Abstract
Laboratory experiments demonstrate high-speed plasma flows from both footpoints of arched magnetic flux tubes, resulting in bulk plasma transport into the flux tube and persistent axial collimation even as the flux tube lengthens and kinks. The measured flows are in agreement with the predictions of hoop force and collimation models involving fundamental MHD forces. These forces are expected to drive plasma acceleration in other open flux configurations with arched geometries, such as those found on the solar surface.
- Received 12 August 2011
DOI:https://doi.org/10.1103/PhysRevLett.109.075001
© 2012 American Physical Society
Viewpoint
Bringing the Sun Down to Earth
Published 13 August 2012
A laboratory analog of solar plasma offers a new tool in the search for the origin of coronal heating.
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