22 Year Solar Magnetic Cycle and its relation to Convection Zone Dynamics
Solar and Stellar Astrophysics
2019-01-30 v1
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.
Cite
@article{arxiv.1805.05371,
title = {22 Year Solar Magnetic Cycle and its relation to Convection Zone Dynamics},
author = {Kiran Jain and Sushanta Tripathy and Rudolf Komm and Frank Hill and Rosaria Simoniello},
journal= {arXiv preprint arXiv:1805.05371},
year = {2019}
}
Comments
To appear in the Proceedings of IAU Symposium 340 held at Jaipur (February 2018)