The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action
I. Zouganelis, A. De Groof, A. P. Walsh, D. R. Williams, D. Mueller,, O. C. St Cyr, F. Auchere, D. Berghmans, A. Fludra, T. S. Horbury, R. A., Howard, S. Krucker, M. Maksimovic, C. J. Owen, J. Rodriiguez-Pacheco, M., Romoli, S. K. Solanki, C. Watson, L. Sanchez, J. Lefort

TL;DR
The Solar Orbiter mission aims to understand solar and heliospheric physics by strategically planning observations to address key scientific questions about solar wind, transients, eruptions, and the solar dynamo, maximizing scientific return.
Contribution
This paper presents a comprehensive Science Activity Plan that translates core scientific questions into coordinated observation strategies for the Solar Orbiter mission.
Findings
Development of a top-level observation plan (SAP) for Solar Orbiter.
Organization of observations into Solar Orbiter Observing Plans (SOOPs).
Enhanced coordination of remote sensing and in-situ measurements.
Abstract
Solar Orbiter is the first space mission observing the solar plasma both in situ and remotely, from a close distance, in and out of the ecliptic. The ultimate goal is to understand how the Sun produces and controls the heliosphere, filling the Solar System and driving the planetary environments. With six remote-sensing and four in-situ instrument suites, the coordination and planning of the operations are essential to address the following four top-level science questions: (1) What drives the solar wind and where does the coronal magnetic field originate? (2) How do solar transients drive heliospheric variability? (3) How do solar eruptions produce energetic particle radiation that fills the heliosphere? (4) How does the solar dynamo work and drive connections between the Sun and the heliosphere? Maximising the mission's science return requires considering the characteristics of each…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Space exploration and regulation · Astro and Planetary Science
