中文簡(jiǎn)介

地球物理和天體物理流體動(dòng)力學(xué)是為了發(fā)表原始的研究論文和簡(jiǎn)短的通訊，偶爾發(fā)表關(guān)于地球和行星流體力學(xué)的調(diào)查文章和會(huì)議報(bào)告，包括海洋、大氣和內(nèi)部，以及太陽、恒星和其他天體物理物體的流體力學(xué)。此外，還研究了它們的磁流體力學(xué)行為。對(duì)地球物理學(xué)家和天體物理學(xué)家普遍感興趣的旋轉(zhuǎn)、分層和對(duì)流流體進(jìn)行了實(shí)驗(yàn)、理論和數(shù)值研究。正確解釋的觀測(cè)結(jié)果也被公布。如果您對(duì)一些特殊問題有想法，希望出現(xiàn)在地球物理和天體物理流體動(dòng)力學(xué)中，請(qǐng)將其發(fā)送給期刊編輯Andrew Soward，電子郵件：andrew.soward@ncl.ac.uk，并抄送給總編輯Scott Yearsley，電子郵件：scott.yearsley@tandf.co.uk。本雜志所有發(fā)表的研究文章都經(jīng)過了嚴(yán)格的同行評(píng)審，通過最初的編輯篩選和獨(dú)立專家評(píng)審的匿名評(píng)審。所有同行評(píng)審都是單盲的，并且通過學(xué)術(shù)手稿在線提交。

　　英文簡(jiǎn)介

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.

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