Fig. 2. The different scenario of solar wind interaction of magnetic anomalies (the spatial scale is exaggerated), in both of which there is no bow shock and the ion kinetic effects dominate. (IMAGE)

Beijing Institute of Technology Press Co., Ltd

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.