GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS期刊中文簡介

地球物理和天體物理流體動力學是為了發(fā)表原始的研究論文和簡短的通訊，偶爾發(fā)表關于地球和行星流體力學的調查文章和會議報告，包括海洋、大氣和內部，以及太陽、恒星和其他天體物理物體的流體力學。此外，還研究了它們的磁流體力學行為。對地球物理學家和天體物理學家普遍感興趣的旋轉、分層和對流流體進行了實驗、理論和數值研究。正確解釋的觀測結果也被公布。如果您對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力學中，請將其發(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)表的研究文章都經過了嚴格的同行評審，通過最初的編輯篩選和獨立專家評審的匿名評審。所有同行評審都是單盲的，并且通過學術手稿在線提交。

　　GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS期刊英文簡介

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.

　　GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS近年期刊影響因子趨勢圖

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