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: Reviews in Modern Astronomy; Gerhard Klare Conference proceedings 1991 Springer-Verlag Berlin Heidelberg 1991 Accretion.Astronomie.Superno

[復(fù)制鏈接]
樓主: Menthol
21#
發(fā)表于 2025-3-25 05:25:01 | 只看該作者
22#
發(fā)表于 2025-3-25 10:03:48 | 只看該作者
Instabilities in Astrophysical Shear Flows,ortant with respect to the occurrence of turbulence in accretion disks and the stability of stellar rotation laws. Properties and mechanisms of shear instabilities relevant in various astrophysical situations are discussed.
23#
發(fā)表于 2025-3-25 14:25:25 | 只看該作者
Simultaneous Observations with a Tunable Filter and the Echelle Spectrograph of the Vacuum Tower Temportant characteristics of the telescope are described. The science observing programs were dedicated to the measurements of small scale magnetic structures and the velocity fields in both horizontal coordinates and at different heights in the solar atmosphere. Narrow band filtergrams in left and r
24#
發(fā)表于 2025-3-25 17:45:41 | 只看該作者
Aspects of the Present Heliospheric Research,he fact that counts most in this context is the evident peculiar motion of the sun relative to the ambient interstellar medium. An interesting puzzle thus is how the inner heliospheric plasma properties reflect this fact. Here we briefly will follow the lines by which the interstellar medium influen
25#
發(fā)表于 2025-3-25 22:37:34 | 只看該作者
26#
發(fā)表于 2025-3-26 01:03:02 | 只看該作者
27#
發(fā)表于 2025-3-26 07:21:59 | 只看該作者
First Results from the X-Ray Astronomy Mission ROSAT,urce in 1962. Collimated counters have been used exclusively in the first 16 years, and they are still the only way to perform X-ray observations at energies above about 20 keV. At lower energies imaging telescopes offer the opportunity to take true pictures of celestial sources at a significantly r
28#
發(fā)表于 2025-3-26 09:32:58 | 只看該作者
29#
發(fā)表于 2025-3-26 13:25:04 | 只看該作者
30#
發(fā)表于 2025-3-26 20:32:58 | 只看該作者
Magnetic Field Measurements on Cool Stars, overview the basics underlying the measurement of magnetic fields on cool stars are briefly introduced. The special role played by the sun in the study of stellar magnetism is pointed out and illustrated with the help of two examples. Stellar measurements in circularly polarized light are discussed
 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, 2025-10-8 04:55
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
开平市| 永清县| 静安区| 黄山市| 铜山县| 阜康市| 长春市| 和林格尔县| 扶绥县| 麟游县| 岱山县| 涿鹿县| 霍林郭勒市| 永胜县| 武汉市| 瑞昌市| 红桥区| 定日县| 珠海市| 郸城县| 科技| 宜昌市| 蛟河市| 区。| 新密市| 瑞丽市| 卢湾区| 榆中县| 泰和县| 阿坝| 长丰县| 新竹县| 大埔县| 鄂托克前旗| 海门市| 彩票| 宁国市| 青龙| 长汀县| 汝城县| 洱源县|