Untangling the global coronal magnetic field with multiwavelength observations
Abstract
Magnetism defines the complex and dynamic solar corona. Coronal mass ejections (CMEs) are thought to be caused by stresses, twists, and tangles in coronal magnetic fields that build up energy and ultimately erupt, hurling plasma into interplanetary space. Even the ever-present solar wind possesses a three-dimensional morphology shaped by the global coronal magnetic field, forming geoeffective corotating interaction regions. CME evolution and the structure of the solar wind depend intimately on the coronal magnetic field, so comprehensive observations of the global magnetothermal atmosphere are crucial both for scientific progress and space weather predictions. Although some advances have been made in measuring coronal magnetic fields locally, synoptic measurements of the global coronal magnetic field are not yet available. We conclude that a key goal for 2050 should be comprehensive, ongoing 3D synoptic maps of the global coronal magnetic field. This will require the construction of new telescopes, ground and space-based, to obtain complementary, multiwavelength observations sensitive to the coronal magnetic field. It will also require development of inversion frameworks capable of incorporating multi-wavelength data, and forward analysis tools and simulation testbeds to prioritize and establish observational requirements on the proposed telescopes.
Cite
@article{arxiv.2012.09992,
title = {Untangling the global coronal magnetic field with multiwavelength observations},
author = {S. E. Gibson and A. Malanushenko and G. de Toma and S. Tomczyk and K. Reeves and H. Tian and Z. Yang and B. Chen and G. Fleishman and D. Gary and G. Nita and V. M. Pillet and S. White and U. Bąk-Stęślicka and K. Dalmasse and T. Kucera and L. A. Rachmeler and N. E. Raouafi and J. Zhao},
journal= {arXiv preprint arXiv:2012.09992},
year = {2020}
}
Comments
Helio2050 white paper