In situ categorization and coronal origins of different slow solar wind types
Abstract
The slow solar wind is not as regular as the fast wind, and a number of periods have been identified where the turbulence is essentially Alfvénic (Marsch et al. 1981, D'Amicis and Bruno, 2015). What creates the difference between “standard" and Alfvénic slow wind? Is the
- Publication:
-
Solar Heliospheric and INterplanetary Environment (SHINE 2018)
- Pub Date:
- July 2018
- Bibcode:
- 2018shin.confE.236P