AUTHOR=Van Doorsselaere Tom , Antolin Patrick , Yuan Ding , Reznikova Veronika , Magyar Norbert 

TITLE=Forward Modeling of EUV and Gyrosynchrotron Emission from Coronal Plasmas with FoMo

JOURNAL=Frontiers in Astronomy and Space Sciences

VOLUME=Volume 3 - 2016

YEAR=2016

URL=https://www.frontiersin.org/journals/astronomy-and-space-sciences/articles/10.3389/fspas.2016.00004

DOI=10.3389/fspas.2016.00004

ISSN=2296-987X

ABSTRACT=The FoMo code was developed to calculate the EUV emission from optically
thin coronal plasmas. The input data for FoMo consists of the coronal
density, temperature and velocity on a 3D grid. This is translated to
emissivity on the 3D grid, using CHIANTI data. Then, the emissivity is
integrated along the line-of-sight to calculate the emergent spectral
line that could be observed by a spectrometer.
Moreover, the code has been extended to model also the radio emission
from plasmas with a population of non-thermal particles. In this case,
also optically thick plasmas may be modelled. The radio spectrum is
calculated over a large wavelength range, allowing for the comparison
with data from a wide range of radio telescopes.