Internet Archive Scholar

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

Kiran Jain, Sushanta Tripathy, Rudolf Komm, Frank Hill, Rosaria Simoniello
2018 Proceedings of the International Astronomical Union  

Preserved Fulltext

fulltext thumbnail
Web Archive Capture PDF (354.4 kB)
https://web.archive.org/web/20200826002331/https://arxiv.org/pdf/1805.05371v1.pdf

A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL. The file type is application/pdf.

Note that this fulltext copy is not of the "primary" version of this work. The version it corresponds to is:

2018 pre-print arXiv:1805.05371v1 fatcat:btxojyvwdbepfcgjqxqeyq3ha4
AbstractUsing 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.
doi:10.1017/s1743921318001242 fatcat:xczjcmo7djdl3gadcxk2foljum
Multiple Versions
Citation

Kiran Jain, Sushanta Tripathy, Rudolf Komm, Frank Hill, Rosaria Simoniello. "22 Year Solar Magnetic Cycle and its relation to Convection Zone Dynamics." Proceedings of the International Astronomical Union 13.S340 (2018) 9-10