17th European Solar Physics Meeting ESPM-17

Testing MURaM chromosphere: ALMA’s perspective

Not scheduled

1h

Turin, Italy

Poster Fundamental mechanisms of solar plasmas: magnetic reconnection, waves, radiation and particle acceleration Coffee break and poster session 1

Description

In this contribution we use millimeter wavelength diagnostic to test a new model of the solar chromosphere resembling an enhanced network region. The model is based on the recently developed chromospheric extension of the non-equilibrium version of the radiative-MHD code MURaM. We synthesized radio brightness at the operational wavelengths of the Atacama Large Millimeter/Submillimeter Array (ALMA) and compared those with the brightness obtained in the interferometric ALMA observations.