22 Year Solar Magnetic Cycle and its relation to Convection Zone Dynamics
Abstract
Using continuous observations for 22 years from ground-based network GONG and space-borne instruments MDI onboard SoHO and HMI onboard SDO, we report both global and local properties of the convection zone and their variations with time.
- Publication:
-
Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles
- Pub Date:
- February 2018
- DOI:
- 10.1017/S1743921318001242
- arXiv:
- arXiv:1805.05371
- Bibcode:
- 2018IAUS..340....9J
- Keywords:
-
- Sun: activity;
- Sun: helioseismology;
- Sun: oscillations;
- Sun: interior;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- To appear in the Proceedings of IAU Symposium 340 held at Jaipur (February 2018)