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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
Affiliation:
National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303, USA email: [email protected], [email protected], [email protected], [email protected]
Sushanta Tripathy
Affiliation:
National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303, USA email: [email protected], [email protected], [email protected], [email protected]
Rudolf Komm
Affiliation:
National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303, USA email: [email protected], [email protected], [email protected], [email protected]
Frank Hill
Affiliation:
National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303, USA email: [email protected], [email protected], [email protected], [email protected]
Rosaria Simoniello
Affiliation:
Geneva Observatory, University of Geneva, Geneva, Switzerland email: [email protected]
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

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