Figure 2 (IMAGE)

Tohoku University

Figure 2

Caption

The spatial structures of magnetorotational turbulence in an accretion disk (modeled). (A) shows the flow and (B) shows the magnetic field intensity. White lines represent typical magnetic field lines. 

Credit

©Yohei Kawazura

Usage Restrictions

Reporters may use freely these materials in news coverage with appropriate credit information.

License

Original content

Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.