Linking the Sun to the Heliosphere Using Composition Data and Modelling
Abstract
Our understanding of the formation and evolution of the corona and the heliosphere is linked to our capability of properly interpret the data from remote sensing and in-situ observations. In this respect, being able to correctly connect in-situ observations with their source regions on the Sun is the key for solving this problem. In this work we aim at testing a diagnostics method for this connectivity.
- Publication:
-
Space Science Reviews
- Pub Date:
- December 2021
- DOI:
- 10.1007/s11214-021-00856-1
- arXiv:
- arXiv:2110.06111
- Bibcode:
- 2021SSRv..217...78P
- Keywords:
-
- Active region;
- Solar wind;
- Connectivity;
- Diagnostics;
- Modelling;
- UV emission;
- In-situ data;
- Astrophysics - Solar and Stellar Astrophysics;
- Physics - Space Physics
- E-Print:
- 53 pages, 15 figures, 5 tables, accepted for publication in Space Science Reviews