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22 Year Solar Magnetic Cycle and its relation to Convection Zone Dynamics

Published online by Cambridge University Press:  27 November 2018

Kiran Jain Open the ORCID record for Kiran Jain [Opens in a new window] ,
Sushanta Tripathy ,
Rudolf Komm ,
Frank Hill  and
Rosaria Simoniello
Kiran Jain
Affiliation:
National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303, USA email: kjain@nso.edu, stripathy@nso.edu, rkomm@nso.edu, fhill@nso.edu
Sushanta Tripathy
Affiliation:
National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303, USA email: kjain@nso.edu, stripathy@nso.edu, rkomm@nso.edu, fhill@nso.edu
Rudolf Komm
Affiliation:
National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303, USA email: kjain@nso.edu, stripathy@nso.edu, rkomm@nso.edu, fhill@nso.edu
Frank Hill
Affiliation:
National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303, USA email: kjain@nso.edu, stripathy@nso.edu, rkomm@nso.edu, fhill@nso.edu
Rosaria Simoniello
Affiliation:
Geneva Observatory, University of Geneva, Geneva, Switzerland email: rosaria.simoniello@unige.ch
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Abstract

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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.

Keywords

Sun: activitySun: helioseismologySun: oscillationsSun: interior
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 9 - 10
Copyright
Copyright © International Astronomical Union 2018 

References

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