Recent high resolution observations of the Call fine structure are discussed, An analytic method is applied to examine the effects of velocity fields on multi-component model atmospheres in which the central reversal in the bright components is due to self-absorption. It is shown that the inclusion
An empirical interpretation for the time evolution of the CaiiK line
β Scribed by Sou-Yang Liu; Andrew Skumanich
- Publisher
- Springer
- Year
- 1974
- Tongue
- English
- Weight
- 280 KB
- Volume
- 38
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
An empirical approach to interpret the time evolution of the high spatial resolution Ca Ii K line is presented. We specify the physical parameters, such as electron temperature, hydrogen density, and velocity (microturbulent and systematic) as functions of height. The electron density is obtained from scaled non-LTE solutions for hydrogen ionization. The population indices, and thus the Ca n source functions, for a 5-level Ca II atom are computed by using the generalized Newton-Raphson method. K line profiles are then synthesized for different evolutionary stages and are compared with the observed ones. The explanation of the 'peculiar' type profile is also attempted.
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A recent two-component model for the formation of the Ca II K line in the solar chromosphere put forward by Beebe and Johnson is discussed. Although this model is a great advance on existing one-component models, it is pointed out that observations require a minimum of three components in order to u