22 Year Solar Magnetic Cycle and its relation to Convection Zone Dynamics
Kiran Jain, Sushanta Tripathy, Rudolf Komm, Frank Hill, Rosaria, Simoniello
TL;DR
This study analyzes 22 years of solar observations to explore how the solar magnetic cycle influences convection zone dynamics, revealing both global and local property variations over time.
Contribution
It provides a comprehensive analysis of long-term solar convection zone properties and their relation to the solar magnetic cycle using multi-instrument observational data.
Findings
Identification of temporal variations in convection zone properties.
Correlation between magnetic cycle phases and convection zone dynamics.
Insights into the solar magnetic cycle's impact on solar interior processes.
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.