Statistics – Computation
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh23b1550d&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #SH23B-1550
Statistics
Computation
[0545] Computational Geophysics / Modeling, [7507] Solar Physics, Astrophysics, And Astronomy / Chromosphere, [7534] Solar Physics, Astrophysics, And Astronomy / Radio Emissions, [7538] Solar Physics, Astrophysics, And Astronomy / Solar Irradiance
Scientific paper
We present a numerical package intended to compute the solar emission in the millimeter to infrared part of the spectrum. This package is composed by three parts, namely: Seris, PakalMPI and Jaguar. We discuss the physical models and basic assumptions of the code. We have used, as inputs, three different theoretical solar atmospheric models: VALC, C7 and CAIUS05 in order to reproduce the solar spectrum. We also included three different opacity functions: Classic Bremsstrahlung, Inverse Bremsstrahlung and H-, and we have compared their relative contribution to the total opacity. We present the detailed analysis of the solar emission at three particular frequencies: 17GHz, 212GHz and 405GHz. Finally we compare our results with several observations including the Solar Submillimeter Telescope observations at 212 and 405GHz.
de La Luz V. H.
Kaufmann Patrik
Lara Alejandro
Raulin J.
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