Theoretical hydrogen population relations for horizontal cloud-like solar structures

Details Theoretical hydrogen population relations for horizontal cloud-like solar structures Theoretical hydrogen population relations for horizontal cloud-like solar structures

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..183t&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Statistics

Computation

Solar Surface: Structure, Solar Prominences

Scientific paper

A large set of parameterized NLTE models has been computed for a 1D horizontal cloud-like structure standing above the solar surface. The used input model parameters are temperature, velocity, microturbulence, electronic density and geometrical thickness of the structure. From the output of our computations which is the hydrogen level populations as a function of the line center optical depth, we calculate several relations between the hydrogen population levels and the considered electron density. These relations are important for the study of prominence-like structures from observations.

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