of bipolar structure (Parker, 1955). To transfer the recon
板凳
發(fā)表于 2025-3-22 03:09:38 | 只看該作者
The Origin of Interplanetary Sectorsize the force-free condition, . × . = 0, and in fact make the more restrictive assumption that this region is current free. The magnetic field in this region can be derived from a solution to the Laplace equation.
地板
發(fā)表于 2025-3-22 05:23:35 | 只看該作者
Stellar Mass Flux and Coronal Heating by Shock Wavese and dissipation terms. The input parameters are the base pressure, the base temperature and the mechanical flux introduced at chromospheric level in form of shock waves. If these three parameters allow a solar wind expansion, the output results are the radial variations of the density, of the temp
5#
發(fā)表于 2025-3-22 12:48:04 | 只看該作者
6#
發(fā)表于 2025-3-22 16:58:16 | 只看該作者
Book 1980 be understood only by the coupling of solar and interplan- etary topics in an intimate observational and theoretical structure. This book, intended for active research scientists and advanced grad- uate students, is an important step in this direction. The background of solar and interplanetary dyn
7#
發(fā)表于 2025-3-22 19:54:58 | 只看該作者
8#
發(fā)表于 2025-3-22 23:18:48 | 只看該作者
9#
發(fā)表于 2025-3-23 03:40:24 | 只看該作者
K. V. Sheridan,G. A. Dulkl ein besonders gesch?ftiges Jahr. Wie Richard Bellman es ausdrückte: ?Man wu?te nie, wo Erd?s sich gerade aufhielt, nicht einmal das Land kannte man. Aber man konnte sicher sein, da? er im Laufe eines ganzen Jahres überall erschien. Er kam einem ergodischen Teilchen [eines, das schlie?lich alle phy
10#
發(fā)表于 2025-3-23 08:19:52 | 只看該作者
 關于派博傳思  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, 2025-10-5 04:05
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
鹤岗市| 明水县| 莱阳市| 镇巴县| 天柱县| 赫章县| 衡阳市| 重庆市| 荣昌县| 晴隆县| 江永县| 连州市| 德兴市| 洮南市| 清河县| 绿春县| 汝州市| 洪泽县| 深水埗区| 阳泉市| 聂拉木县| 麻城市| 扎兰屯市| 和顺县| 阿拉善盟| 桐庐县| 莎车县| 上杭县| 丰宁| 天祝| 交城县| 阳谷县| 镇远县| 西乡县| 屯门区| 古浪县| 油尖旺区| 安康市| 株洲县| 福清市| 昂仁县|