共查询到20条相似文献,搜索用时 15 毫秒
1.
2.
Ralph D. Lorenz 《Meteoritics & planetary science》2014,49(6):1139-1140
3.
4.
35 Seasons of U.S. Antarctic Meteorites: A Pictorial Guide to the Collection,edited by K. Righter,C. M. Corrigan,T. J. McCoy and R. P. Harvey. Hoboken,New Jersey: Wiley, 2014, 320 p. $99.95, hardcover (ISBN #978‐1‐118‐79832‐4).
下载免费PDF全文
![点击此处可从《Meteoritics & planetary science》网站下载免费的PDF全文](/ch/ext_images/free.gif)
Nicolle E. B. Zellner 《Meteoritics & planetary science》2015,50(12):2140-2141
5.
6.
7.
8.
9.
10.
11.
Ernst Zinner 《Meteoritics & planetary science》2010,45(9):1527-1528
12.
13.
14.
15.
Ulrich Bleyer 《Astronomische Nachrichten》1986,307(3):220-220
16.
17.
18.
We have carried out global three‐dimensional magnetohydrodynamic simulations of the star‐disc interaction region around a young solar‐type star. The magnetic field is generated and maintained by dynamos in the star as well as in the disc. The developing mass flows possess non‐periodic time‐variable azimuthal structure and are controlled by the nonaxisymmetric magnetic fields. Since the stellar field drives a strong stellar wind, accretion is anti‐correlated with the stellar field strength and disc matter is spiraling onto the star at low latitudes, both contrary to the generally assumed accretion picture. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
19.