The ionization conditions in coronal loops are investigated in the temperature range 2 x 10s-2 β’ 106 K, assuming velocity, density and temperature distributions computed for a siphon model of a pure hydrogen plasma, Use is made of the set of the carbon ions as an example of the general behaviour of
Non-equilibrium ionization as a consequence of flows in coronal loops
β Scribed by D. Spadaro
- Publisher
- Elsevier Science
- Year
- 1991
- Tongue
- English
- Weight
- 810 KB
- Volume
- 11
- Category
- Article
- ISSN
- 0273-1177
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
The loss of equilibrium in coronal magnetic field structures is a possible source of energy for coronal heating and solar flares. We investigate whether such a loss of equilibrium occurs when a coronal loop is progressively twisted by photospheric motions. In studies of 2-D cylindrical equilibria, l
The coronal explosions, discovered by De Jager and Boelee (1984), and interpreted by them as manifestations of plasma streaming out of the flare kernels, can also be interpreted as signatures of current loop coalescence in the flaring region. ## i. Characteristics of coronal Explosions.