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An Overview of Science Results Obtained From Kodaikanal Digitized White-Light Data Archive: 1921-2011

Published online by Cambridge University Press:  27 November 2018

Sudip Mandal  and
Dipankar Banerjee Open the ORCID record for Dipankar Banerjee [Opens in a new window]
Sudip Mandal
Affiliation:
Indian Institute of Astrophysics, Banglore 560034, India email: [email protected]
Dipankar Banerjee
Affiliation:
Indian Institute of Astrophysics, Banglore 560034, India email: [email protected] Center of Excellence in Space Sciences India, IISER Kolkata, Mohanpur 741246, West Bengal, India email: [email protected]
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Abstract

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In this proceeding, we present a summary of the recent scientific results that have been derived using the newly digitized whit-light (WL) data obtained from the Kodaikanal Solar Observatory.

Keywords

Sun: sunspotsSun: magnetic fields
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. 196 - 197
Copyright
Copyright © International Astronomical Union 2018 

References

Berdyugina, S. V. (2007). Preferred longitudes in solar and stellar activity, memsai, 78:242.Google Scholar
Mandal, S. & Banerjee, D. (2016). Sunspot Sizes and the Solar Cycle: Analysis Using Kodaikanal White-light Digitized Data, ApjL, 830:L33.Google Scholar
Mandal, S., Chatterjee, S., & Banerjee, D. (2017a). Solar Active Longitudes from Kodaikanal White-light Digitized Data, ApJ, 835:62.Google Scholar
Mandal, S., Hegde, M., Samanta, T., Hazra, G., Banerjee, D., & Ravindra, B. (2017b). Kodaikanal digitized white-light data archive (1921-2011): Analysis of various solar cycle features, A&A, 601:A106.Google Scholar
Ravindra, B., Priya, T. G., Amareswari, K., Priyal, M., Nazia, A. A. & Banerjee, D. (2013). Digitized archive of the Kodaikanal images: Representative results of solar cycle variation from sunspot area determination, ApJ, 550:A19.Google Scholar