The solar wind streams from flares: Magnetic field configuration at 1 a.u.

1987 ◽  
Vol 35 (6) ◽  
pp. 793-798
Author(s):  
M.S. Bobrov
Keyword(s):  
Magnetic Field ◽  
Solar Wind ◽  
Field Configuration ◽  
Magnetic Field Configuration

scholarly journals APPLICATION OF A SOLAR WIND MODEL DRIVEN BY TURBULENCE DISSIPATION TO A 2D MAGNETIC FIELD CONFIGURATION

2014 ◽  
Vol 796 (2) ◽  
pp. 111 ◽  
Author(s):  
Roberto Lionello ◽  
Marco Velli ◽  
Cooper Downs ◽  
Jon A. Linker ◽  
Zoran Mikić
Keyword(s):  
Magnetic Field ◽  
Solar Wind ◽  
Field Configuration ◽  
Magnetic Field Configuration ◽  
Wind Model ◽  
Model Driven ◽  
Solar Wind Model

Asymmetric shear flow effects on magnetic field configuration within oppositely directed solar wind reconnection exhausts

2009 ◽  
Vol 114 (A7) ◽  
pp. n/a-n/a ◽  
Author(s):  
S. Eriksson ◽  
J. T. Gosling ◽  
T. D. Phan ◽  
L. M. Blush ◽  
K. D. C. Simunac ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Solar Wind ◽  
Shear Flow ◽  
Field Configuration ◽  
Magnetic Field Configuration ◽  
Flow Effects

scholarly journals Heliospheric Magnetic Field Configuration and its Coronal Sources

2001 ◽  
Vol 203 ◽  
pp. 585-594 ◽  
Author(s):  
T. H. Zurbuchen
Keyword(s):  
Magnetic Field ◽  
Solar Wind ◽  
Solar Cycle ◽  
Differential Rotation ◽  
Field Configuration ◽  
The Sun ◽  
Coronal Structure ◽  
Magnetic Field Configuration ◽  
Archimedean Spiral ◽  
Heliospheric Magnetic Field

The heliospheric magnetic field configuration is largely determined in the solar atmosphere. The interplanetary magnetic field is therefore intimately linked with the coronal structure and evolution during the solar cycle. We summarize recent experimental results from active satellite experiments on Ulysses and the Advanced Composition Explorer (ACE). These results provide constraints on the sources of the solar wind and also the magnetic structure of the heliosphere and the corona. These results suggest the relevance of reconnection processes and differential rotation effects close to the Sun. This leads to large perturbations from a standard Archimedean spiral configuration which cannot be successfully modeled using coronal models which assume a potential magnetic field.

Experimental study of force-free, collinear plasma structures

1973 ◽  
Vol 9 (1) ◽  
pp. 1-15 ◽  
Author(s):  
E. E. Nolting ◽  
P. E. Jindra ◽  
D. R. Wells
Keyword(s):  
Magnetic Field ◽  
Experimental Study ◽  
Magnetic Fields ◽  
Flow Fields ◽  
Diagnostic Techniques ◽  
Field Configuration ◽  
Magnetic Mirror ◽  
Magnetic Field Configuration ◽  
Magnetic Barrier ◽  
Magnetic Well

Detailed measurements of the trapped magnetic fields and currents in plasma structures generated by conical theta-pinches are reported. Studies of these structures interacting with a magnetic barrier, and with each other in a collision at the centre of a magnetic mirror, are reported. The magnetic well formed by the collision has been studied by simultaneous use of several diagnostic techniques. The measurements are in agreement with a force-free, collinear magnetic field configuration (Wells 1972). Arguments relating superposability and collinearity of flow fields to these observations are given.

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