INSTRUMENTAL APPROACHES TO ACHIEVE THE MEASUREMENTS REQUIRED FOR EXPLORING THE ENERGETICS, DYNAMICS, AND FINE-SCALE STRUCTURE OF THE SUN'S MAGNETIZED ATMOSPHERE

摘要

An overview is given about the technical implementation of the remote sensing instrumentation of the Solar Orbiter mission. We will discuss the "science implementation" related to the specific scientific goal "Explore the energetics, dynamics and fine-scale structure of the Sun's magnetized atmosphere". The technical approaches to implement the observational scenarios outlined in the Science Requirements Document (SRD) are reviewed. Some technical design options proposed for the remote sensing instruments will be shown in detail and some open technical issues are highlighted in regard to answering the question "How do we achieve this goal?"