GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS

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地球物理和天体物理流体动力学是为了发表原始的研究论文和简短的通讯，偶尔发表关于地球和行星流体力学的调查文章和会议报告，包括海洋、大气和内部，以及太阳、恒星和其他天体物理物体的流体力学。此外，还研究了它们的磁流体力学行为。对地球物理学家和天体物理学家普遍感兴趣的旋转、分层和对流流体进行了实验、理论和数值研究。正确解释的观测结果也被公布。如果您对一些特殊问题有想法，希望出现在地球物理和天体物理流体动力学中，请将其发送给期刊编辑Andrew Soward，电子邮件：andrew.soward@ncl.ac.uk，并抄送给总编辑Scott Yearsley，电子邮件：scott.yearsley@tandf.co.uk。本杂志所有发表的研究文章都经过了严格的同行评审，通过最初的编辑筛选和独立专家评审的匿名评审。所有同行评审都是单盲的，并且通过学术手稿在线提交。

Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published. If you have ideas for Special Issues that you would like to appear in Geophysical and Astrophysical Fluid Dynamics, please send them to the Journal Editor, Andrew Soward, E-mail: andrew.soward@ncl.ac.uk, and copied to the Managing Editor, Scott Yearsley, E-mail: scott.yearsley@tandf.co.uk. All published research articles in this journal have undergone rigorous peer review, based on initial editor screening and anonymized refereeing by independent and expert referees. All peer review is single blind, and submission is online via ScholarOne Manuscripts.