The Solar Close Observations and Proximity Experiments (SCOPE) mission
Jun Lin, Jing Feng, Zhenhua Ge, Jiang Tian, Yuhao Chen, Xin Cheng, Hui Tian, Jiansen He, Alexei Pevtsov, Haisheng Ji, Shangbin Yang, Parida Hashim, Bin Zhou, Yiteng Zhang, Shenyi Zhang, Xi Lu, Yuan Yuan, Liu Liu, Haoyu Wang, Hu Jiang, Lei Deng, Xingjian Shi, Lin Ma

TL;DR
The SCOPE mission aims to send a spacecraft close to the Sun to directly measure the coronal magnetic field, study solar eruptions, coronal heating, and solar wind acceleration through in situ and high-resolution observations.
Contribution
This paper introduces the SCOPE mission concept, detailing its innovative approach to directly measure the solar magnetic field and investigate key solar phenomena at unprecedented proximity.
Findings
Design of a spacecraft to approach within 5 R_sun of the Sun
Proposed measurements of nano-flares and magnetic fields at small scales
Plan to observe the solar wind acceleration and magnetic reconnection processes
Abstract
The Solar Close Observations and Proximity Experiments (SCOPE) mission will send a spacecraft into the solar atmosphere at a low altitude of just 5 R_sun from the solar center. It aims to elucidate the mechanisms behind solar eruptions and coronal heating, and to directly measure the coronal magnetic field. The mission will perform in situ measurements of the current sheet between coronal mass ejections and their associated solar flares, and energetic particles produced by either reconnection or fast-mode shocks driven by coronal mass ejections. This will help to resolve the nature of reconnections in current sheets, and energetic particle acceleration regions. To investigate coronal heating, the mission will observe nano-flares on scales smaller than 70 km in the solar corona and regions smaller than 40 km in the photosphere, where magnetohydrodynamic waves originate. To study solar…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Astro and Planetary Science
