22 Year Solar Magnetic Cycle and its relation to Convection Zone Dynamics
arXiv:1805.05371 · doi:10.1017/S1743921318001242
Abstract
Using continuous observations for 22 years from ground-based network GONG and space-borne instruments MDI onboard {\it SoHO} and HMI onboard {\it SDO}, we report both global and local properties of the convection zone and their variations with time.
To appear in the Proceedings of IAU Symposium 340 held at Jaipur (February 2018)
References in corpus (4)
- Variations in High Degree Acoustic Mode Frequencies of the Sun during Solar Cycle 23 and 24
- A New Challenge to Solar Dynamo Models from Helioseismic Observations: The Latitudinal Dependence of the Progression of the Solar Cycle
- Persistent Near-Surface Flow Structures from Local Helioseismology
- Probing Subsurface Flows in Active Region NOAA 12192 - Comparison with NOAA 10486