Defiance 发表于 2025-4-1 05:23:23

http://reply.papertrans.cn/43/4256/425508/425508_61.png

Banquet 发表于 2025-4-1 06:42:35

http://reply.papertrans.cn/43/4256/425508/425508_62.png

NOMAD 发表于 2025-4-1 10:16:45

Fluid Dynamics and MHD of the Solar Convection Zone and Tachocline: Current Understanding and Unsolvnetic structures; global convection and circulation; the rise of magnetic flux tubes to the photosphere, and their injection into the base of the convection zone; tachocline fluid dynamics and MHD; and the solar dynamo. We close with a set of observational’ targets’ for helioseismologists to aim for.

作茧自缚 发表于 2025-4-1 15:25:21

http://reply.papertrans.cn/43/4256/425508/425508_64.png

空洞 发表于 2025-4-1 20:11:16

http://image.papertrans.cn/h/image/425508.jpg
页: 1 2 3 4 5 6 [7]
查看完整版本: Titlebook: Helioseismic Diagnostics of Solar Convection and Activity; Thomas L. Duvall,John W. Harvey,Zdeněk Švestka Book 2001 Springer Science+Busin