The ionization conditions in coronal loops are investigated in the temperature range 2 x 10s-2 โข 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 in the transition region network
โ Scribed by Michael H. Francis
- Publisher
- Springer
- Year
- 1981
- Tongue
- English
- Weight
- 765 KB
- Volume
- 69
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
We explore the consequences of the recently reported, persistent downflow of material within the supergranule network. The velocities observed by OSO-8, about 5 km s -1 for C IV A 1548 and 20 km s -1 for O vI h1032, are sufficient to cause the ion distributions to differ significantly from those of ionization equilibrium. Using an accepted temperature model and two models of the velocity fields, we determine the ion distributions of carbon, nitrogen, and oxygen throughout the transition region and compare them with the equilibrium distributions. We then investigate how the temperature model must be modified in order to reconcile the computed line intensities with observed and show that a smaller temperature gradient, and possibly a different pressure distribution, are required. Finally, we demonstrate that the observed downflow is probably adequate to overcome the tendency for thermal diffusion to establish concentration gradients and thus the downflow keeps the atmosphere well mixed.
๐ SIMILAR VOLUMES
In the present paper we have investigated the growth rate of ionization instability taking into account the temperature/velocity dependence of collision frequency by using the phenomenological and semi-kinetic approach. For the semi-kinetic treatment, the Boltzmann Transfer Equation (BTE) has been u