Solar Radius Observer Satellite (SoROS)

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

It is known a long time ago that the Sun presents variations. The most obvious of the manifestations is the variation of the solar spots in his surface. With the invention of the telescope around 1600 regular observations, but no systematic, of the solar surface began to be done by several observatories in Europe. The manifestations of the activity cycle in the production of solar energy are associated to the solar wind, to the emission of particles and the magnetic fields on the solar surface. While the energy of the solar wind is negligible compared to the energy in the ultraviolet and in the visible, the relative variations are significantly larger. But can those small fluctuations of energy affect the climate? This mission aim to measure solar shape and radius to test models to explain the variation of solar energy, help to determine Sun's gravitational potential and its internal rotational and for the first time, measure gmodes oscillations frequencies.

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