日期:
2020 年 — 2026 年
2020
2021
2022
2023
2024
2025
2026
影响因子:

The solar dynamo begins near the surface

太阳发电机效应始于地表附近。

Vasil, Geoffrey M; Lecoanet, Daniel; Augustson, Kyle; Burns, Keaton J; Oishi, Jeffrey S; Brown, Benjamin P; Brummell, Nicholas; Julien, Keith

The photometric variability of massive stars due to gravity waves excited by core convection.

大质量恒星由于核心对流激发的引力波而产生的光度变化

Anders Evan H, Lecoanet Daniel, Cantiello Matteo, Burns Keaton J, Hyatt Benjamin A, Kaufman Emma, Townsend Richard H D, Brown Benjamin P, Vasil Geoffrey M, Oishi Jeffrey S, Jermyn Adam S

Rotation suppresses giant-scale solar convection

自转抑制了大规模太阳对流

Vasil, Geoffrey M; Julien, Keith; Featherstone, Nicholas A

Improved phase-field models of melting and dissolution in multi-component flows

改进的多组分流动中熔化和溶解的相场模型

Hester, Eric W; Couston, Louis-Alexandre; Favier, Benjamin; Burns, Keaton J; Vasil, Geoffrey M

The magnetorotational instability prefers three dimensions

磁旋转不稳定性倾向于三维空间。

Oishi, Jeffrey S; Vasil, Geoffrey M; Baxter, Morgan; Swan, Andrew; Burns, Keaton J; Lecoanet, Daniel; Brown, Benjamin P

On the magnetorotational instability and elastic buckling

关于磁旋转不稳定性与弹性屈曲

Vasil, Geoffrey M