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arXiv · 1502.03368

The Polarimetric and Helioseismic Imager for Solar Orbiter: SO/PHI

Sami K. Solanki·Jose Carlos del Toro Iniesta·Joachim Woch·Achim Gandorfer·Johann Hirzberger·Wolfgang Schmidt·Thierry Appourchaux·Alberto Alvarez-Herrero
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Abstract

The {\em Solar Orbiter} is the next solar physics mission of the European Space Agency, ESA, in collaboration with NASA, with a launch planned in 2018. The spacecraft is designed to approach the Sun to within 0.28\,AU at perihelion of a highly eccentric orbit. The proximity with the Sun will also allow its observation at uniformly high resolution at EUV and visible wavelengths. Such observations are central for learning more about the magnetic coupling of the solar atmosphere. At a later phase in the mission the spacecraft will leave the ecliptic and study the enigmatic poles of the Sun from a heliographic latitude of up to 33$^\circ$.

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Sami K. Solanki, Jose Carlos del Toro Iniesta, Joachim Woch, Achim Gandorfer, Johann Hirzberger, Wolfgang Schmidt, Thierry Appourchaux, Alberto Alvarez-Herrero. 2015-02-11. The Polarimetric and Helioseismic Imager for Solar Orbiter: SO/PHI. https://arxiv.org/abs/1502.03368

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