Some aspects of an explanation of the soft X-ray solar emission lines on the basis of a finite-temperature Schroedinger equation

Details Some aspects of an explanation of the soft X-ray solar emission lines on the basis of a finite-temperature Schroedinger equation Some aspects of an explanation of the soft X-ray solar emission lines on the basis of a finite-temperature Schroedinger equation

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.199..299m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 199, no. 2, p. 299-315.

Astronomy and Astrophysics

Astrophysics

5

Emission Spectra, Schroedinger Equation, Solar X-Rays, Coulomb Potential, Eigenvalues, Wave Functions

Scientific paper

We discuss the range of validity of solutions of the Schroedinger equation with a temperature modified Coulomb potential. Such a potential, as was recently pointed out, may be relevant to the resolution of the long-standing problem of unidentified solar emission lines. We also consider in detail a predictive test of our approach, and draw attention to some related conceptual issues.

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