Models for temperature distribution in the solar atmosphere

Details Models for temperature distribution in the solar atmosphere Models for temperature distribution in the solar atmosphere

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ijrsp..20..135a&link_type=abstract

Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 20, April 1991, p. 135-139.

Physics

Space Physics

Solar Atmosphere, Solar Corona, Solar Temperature, Temperature Distribution, Atmospheric Models, Iron, Stellar Models, Sunspot Cycle, Vertical Distribution

Scientific paper

A temperature model for the transition region-inner corona is deduced by assuming a constant conductive flux from higher temperature region toward the lower temperature region. Moreover, using the observed temperatures, a general model (denoted by A) is also fitted, which appears to represent the whole temperature regime of the solar atmosphere. These models are then compared with earlier models. Besides, a comparative study of all of the models (earlier and present ones) with various sets of parameters is also presented. The temperature distribution given by all these models do not differ much from each other. Consequently, one from each region, i.e., TR2 for the transition region-inner corona and OC2 for the outer corona, may be chosen as representative models. The combination of these two models then represents the whole solar atmosphere.

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