Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...304..532a&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 304, May 1, 1986, p. 532-541. Research supported by the National Academy of
Astronomy and Astrophysics
Astrophysics
7
Condensation, Magnetohydrodynamic Stability, Solar Magnetic Field, Solar Prominences, Cylindrical Plasmas, Lines Of Force, Magnetic Effects, Plasma Density, Plasma Temperature, Shear Properties
Scientific paper
The present study of the condensation modes in coronal cylindrical plasmas, with attention to magnetic shear effects on stability, notes that such shear is insignificant in the initiation of condensation in the case of low beta coronal plasmas. The effects of magnetic field shear, twist, and strength on condensation modes differ, depending on the wave vector. The stability of condensation modes strongly depends on the choice of equilibrium temperature and density profiles. If plasma temperature increases with twist but density does not, condensation modes are unstable for low field twist; by contrast, if plasma density increases with twist but temperature does not, condensation modes are unstable for high twist.
No associations
LandOfFree
Condensation modes in sheared magnetic fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Condensation modes in sheared magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Condensation modes in sheared magnetic fields will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1773109