Solar Magnetic Fields: The Key to Understanding Solar Irradiance Variations

Astronomy and Astrophysics – Astronomy

Scientific paper

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Light (Visible Radiation), Solar Magnetic Field, Solar Atmosphere, Solar Radiation, Synoptic Measurement, Ultraviolet Radiation, Solar Cycles, Secular Variations, Line Of Sight, Solar Convection (Astronomy), Algorithms, Irradiation

Scientific paper

The objective of this research is the development of a scheme for analyzing the properties of full-disk solar magnetograms to determine the variability of different types of solar magnetic structure and its effect on the variation of the radiation emitted by these structures. This approach has operational applications since we consider the analysis of daily synoptic measurements of the line-of-sight magnetic field on the solar hemisphere visible from the Earth with the view to using the results to estimate the variability of solar irradiances at the Earth. However, the study is also one of fundamental importance in solar physics: the relationship of solar magnetism to the radiative losses in the solar atmosphere.

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