MHD Collimation Mechanism in Arched Flux Ropes Characterized Using Volumetric, Time-Dependent B-Vector Measurements
Journal Article
·
· Geophysical Research Letters
- California Inst. of Technology (CalTech), Pasadena, CA (United States); DOE/OSTI
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
Laboratory measurements of B(x,t) in a volume enclosing portions of two arched flux ropes show flux rope collimation driven by gradients in axial current density. These measurements verify the three predictions of a proposed MHD collimation mechanism: (1) axial magnetic forces exist in current channels with spatially varying minor radius, (2) these forces can drive counterpropagating axial flows, and (3) this process collimates the flux rope. As a result, this mechanism may explain the axial uniformity of solar loops and is relevant to other systems with current channels of varying minor radius such as solar prominences and astrophysical jets.
- Research Organization:
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC)
- Grant/Contract Number:
- FG02-04ER54755; SC0010471
- OSTI ID:
- 1537298
- Alternate ID(s):
- OSTI ID: 1574934; OSTI ID: 1397314
- Journal Information:
- Geophysical Research Letters, Journal Name: Geophysical Research Letters Journal Issue: 19 Vol. 44; ISSN 0094-8276
- Publisher:
- American Geophysical UnionCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Experiments and models of MHD jets and their relevance to astrophysics and solar physics
|
journal | May 2018 |
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