Modelling short-term Solar Spectral Irradiance (SSI) using coronal electron density and temperature profiles based on solar magnetic field observations

• Published in: Proceedings of the International Astronomical Union Vol. 12; no. S327; pp. 82 - 85
• Main Authors: Gómez, J. M. Rodríguez, Vieira, L. E. Antunes, Lago, A. Dal, Palacios, J., Balmaceda, L. A., Stekel, T.
• Format: Journal Article
• Language: English
• Published: Cambridge, UK Cambridge University Press 01.10.2016
• Subjects: Astronomy; Atmospheric models; Contributed Papers; Electron density; Emission spectra; Irradiance; Magnetic fields; Magnetic flux; Solar corona; Solar cycle; Solar magnetic field; Temperature profiles; corona; Sun: magnetic fields; photosphere
• ISSN: 1743-9213; 1743-9221
• DOI: 10.1017/S174392131700182X

Some key physical processes that impact the evolution of Earth's atmosphere on time-scale from days to millennia, such as the EUV emissions, are determined by the solar magnetic field. However, observations of the solar spectral irradiance are restricted to the last few solar cycles and are sub...